diff --git a/Instrument/CDPP-AMDA/ARTEMIS/P1/Models.xml b/Instrument/CDPP-AMDA/ARTEMIS/P1/Models.xml
index 50f696c..5909ce7 100644
--- a/Instrument/CDPP-AMDA/ARTEMIS/P1/Models.xml
+++ b/Instrument/CDPP-AMDA/ARTEMIS/P1/Models.xml
@@ -5,16 +5,16 @@
spase://CNES/Instrument/CDPP-AMDA/ARTEMIS/P1/Models
Analytical Models
- ThemisB different magnetospheric analytical models
+ Artemis-P1 different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ Artemis-P1 different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
Platform
- ThemisB different magnetospheric analytical models
+ Artemis-P1 different magnetospheric analytical models
spase://CNES/Observatory/CDPP-AMDA/ARTEMIS/ArtemisP1
diff --git a/Instrument/CDPP-AMDA/ARTEMIS/P2/Models.xml b/Instrument/CDPP-AMDA/ARTEMIS/P2/Models.xml
index 755c0c3..cf6386f 100644
--- a/Instrument/CDPP-AMDA/ARTEMIS/P2/Models.xml
+++ b/Instrument/CDPP-AMDA/ARTEMIS/P2/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
Artemis-P2 different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ Artemis-P2 different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/Cluster1/Models.xml b/Instrument/CDPP-AMDA/Cluster1/Models.xml
index e534c11..ddd1d64 100644
--- a/Instrument/CDPP-AMDA/Cluster1/Models.xml
+++ b/Instrument/CDPP-AMDA/Cluster1/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
Mars crustal magnetic field analytical models
2017-02-04T15:37:46Z
- ToDo
+ Mars crustal magnetic field analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/Cluster2/Models.xml b/Instrument/CDPP-AMDA/Cluster2/Models.xml
index f2f5295..f4eb246 100644
--- a/Instrument/CDPP-AMDA/Cluster2/Models.xml
+++ b/Instrument/CDPP-AMDA/Cluster2/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
Cluster2 different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ Cluster2 different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/Cluster3/Models.xml b/Instrument/CDPP-AMDA/Cluster3/Models.xml
index f2a5f44..49778d8 100644
--- a/Instrument/CDPP-AMDA/Cluster3/Models.xml
+++ b/Instrument/CDPP-AMDA/Cluster3/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
Cluster3 different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ Cluster3 different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/Cluster4/Models.xml b/Instrument/CDPP-AMDA/Cluster4/Models.xml
index 7a555b7..51e81a8 100644
--- a/Instrument/CDPP-AMDA/Cluster4/Models.xml
+++ b/Instrument/CDPP-AMDA/Cluster4/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
Cluster4 different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ Cluster4 different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/Comets.xml b/Instrument/CDPP-AMDA/Comets.xml
index ea30ca0..0be74e7 100644
--- a/Instrument/CDPP-AMDA/Comets.xml
+++ b/Instrument/CDPP-AMDA/Comets.xml
@@ -6,7 +6,7 @@
Comets
2009-05-20T21:10:13Z
- ToDo
+ Comet Churyumov-Gerasimenko (C-G; P67) - Ephemeris
spase://CNES/Person/CDPP-AMDA/NAIF
PrincipalInvestigator
diff --git a/Instrument/CDPP-AMDA/Ephemerides.xml b/Instrument/CDPP-AMDA/Ephemerides.xml
index 73d492e..85d0e86 100644
--- a/Instrument/CDPP-AMDA/Ephemerides.xml
+++ b/Instrument/CDPP-AMDA/Ephemerides.xml
@@ -6,7 +6,7 @@
Planets and Moons
2009-05-20T21:10:13Z
- ToDo
+ Planets/Moons Orbitography
spase://CNES/Person/CDPP-AMDA/NAIF
PrincipalInvestigator
diff --git a/Instrument/CDPP-AMDA/Geotail/Models.xml b/Instrument/CDPP-AMDA/Geotail/Models.xml
index 9025abb..9985aba 100644
--- a/Instrument/CDPP-AMDA/Geotail/Models.xml
+++ b/Instrument/CDPP-AMDA/Geotail/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
Geotail different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ Geotail different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/Giotto/JPA.xml b/Instrument/CDPP-AMDA/Giotto/JPA.xml
index 59750a2..013ec26 100644
--- a/Instrument/CDPP-AMDA/Giotto/JPA.xml
+++ b/Instrument/CDPP-AMDA/Giotto/JPA.xml
@@ -7,7 +7,7 @@
JPA
Johnstone Plasma Analyser
2009-05-20T21:10:13Z
- ToDo
+ One of two plasma experiments to study the solar wind and charged particles. This instrument measures the three-dimensional energy distribution of positive ions in order to study the interaction between the solar wind and ionised cometary particles.
spase://SMWG/Person/Alan.D.Johnstone
PrincipalInvestigator
diff --git a/Instrument/CDPP-AMDA/Giotto/MAG.xml b/Instrument/CDPP-AMDA/Giotto/MAG.xml
index c711665..016cc6c 100644
--- a/Instrument/CDPP-AMDA/Giotto/MAG.xml
+++ b/Instrument/CDPP-AMDA/Giotto/MAG.xml
@@ -6,7 +6,7 @@
MAG
2009-05-20T21:10:13Z
- ToDo
+ Investigation of the interaction between Comet Halley and the solar wind during the encounter, as well as a study of the interplanetary magnetic field.
spase://SMWG/Person/Fritz.M.Neubauer
PrincipalInvestigator
diff --git a/Instrument/CDPP-AMDA/Giotto/RPA.xml b/Instrument/CDPP-AMDA/Giotto/RPA.xml
index 90ab888..d820a8b 100644
--- a/Instrument/CDPP-AMDA/Giotto/RPA.xml
+++ b/Instrument/CDPP-AMDA/Giotto/RPA.xml
@@ -7,7 +7,8 @@
RPA
Reme Copernic Plasma Experiment
2009-05-20T21:10:13Z
- ToDo
+ One of two plasma experiments to study the solar wind and charged particles.
+ The RPA measured velocity distributions of electrons and composition/distribution of thermal positive ions close to the cometary object.
spase://SMWG/Person/Henri.Reme
PrincipalInvestigator
diff --git a/Instrument/CDPP-AMDA/ICE/MAG.xml b/Instrument/CDPP-AMDA/ICE/MAG.xml
index 67d5142..6f2e264 100644
--- a/Instrument/CDPP-AMDA/ICE/MAG.xml
+++ b/Instrument/CDPP-AMDA/ICE/MAG.xml
@@ -5,8 +5,15 @@
spase://CNES/Instrument/CDPP-AMDA/ICE/MAG
MAG
+ Vector Helium Magnetometer
2009-05-20T21:10:13Z
- ToDo
+ The vector helium magnetometer is mounted on the end of a 3 m boom and makes in-situ measurements of
+ the ambient magnetic field vector in the frequency range 0-3 Hz. The instrument automatically chooses
+ one of eight ranges in which to operate, the four lowest full-scale ranges being +/-4, +/- 14, +/-42,
+ and +/- 146 nT. The precision of measurement is 1/256 of the full-scale field values (0.016, 0.055nT, etc.). The absolute accuracy is limited by
+ knowledge of the spacecraft magnetic field, which is presently known to better than 0.1 nT. The time
+ resolution corresponds to three triaxial samples per second at 1024 bit/s . The magnetometer contains a three- channel spectrum analyzer which
+ is connected to the search-coil sensor of the plasma- wave investigation.
spase://SMWG/Person/Edward.J.Smith
PrincipalInvestigator
diff --git a/Instrument/CDPP-AMDA/Interball-1/Models.xml b/Instrument/CDPP-AMDA/Interball-1/Models.xml
index 26e5717..5a48024 100644
--- a/Instrument/CDPP-AMDA/Interball-1/Models.xml
+++ b/Instrument/CDPP-AMDA/Interball-1/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
Interball-1 different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ Interball-1 different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/MAVEN/Models.xml b/Instrument/CDPP-AMDA/MAVEN/Models.xml
index 78c635e..b28cf75 100644
--- a/Instrument/CDPP-AMDA/MAVEN/Models.xml
+++ b/Instrument/CDPP-AMDA/MAVEN/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
MAVEN : Mars crustal magnetic field analytical models
2017-02-04T15:37:46Z
- ToDo
+ MAVEN : Mars crustal magnetic field analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/MEX/Models.xml b/Instrument/CDPP-AMDA/MEX/Models.xml
index 8904c31..5de3617 100644
--- a/Instrument/CDPP-AMDA/MEX/Models.xml
+++ b/Instrument/CDPP-AMDA/MEX/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
MEX : Mars crustal magnetic field analytical models
2017-02-04T15:37:46Z
- ToDo
+ MEX : Mars crustal magnetic field analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/MGS/Models.xml b/Instrument/CDPP-AMDA/MGS/Models.xml
index 4a85fdb..ca04acf 100644
--- a/Instrument/CDPP-AMDA/MGS/Models.xml
+++ b/Instrument/CDPP-AMDA/MGS/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
MGS : Mars crustal magnetic field analytical models
2017-02-04T15:37:46Z
- ToDo
+ MGS : Mars crustal magnetic field analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/MMS1/Models.xml b/Instrument/CDPP-AMDA/MMS1/Models.xml
index bfaf5cc..b66bc10 100644
--- a/Instrument/CDPP-AMDA/MMS1/Models.xml
+++ b/Instrument/CDPP-AMDA/MMS1/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
MMS1 different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ MMS1 different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/MMS2/Models.xml b/Instrument/CDPP-AMDA/MMS2/Models.xml
index 25a091d..dcc7966 100644
--- a/Instrument/CDPP-AMDA/MMS2/Models.xml
+++ b/Instrument/CDPP-AMDA/MMS2/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
MMS2 different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ MMS2 different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/MMS3/Models.xml b/Instrument/CDPP-AMDA/MMS3/Models.xml
index e84bb03..3e1835c 100644
--- a/Instrument/CDPP-AMDA/MMS3/Models.xml
+++ b/Instrument/CDPP-AMDA/MMS3/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
MMS3 different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ MMS3 different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/MMS4/Models.xml b/Instrument/CDPP-AMDA/MMS4/Models.xml
index c869fe1..1adbfa5 100644
--- a/Instrument/CDPP-AMDA/MMS4/Models.xml
+++ b/Instrument/CDPP-AMDA/MMS4/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
MMS4 different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ MMS4 different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/POLAR/Models.xml b/Instrument/CDPP-AMDA/POLAR/Models.xml
index 4145976..7e8c10b 100644
--- a/Instrument/CDPP-AMDA/POLAR/Models.xml
+++ b/Instrument/CDPP-AMDA/POLAR/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
Polar different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ Polar different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/Phobos2/MAG.xml b/Instrument/CDPP-AMDA/Phobos2/MAG.xml
index 0a3a1ea..cc37d7f 100644
--- a/Instrument/CDPP-AMDA/Phobos2/MAG.xml
+++ b/Instrument/CDPP-AMDA/Phobos2/MAG.xml
@@ -7,7 +7,8 @@
MAG
MAGMA
2019-11-18T16:00:05Z
- ToDo
+ The magnetometers on board the Phobos 2 spacecraft provided the opportunity to study the magnetic environment around Mars,
+ including regions which have never been explored before, such as at low altitudes (down to 850 km above the surface of Mars) and in the tail.
spase://SMWG/Person/Konrad.Schwingenschuh
PrincipalInvestigator
diff --git a/Instrument/CDPP-AMDA/Pioneer10/CPI.xml b/Instrument/CDPP-AMDA/Pioneer10/CPI.xml
index b3cd919..5a64c6e 100644
--- a/Instrument/CDPP-AMDA/Pioneer10/CPI.xml
+++ b/Instrument/CDPP-AMDA/Pioneer10/CPI.xml
@@ -7,7 +7,13 @@
CPI
Charged Particle Instrument
2009-05-20T21:10:13Z
- ToDo
+ This experiment (carried also on Pioneer 11) measured charged-particle composition and spectra using four detector systems:
+ (1) the main telescope, consisting of seven elements and providing energy spectra (approximately 3 to 68 MeV for protons and 10 to 150 MeV/nucleon for oxygen), element resolution (through oxygen), and isotope resolution (for H and He);
+ (2) the low-energy subsystem telescope, consisting of two elements and using a very small thin first element to extend the high-sensitivity proton measurements below 1 MeV (0.3 to 9 MeV) in the presence of a high gamma-ray background aboard the spacecraft;
+ (3) the electron-current detector (ECG), consisting of a beryllium-shield silicon detector operated in current mode to measure high fluxes of electrons with energies above 3 MeV; and
+ (4) the fission cell detector, recording fission fragments from the nucleon-induced fission of thorium 232 sandwiched between two large-area silicon detectors to measure fluxes of protons (above 30 MeV) in the presence of high fluxes of electrons.
+
+ The experiment sample time was synchronized with the spacecraft spin, permitting sectoring of the readout of the main and low-energy telescopes into eight octants about the spin axis. Data also include the interplanetary region.
spase://SMWG/Person/John.A.Simpson
PrincipalInvestigator
diff --git a/Instrument/CDPP-AMDA/Pioneer11/CPI.xml b/Instrument/CDPP-AMDA/Pioneer11/CPI.xml
index e19512d..014c8e8 100644
--- a/Instrument/CDPP-AMDA/Pioneer11/CPI.xml
+++ b/Instrument/CDPP-AMDA/Pioneer11/CPI.xml
@@ -7,7 +7,13 @@
CPI
Charged Particle Instrument
2009-05-20T21:10:13Z
- ToDo
+ This experiment (carried also on Pioneer 10) measured charged-particle composition and spectra using four detector systems:
+ (1) the main telescope, consisting of seven elements and providing energy spectra (approximately 3 to 68 MeV for protons and 10 to 150 MeV/nucleon for oxygen), element resolution (through oxygen), and isotope resolution (for H and He);
+ (2) the low-energy subsystem telescope, consisting of two elements and using a very small thin first element to extend the high-sensitivity proton measurements below 1 MeV (0.3 to 9 MeV) in the presence of a high gamma-ray background aboard the spacecraft;
+ (3) the electron-current detector (ECG), consisting of a beryllium-shield silicon detector operated in current mode to measure high fluxes of electrons with energies above 3 MeV; and
+ (4) the fission cell detector, recording fission fragments from the nucleon-induced fission of thorium 232 sandwiched between two large-area silicon detectors to measure fluxes of protons (above 30 MeV) in the presence of high fluxes of electrons.
+
+ The experiment sample time was synchronized with the spacecraft spin, permitting sectoring of the readout of the main and low-energy telescopes into eight octants about the spin axis. Data also include the interplanetary region.
spase://SMWG/Person/John.A.Simpson
PrincipalInvestigator
diff --git a/Instrument/CDPP-AMDA/SWARM-A/GNSS.xml b/Instrument/CDPP-AMDA/SWARM-A/GNSS.xml
index 711efcc..e291ba9 100644
--- a/Instrument/CDPP-AMDA/SWARM-A/GNSS.xml
+++ b/Instrument/CDPP-AMDA/SWARM-A/GNSS.xml
@@ -7,7 +7,7 @@
GNSS
Global Navigation Satellite System
2016-11-04T15:37:46Z
- ToDo
+ Global Navigation Satellite System
spase://CNES/Person/CDPP-AMDA/R.Haagmans
ProjectScientist
diff --git a/Instrument/CDPP-AMDA/SWARM-B/GNSS.xml b/Instrument/CDPP-AMDA/SWARM-B/GNSS.xml
index 323b133..4c56b24 100644
--- a/Instrument/CDPP-AMDA/SWARM-B/GNSS.xml
+++ b/Instrument/CDPP-AMDA/SWARM-B/GNSS.xml
@@ -7,7 +7,7 @@
GNSS
Global Navigation Satellite System
2016-11-04T15:37:46Z
- ToDo
+ Global Navigation Satellite System
spase://CNES/Person/CDPP-AMDA/R.Haagmans
ProjectScientist
diff --git a/Instrument/CDPP-AMDA/SWARM-C/GNSS.xml b/Instrument/CDPP-AMDA/SWARM-C/GNSS.xml
index 057b907..c578a62 100644
--- a/Instrument/CDPP-AMDA/SWARM-C/GNSS.xml
+++ b/Instrument/CDPP-AMDA/SWARM-C/GNSS.xml
@@ -7,7 +7,7 @@
GNSS
Global Navigation Satellite System
2016-11-04T15:37:46Z
- ToDo
+ Global Navigation Satellite System
spase://CNES/Person/CDPP-AMDA/R.Haagmans
ProjectScientist
diff --git a/Instrument/CDPP-AMDA/THEMIS/A/Models.xml b/Instrument/CDPP-AMDA/THEMIS/A/Models.xml
index da77cf6..dea5538 100644
--- a/Instrument/CDPP-AMDA/THEMIS/A/Models.xml
+++ b/Instrument/CDPP-AMDA/THEMIS/A/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
ThemisA different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ ThemisA different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/THEMIS/B/Models.xml b/Instrument/CDPP-AMDA/THEMIS/B/Models.xml
index 56841db..1ab89ce 100644
--- a/Instrument/CDPP-AMDA/THEMIS/B/Models.xml
+++ b/Instrument/CDPP-AMDA/THEMIS/B/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
ThemisB different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ ThemisB different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/THEMIS/C/Models.xml b/Instrument/CDPP-AMDA/THEMIS/C/Models.xml
index f68d1fd..3a6e9a3 100644
--- a/Instrument/CDPP-AMDA/THEMIS/C/Models.xml
+++ b/Instrument/CDPP-AMDA/THEMIS/C/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
ThemisC different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ ThemisC different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/THEMIS/D/Models.xml b/Instrument/CDPP-AMDA/THEMIS/D/Models.xml
index 0a14a98..c0f5328 100644
--- a/Instrument/CDPP-AMDA/THEMIS/D/Models.xml
+++ b/Instrument/CDPP-AMDA/THEMIS/D/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
ThemisD different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ ThemisD different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/Instrument/CDPP-AMDA/THEMIS/E/Models.xml b/Instrument/CDPP-AMDA/THEMIS/E/Models.xml
index fc0e138..a17ee49 100644
--- a/Instrument/CDPP-AMDA/THEMIS/E/Models.xml
+++ b/Instrument/CDPP-AMDA/THEMIS/E/Models.xml
@@ -7,7 +7,7 @@
Analytical Models
ThemisE different magnetospheric analytical models
2017-02-04T15:37:46Z
- ToDo
+ ThemisE different magnetospheric analytical models
spase://SMWG/Person/Christian.Jacquey
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/ACE/MFI/ace-mag-real.xml b/NumericalData/CDPP-AMDA/ACE/MFI/ace-mag-real.xml
index 565e5ca..225fbd1 100644
--- a/NumericalData/CDPP-AMDA/ACE/MFI/ace-mag-real.xml
+++ b/NumericalData/CDPP-AMDA/ACE/MFI/ace-mag-real.xml
@@ -6,7 +6,7 @@
real time
Interplanetary Magnetic Field 60-sec real time Data
- 2024-05-22T09:07:09Z
+ 2024-05-23T07:07:27Z
ACE Magnetometer real time, 60-second averages of field magnitude and vectors in GSE and GSM coordinates systems.
@@ -66,7 +66,7 @@
2024-01-15T00:00:00Z
- 2024-05-22T08:59:59Z
+ 2024-05-23T06:59:59Z
PT60S
diff --git a/NumericalData/CDPP-AMDA/ACE/SWEPAM/ace-swepam-real.xml b/NumericalData/CDPP-AMDA/ACE/SWEPAM/ace-swepam-real.xml
index 5847817..ac6e0f6 100644
--- a/NumericalData/CDPP-AMDA/ACE/SWEPAM/ace-swepam-real.xml
+++ b/NumericalData/CDPP-AMDA/ACE/SWEPAM/ace-swepam-real.xml
@@ -6,7 +6,7 @@
sw : real time
Solar wind 60-sec real time data
- 2024-05-22T09:04:00Z
+ 2024-05-23T07:04:14Z
The ram pressure is calculated using P=rho*Np*Vp², where rho=1.672622*(1+4*(1/(1-He++_ratio)-1)).
We use rho=2 here, which corresponds to a ratio of He++ between 4% and 5%.
@@ -63,7 +63,7 @@
2024-01-15T00:00:00Z
- 2024-05-22T07:59:59Z
+ 2024-05-23T05:59:59Z
PT60S
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2e.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2e.xml
index f7eb779..a55a46c 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2e.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2e.xml
@@ -5,8 +5,8 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2e
electron full mode
- 2024-05-22T02:00:23Z
- ToDo
+ 2024-05-23T02:00:23Z
+ Electrostatic Analyzer (ESA) data - Level 2 - electron full mode
spase://SMWG/Person/Elena.Budnik
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2i.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2i.xml
index 1b2cd89..bca873c 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2i.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2i.xml
@@ -5,7 +5,7 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-esa-l2i
ion full mode
- 2024-05-22T02:00:23Z
+ 2024-05-23T02:00:23Z
"Full Mode" is a low-time-resolution data product useful for large-scale surveys of THEMIS data. It generally maintains the "full" 32 energies sampled, and have an 88 solid-angle map. Full distribution data are 1-spin snapshots of the plasma with a measurement cadence of either 32 spins (in "Fast-Survey Spacecraft Mode") or 128 spins ("Slow-Survey Spacecraft Mode").>
spase://SMWG/Person/Charles.W.Carlson
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peem-all.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peem-all.xml
index a5d9b0c..4c65d39 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peem-all.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peem-all.xml
@@ -5,8 +5,8 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peem-all
electron onboard moments
- 2024-05-22T02:01:22Z
- ToDo
+ 2024-05-23T02:01:21Z
+ Electrostatic Analyzer (ESA) data - Level 2 - electron onboard moments
spase://SMWG/Person/Vassilis.Angelopoulos
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peim-all.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peim-all.xml
index af31dec..87bf126 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peim-all.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peim-all.xml
@@ -5,8 +5,8 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/ESA/athp1-peim-all
ion onboard moments
- 2024-05-22T02:01:22Z
- ToDo
+ 2024-05-23T02:01:21Z
+ Electrostatic Analyzer (ESA) data - Level 2 - ion onboard moments
spase://SMWG/Person/Vassilis.Angelopoulos
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P1/Ephemeris/athp1-orb-all.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P1/Ephemeris/athp1-orb-all.xml
index 30ad35d..f6cb310 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P1/Ephemeris/athp1-orb-all.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P1/Ephemeris/athp1-orb-all.xml
@@ -5,7 +5,7 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/Ephemeris/athp1-orb-all
orbit
- 2024-05-22T02:03:30Z
+ 2024-05-23T02:03:23Z
ARTEMIS P1 ephemeris
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-l.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-l.xml
index 419c5c5..e16fca7 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-l.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-l.xml
@@ -5,8 +5,8 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-l
0.25 sec (low)
- 2024-05-22T02:03:30Z
- ToDo
+ 2024-05-23T02:03:23Z
+ Fluxgate Magnetometer (FGM) data - Level 2 - FGL (low-resolution) magnetic field
spase://SMWG/Person/Uli.Auster
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-s.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-s.xml
index 0a768bb..d5dbb1a 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-s.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-s.xml
@@ -5,8 +5,8 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P1/FGM/athp1-fgm-s
3 sec (spin)
- 2024-05-22T02:03:32Z
- ToDo
+ 2024-05-23T02:03:26Z
+ Fluxgate Magnetometer (FGM) data - Level 2 - FGS (spin-resolution) magnetic field
spase://SMWG/Person/Uli.Auster
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2e.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2e.xml
index 89d951b..f484629 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2e.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2e.xml
@@ -5,8 +5,8 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2e
electron full mode
- 2024-05-22T02:00:29Z
- ToDo
+ 2024-05-23T02:00:29Z
+ Electrostatic Analyzer (ESA) data - Level 2 - electron full mode
spase://SMWG/Person/Elena.Budnik
TechnicalContact
@@ -48,7 +48,7 @@
2011-07-17T00:00:00Z
- 2024-05-18T22:01:44Z
+ 2024-05-20T16:42:11Z
PT96.27S
PT551.0S
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2i.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2i.xml
index f5e8673..98abe5b 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2i.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2i.xml
@@ -5,7 +5,7 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-esa-l2i
ion full mode
- 2024-05-22T02:00:28Z
+ 2024-05-23T02:00:29Z
"Full Mode" is a low-time-resolution data product useful for large-scale surveys of THEMIS data. It generally maintains the "full" 32 energies sampled, and have an 88 solid-angle map. Full distribution data are 1-spin snapshots of the plasma with a measurement cadence of either 32 spins (in "Fast-Survey Spacecraft Mode") or 128 spins ("Slow-Survey Spacecraft Mode").
spase://SMWG/Person/Charles.W.Carlson
@@ -52,7 +52,7 @@
2011-07-17T00:00:00Z
- 2024-05-18T22:00:05Z
+ 2024-05-20T16:43:25Z
PT96.27S
PT551.0S
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peem-all.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peem-all.xml
index 14641a0..7966c6b 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peem-all.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peem-all.xml
@@ -5,8 +5,8 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peem-all
electron onboard moments
- 2024-05-22T02:01:33Z
- ToDo
+ 2024-05-23T02:01:31Z
+ Electrostatic Analyzer (ESA) data - Level 2 - electron onboard moments
spase://SMWG/Person/Vassilis.Angelopoulos
PrincipalInvestigator
@@ -48,7 +48,7 @@
2011-07-17T00:00:00Z
- 2024-05-18T21:54:28Z
+ 2024-05-19T00:00:29Z
PT3S
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peim-all.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peim-all.xml
index 86b53a0..805166b 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peim-all.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peim-all.xml
@@ -5,8 +5,8 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/ESA/athp2-peim-all
ion onboard moments
- 2024-05-22T02:01:32Z
- ToDo
+ 2024-05-23T02:01:30Z
+ Electrostatic Analyzer (ESA) data - Level 2 - ion onboard moments
spase://SMWG/Person/Vassilis.Angelopoulos
PrincipalInvestigator
@@ -48,7 +48,7 @@
2011-07-17T00:00:00Z
- 2024-05-18T21:54:28Z
+ 2024-05-19T00:00:29Z
PT3S
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-l.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-l.xml
index a04fd75..43d3beb 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-l.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-l.xml
@@ -5,8 +5,8 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-l
0.25 sec (low)
- 2024-05-22T02:03:48Z
- ToDo
+ 2024-05-23T02:03:39Z
+ Fluxgate Magnetometer (FGM) data - Level 2 - FGL (low-resolution) magnetic field
spase://SMWG/Person/Uli.Auster
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-s.xml b/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-s.xml
index a77a80e..f58dfff 100644
--- a/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-s.xml
+++ b/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-s.xml
@@ -5,8 +5,8 @@
spase://CNES/NumericalData/CDPP-AMDA/ARTEMIS/P2/FGM/athp2-fgm-s
3 sec (spin)
- 2024-05-22T02:03:50Z
- ToDo
+ 2024-05-23T02:03:42Z
+ Fluxgate Magnetometer (FGM) data - Level 2 - FGS (spin-resolution) magnetic field
spase://SMWG/Person/Uli.Auster
TechnicalContact
@@ -47,7 +47,7 @@
2011-07-17T00:00:00Z
- 2024-05-18T18:17:41Z
+ 2024-05-19T00:02:50Z
PT4S
diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MGF/bepi-mgf-venus2.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MGF/bepi-mgf-venus2.xml
index dfd7b46..b6ee884 100644
--- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MGF/bepi-mgf-venus2.xml
+++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MGF/bepi-mgf-venus2.xml
@@ -6,7 +6,9 @@
Venus flyby #2
2021-10-12T14:05:27Z
- ToDo
+ The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath from the nightside down to the almost unexplored subsolar region.
+
+Magnetic field.
spase://SMWG/Person/Wolfgang.Baumjohann
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/Cluster/Cluster1/RAPID/clust1-rap-elsp.xml b/NumericalData/CDPP-AMDA/Cluster/Cluster1/RAPID/clust1-rap-elsp.xml
index 8e1f7b4..5e4aab9 100644
--- a/NumericalData/CDPP-AMDA/Cluster/Cluster1/RAPID/clust1-rap-elsp.xml
+++ b/NumericalData/CDPP-AMDA/Cluster/Cluster1/RAPID/clust1-rap-elsp.xml
@@ -7,7 +7,7 @@
prime parameters : electrons
Cluster 1 Prime Parameter RAPID Data
2012-03-06T17:14:59Z
- ToDo
+ Prime Parameters RAPID Electron Data
spase://SMWG/Person/Peter.W.Daly
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/Cluster/Cluster1/RAPID/clust1-rap-psp.xml b/NumericalData/CDPP-AMDA/Cluster/Cluster1/RAPID/clust1-rap-psp.xml
index bb60bc7..9b08995 100644
--- a/NumericalData/CDPP-AMDA/Cluster/Cluster1/RAPID/clust1-rap-psp.xml
+++ b/NumericalData/CDPP-AMDA/Cluster/Cluster1/RAPID/clust1-rap-psp.xml
@@ -7,7 +7,7 @@
prime parameters : protons
Cluster 1 Prime Parameter RAPID Data
2012-03-06T17:15:38Z
- ToDo
+ Prime Parameters RAPID Protons Data
spase://SMWG/Person/Peter.W.Daly
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-elsp.xml b/NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-elsp.xml
index 493f8ef..ca02dd6 100644
--- a/NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-elsp.xml
+++ b/NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-elsp.xml
@@ -7,7 +7,7 @@
prime parameters : electrons
Cluster 2 Prime Parameter RAPID Data
2012-03-06T19:01:05Z
- ToDo
+ Prime Parameters RAPID Electron Data
spase://SMWG/Person/Peter.W.Daly
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp.xml b/NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp.xml
index 00ac435..d82b42f 100644
--- a/NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp.xml
+++ b/NumericalData/CDPP-AMDA/Cluster/Cluster2/RAPID/clust2-rap-psp.xml
@@ -7,13 +7,7 @@
prime parameters : protons
Cluster 2 Prime Parameter RAPID Data
2012-03-06T19:01:43Z
- The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging
- Detectors) analyzes suprathermal plasma distributions in the energy range from 20-400 KeV
- for electrons and from 2 KeV/nucleon to 1.50 MeV/nucleon for ions. For more details of the
- Cluster mission, the spacecraft, and its instruments, see the report Cluster: mission,
- payload and supporting activities, March 1993, ESA SP-1159, and the included article RAPID:
- The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which
- this information was obtained.
+ Prime Parameters RAPID Protons Data
spase://SMWG/Person/Peter.W.Daly
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/Cluster/Cluster3/RAPID/clust3-rap-elsp.xml b/NumericalData/CDPP-AMDA/Cluster/Cluster3/RAPID/clust3-rap-elsp.xml
index a0fb0d4..296964a 100644
--- a/NumericalData/CDPP-AMDA/Cluster/Cluster3/RAPID/clust3-rap-elsp.xml
+++ b/NumericalData/CDPP-AMDA/Cluster/Cluster3/RAPID/clust3-rap-elsp.xml
@@ -7,7 +7,7 @@
electrons
Cluster 3 Prime Parameter RAPID Data
2012-03-06T16:11:35Z
- ToDo
+ Prime Parameters RAPID Electron Data
spase://SMWG/Person/Peter.W.Daly
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/Cluster/Cluster3/RAPID/clust3-rap-psp.xml b/NumericalData/CDPP-AMDA/Cluster/Cluster3/RAPID/clust3-rap-psp.xml
index 75cfafd..d2a8444 100644
--- a/NumericalData/CDPP-AMDA/Cluster/Cluster3/RAPID/clust3-rap-psp.xml
+++ b/NumericalData/CDPP-AMDA/Cluster/Cluster3/RAPID/clust3-rap-psp.xml
@@ -7,7 +7,7 @@
protons
Cluster 3 Prime Parameter RAPID Data
2012-03-06T16:12:23Z
- ToDo
+ Prime Parameters RAPID Protons Data
spase://SMWG/Person/Peter.W.Daly
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/Cluster/Cluster4/RAPID/clust4-rap-elsp.xml b/NumericalData/CDPP-AMDA/Cluster/Cluster4/RAPID/clust4-rap-elsp.xml
index ced0cf4..0eb8c02 100644
--- a/NumericalData/CDPP-AMDA/Cluster/Cluster4/RAPID/clust4-rap-elsp.xml
+++ b/NumericalData/CDPP-AMDA/Cluster/Cluster4/RAPID/clust4-rap-elsp.xml
@@ -7,7 +7,7 @@
electrons
Cluster 4 Prime Parameter RAPID Data
2012-03-06T19:39:56Z
- ToDo
+ Prime Parameters RAPID Electron Data
spase://SMWG/Person/Peter.W.Daly
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp.xml b/NumericalData/CDPP-AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp.xml
index 3957d54..a311442 100644
--- a/NumericalData/CDPP-AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp.xml
+++ b/NumericalData/CDPP-AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp.xml
@@ -7,7 +7,7 @@
protons
Cluster 4 Prime Parameter RAPID Data
2012-03-06T19:40:38Z
- ToDo
+ Prime Parameters RAPID Protons Data
spase://SMWG/Person/Peter.W.Daly
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-1m.xml b/NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-1m.xml
index 92eacc4..805da85 100644
--- a/NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-1m.xml
+++ b/NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-1m.xml
@@ -6,7 +6,7 @@
sw : 1 m
solar wind parameters
- 2024-05-22T02:12:40Z
+ 2024-05-23T02:12:59Z
Faraday Cup (FC) measures the solar wind bulk properties (wind speed, density and temperature).
The ram pressure is calculated using P=rho*Np*Vp², where rho=1.672622*(1+4*(1/(1-He++_ratio)-1)).
We use rho=2 here, which corresponds to a ratio of He++ between 4% and 5%.
@@ -61,7 +61,7 @@
2016-08-01T00:00:00Z
- 2024-05-20T23:59:00Z
+ 2024-05-21T23:59:00Z
PT60S
diff --git a/NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-3s.xml b/NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-3s.xml
index eff3f8b..12a9b8d 100644
--- a/NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-3s.xml
+++ b/NumericalData/CDPP-AMDA/DSCOVR/FC/dsc-fc-3s.xml
@@ -6,7 +6,7 @@
sw : 3 s
solar wind parameters
- 2024-05-22T02:14:11Z
+ 2024-05-23T02:14:27Z
Faraday Cup (FC) measures the solar wind bulk properties (wind speed, density and temperature).
The ram pressure is calculated using P=rho*Np*Vp², where rho=1.672622*(1+4*(1/(1-He++_ratio)-1)).
We use rho=2 here, which corresponds to a ratio of He++ between 4% and 5%.
@@ -61,7 +61,7 @@
2016-08-01T00:00:00Z
- 2024-05-20T23:59:40Z
+ 2024-05-21T23:59:40Z
PT3S
diff --git a/NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1m.xml b/NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1m.xml
index bb106ae..a454ed7 100644
--- a/NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1m.xml
+++ b/NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1m.xml
@@ -6,7 +6,7 @@
1 m
interplanetary magnetic field
- 2024-05-22T02:06:13Z
+ 2024-05-23T02:06:26Z
Solar wind magnetic field vector (sampling 60s)
NOAA Space Weather Prediction Center (2016): Deep Space Climate Observatory (DSCOVR). NOAA National Centers for Environmental Information.
@@ -60,7 +60,7 @@
2016-08-01T00:00:00Z
- 2024-05-20T23:59:00Z
+ 2024-05-21T23:59:00Z
PT60S
diff --git a/NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1s.xml b/NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1s.xml
index 975e5e5..6b3b638 100644
--- a/NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1s.xml
+++ b/NumericalData/CDPP-AMDA/DSCOVR/MAG/dsc-mag-1s.xml
@@ -6,7 +6,7 @@
1 s
interplanetary magnetic field
- 2024-05-22T02:11:27Z
+ 2024-05-23T02:11:47Z
Solar wind magnetic field vector (sampling 1s)
NOAA Space Weather Prediction Center (2016): Deep Space Climate Observatory (DSCOVR). NOAA National Centers for Environmental Information.
@@ -58,7 +58,7 @@
2016-08-01T00:00:00Z
- 2024-05-20T23:59:59Z
+ 2024-05-21T23:59:59Z
PT60S
diff --git a/NumericalData/CDPP-AMDA/Ephemerides/mars-deimos-orb.xml b/NumericalData/CDPP-AMDA/Ephemerides/mars-deimos-orb.xml
index 609754b..26f9ea2 100644
--- a/NumericalData/CDPP-AMDA/Ephemerides/mars-deimos-orb.xml
+++ b/NumericalData/CDPP-AMDA/Ephemerides/mars-deimos-orb.xml
@@ -6,7 +6,7 @@
Deimos
2022-03-10T10:35:55Z
- ToDo
+ Deimos is the smaller and outer of the two natural satellites of Mars.
spase://CNES/Person/CDPP-AMDA/NAIF
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/Ephemerides/mars-phobos-orb.xml b/NumericalData/CDPP-AMDA/Ephemerides/mars-phobos-orb.xml
index 302ae52..0bec8bd 100644
--- a/NumericalData/CDPP-AMDA/Ephemerides/mars-phobos-orb.xml
+++ b/NumericalData/CDPP-AMDA/Ephemerides/mars-phobos-orb.xml
@@ -6,7 +6,7 @@
Phobos - 1 min
2022-03-10T09:51:00Z
- ToDo
+ Phobos is the innermost and larger of the two natural satellites of Mars.
spase://CNES/Person/CDPP-AMDA/NAIF
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/Ephemerides/mars-phobos-orb1s.xml b/NumericalData/CDPP-AMDA/Ephemerides/mars-phobos-orb1s.xml
index 303c4bc..7ed3582 100644
--- a/NumericalData/CDPP-AMDA/Ephemerides/mars-phobos-orb1s.xml
+++ b/NumericalData/CDPP-AMDA/Ephemerides/mars-phobos-orb1s.xml
@@ -6,7 +6,7 @@
Phobos - 1 sec
2022-03-18T08:45:15Z
- ToDo
+ Phobos is the innermost and larger of the two natural satellites of Mars.
spase://CNES/Person/CDPP-AMDA/NAIF
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/Ephemerides/moon-earth-all.xml b/NumericalData/CDPP-AMDA/Ephemerides/moon-earth-all.xml
index 3a727fd..5b8b36c 100644
--- a/NumericalData/CDPP-AMDA/Ephemerides/moon-earth-all.xml
+++ b/NumericalData/CDPP-AMDA/Ephemerides/moon-earth-all.xml
@@ -6,7 +6,7 @@
Earth Moon
2019-08-23T15:34:00Z
- ToDo
+ The Moon is Earth's only natural satellite. It orbits at an average distance of 384,400 km (238,900 mi), about 30 times the diameter of Earth.
spase://CNES/Person/CDPP-AMDA/NAIF
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/Giotto/Ephemeris/gio-orb-comet.xml b/NumericalData/CDPP-AMDA/Giotto/Ephemeris/gio-orb-comet.xml
index a9a04b1..1e6f4fb 100644
--- a/NumericalData/CDPP-AMDA/Giotto/Ephemeris/gio-orb-comet.xml
+++ b/NumericalData/CDPP-AMDA/Giotto/Ephemeris/gio-orb-comet.xml
@@ -6,7 +6,7 @@
flyby comet/halley
2014-06-18T12:59:54Z
- ToDo
+ Giotto spacecraft positions in various coordinate systems
spase://SMWG/Person/Elena.Budnik
MetadataContact
diff --git a/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-a.xml b/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-a.xml
index 9411710..1f12292 100644
--- a/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-a.xml
+++ b/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-a.xml
@@ -7,7 +7,7 @@
alphas
HERS
2014-06-16T12:53:01Z
- ToDo
+ ION MASS SPECTROMETER - High-Energy Range Spectrometer - Alphas data
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-his.xml b/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-his.xml
index c3a760c..bda50f7 100644
--- a/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-his.xml
+++ b/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-his.xml
@@ -7,7 +7,7 @@
heavy ions countrate
HIS
2014-06-17T16:59:11Z
- ToDo
+ ION MASS SPECTROMETER - High Intensity Spectrometer - Heavy ions countrate data
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-p.xml b/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-p.xml
index 5f0fd34..f30651c 100644
--- a/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-p.xml
+++ b/NumericalData/CDPP-AMDA/Giotto/IMS/gio-ims-p.xml
@@ -7,7 +7,7 @@
protons
HERS
2014-06-16T12:46:56Z
- ToDo
+ ION MASS SPECTROMETER - High-Energy Range Spectrometer - Protons data
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Giotto/JPA/gio-jpa-psa.xml b/NumericalData/CDPP-AMDA/Giotto/JPA/gio-jpa-psa.xml
index a1044ed..42b5a66 100644
--- a/NumericalData/CDPP-AMDA/Giotto/JPA/gio-jpa-psa.xml
+++ b/NumericalData/CDPP-AMDA/Giotto/JPA/gio-jpa-psa.xml
@@ -6,7 +6,7 @@
protons
2014-06-13T14:06:35Z
- ToDo
+ Johnstone Plasma Analyser - protons data.
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Giotto/MAG/gio-mag-psa.xml b/NumericalData/CDPP-AMDA/Giotto/MAG/gio-mag-psa.xml
index 824fc2a..63f2f0b 100644
--- a/NumericalData/CDPP-AMDA/Giotto/MAG/gio-mag-psa.xml
+++ b/NumericalData/CDPP-AMDA/Giotto/MAG/gio-mag-psa.xml
@@ -6,7 +6,7 @@
magnetic field
2014-06-12T09:43:08Z
- ToDo
+ Giotto Magnetometer Experiment data
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Giotto/RPA/gio-rpa1-corr.xml b/NumericalData/CDPP-AMDA/Giotto/RPA/gio-rpa1-corr.xml
index 41e5bf3..a9742c9 100644
--- a/NumericalData/CDPP-AMDA/Giotto/RPA/gio-rpa1-corr.xml
+++ b/NumericalData/CDPP-AMDA/Giotto/RPA/gio-rpa1-corr.xml
@@ -6,7 +6,7 @@
density elec
2014-05-27T15:16:06Z
- ToDo
+ RPA-(Reme) Copernic Plasma Experiment - Eletrons density
spase://SMWG/Person/Elena.Budnik
MetadataContact
diff --git a/NumericalData/CDPP-AMDA/INTERBALL-Tail/CORALL/intt-crl-kp.xml b/NumericalData/CDPP-AMDA/INTERBALL-Tail/CORALL/intt-crl-kp.xml
index 152630d..6f78b9b 100644
--- a/NumericalData/CDPP-AMDA/INTERBALL-Tail/CORALL/intt-crl-kp.xml
+++ b/NumericalData/CDPP-AMDA/INTERBALL-Tail/CORALL/intt-crl-kp.xml
@@ -6,7 +6,7 @@
key parameters
2013-05-24T11:06:59Z
- ToDo
+ CORALL is the ion spectrometer with energy range 30eV - 25keV onboard INTERBALL/TAIL satellite. It has a fan-shape aperture wich plane has a sunward spin axis of spacecraft. The full distribution function is obtained for one spacecraft revolution. So for every revolution plasma parameters ( V, T, N) can be calculated.
spase://SMWG/Person/Andrey.Fedorov
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-1s.xml b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-1s.xml
index bfd5aea..86fde81 100644
--- a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-1s.xml
+++ b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-1s.xml
@@ -7,7 +7,7 @@
spectra : sunward
Electron Spectra : Sunward Flow
2004-12-16T17:44:55Z
- ToDo
+ DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.
spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-1t.xml b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-1t.xml
index 3878769..5fdb8a9 100644
--- a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-1t.xml
+++ b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-1t.xml
@@ -7,7 +7,7 @@
time profiles : sunward
Electron Time Profiles : Sunward Flow
2004-12-02T19:47:03Z
- ToDo
+ DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.
spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-2s.xml b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-2s.xml
index 82a7c21..11f1671 100644
--- a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-2s.xml
+++ b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-2s.xml
@@ -7,7 +7,7 @@
spectra : tailward
Electron Spectra : Tailward Flow
2004-12-16T16:51:20Z
- ToDo
+ DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.
spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-2t.xml b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-2t.xml
index 91995a4..a222ed7 100644
--- a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-2t.xml
+++ b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-2t.xml
@@ -7,7 +7,7 @@
time profiles : tailward
Electron Time Profiles : Tailward Flow
2004-12-02T14:45:57Z
- ToDo
+ DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.
spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-3s.xml b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-3s.xml
index 37190c7..2b0b84d 100644
--- a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-3s.xml
+++ b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-3s.xml
@@ -7,7 +7,7 @@
spectra : sunward
Ion Spectra : Sunward Flow
2004-12-16T17:45:33Z
- ToDo
+ DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.
spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-3t.xml b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-3t.xml
index 9f11454..8e78375 100644
--- a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-3t.xml
+++ b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-3t.xml
@@ -7,7 +7,7 @@
time profiles : sunward
Ion Time Profiles : Sunward Flow
2004-12-02T19:48:02Z
- ToDo
+ DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.
spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-4s.xml b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-4s.xml
index 1445a1c..bc6b7ed 100644
--- a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-4s.xml
+++ b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-4s.xml
@@ -7,7 +7,7 @@
spectra : tailward
Ion Spectra : Tailward Flow
2004-12-16T17:46:24Z
- ToDo
+ DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.
spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-4t.xml b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-4t.xml
index 253b797..8bda978 100644
--- a/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-4t.xml
+++ b/NumericalData/CDPP-AMDA/INTERBALL-Tail/DOK2/iball-dok-4t.xml
@@ -7,7 +7,7 @@
time profiles : tailward
Ion Time Profiles : Tailward Flow
2004-12-02T19:49:42Z
- ToDo
+ DOK2 is solid state spectrometer measuring ions in the energy range 20 keV - 750 keV and electrons in the energy range 30 keV - 400 keV. DOK2 includes two detectors - one looks tailward, the other one looks most of the time at 62 deg to spin axis of satellite.
spase://CNES/Person/CDPP-AMDA/Volt.Lutsenko
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/INTERBALL-Tail/MIF-FM/iball-mif-hr.xml b/NumericalData/CDPP-AMDA/INTERBALL-Tail/MIF-FM/iball-mif-hr.xml
index f99963f..c05e96c 100644
--- a/NumericalData/CDPP-AMDA/INTERBALL-Tail/MIF-FM/iball-mif-hr.xml
+++ b/NumericalData/CDPP-AMDA/INTERBALL-Tail/MIF-FM/iball-mif-hr.xml
@@ -6,7 +6,7 @@
high resolution
2020-07-10T10:55:42Z
- ToDo
+ This data set contains the DC/AC Magnetic Field (0-64 Hz and 1 Hz - 40 kHz) in GSM from the MIF-M magnetometer on board Interball-Tail.
spase://SMWG/Person/Stanislav.A.Romanov
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/INTERBALL-Tail/MIF-FM/intt-fm-kp.xml b/NumericalData/CDPP-AMDA/INTERBALL-Tail/MIF-FM/intt-fm-kp.xml
index 0c39c20..79e22bf 100644
--- a/NumericalData/CDPP-AMDA/INTERBALL-Tail/MIF-FM/intt-fm-kp.xml
+++ b/NumericalData/CDPP-AMDA/INTERBALL-Tail/MIF-FM/intt-fm-kp.xml
@@ -6,7 +6,7 @@
key parameters
2012-03-06T15:38:45Z
- ToDo
+ Interball Tail Magnetic Field 2-min key parameters, GSE and GSM Coordinates
spase://SMWG/Person/Ramona.L.Kessel
DataProducer
diff --git a/NumericalData/CDPP-AMDA/IRM/ORBIT/irm-orb-all.xml b/NumericalData/CDPP-AMDA/IRM/ORBIT/irm-orb-all.xml
index 8cf532d..da975e7 100644
--- a/NumericalData/CDPP-AMDA/IRM/ORBIT/irm-orb-all.xml
+++ b/NumericalData/CDPP-AMDA/IRM/ORBIT/irm-orb-all.xml
@@ -7,7 +7,7 @@
orbit
ephemeris
2020-02-07T15:35:31Z
- ToDo
+ AMPTE/IRM spacecraft positions in various coordinate systems
User will acknowledge the AMPTE/IRM team in any publication resulting from the use of these data.
diff --git a/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-aa.xml b/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-aa.xml
index 5061774..6b37c6f 100644
--- a/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-aa.xml
+++ b/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-aa.xml
@@ -6,7 +6,7 @@
aa
aa IAGA-endorsed magnetic activity index
- 2024-05-22T02:04:57Z
+ 2024-05-23T02:05:03Z
Index which purpose is to measure the amplitude of global geomagnetic activity during 3-hour intervals normalized to geomagnetic latitude ±50°. aa was introduced to monitor geomagnetic activity over the longest possible time period.
ISGI website at EOST; License: CC BY-NC https://creativecommons.org/licenses/by-nc/4.0/
@@ -53,7 +53,7 @@
1975-01-01T00:00:00Z
- 2024-05-19T21:00:00Z
+ 2024-05-20T21:00:00Z
PT3H
diff --git a/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-am.xml b/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-am.xml
index 4dd01f9..c1d09bc 100644
--- a/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-am.xml
+++ b/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-am.xml
@@ -6,7 +6,7 @@
am
am IAGA-endorsed magnetic activity index
- 2024-05-22T02:04:57Z
+ 2024-05-23T02:05:04Z
Index which purpose is to provide a characterization of global geomagnetic activity using a large set of stations representing all longitudes and possible hemispheric discrepancies.
ISGI website at EOST; License: CC BY-NC https://creativecommons.org/licenses/by-nc/4.0/
@@ -55,7 +55,7 @@
1975-01-01T00:00:00Z
- 2024-05-19T21:00:00Z
+ 2024-05-20T21:00:00Z
PT3H
diff --git a/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-dst.xml b/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-dst.xml
index cd934a6..8a2e6a1 100644
--- a/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-dst.xml
+++ b/NumericalData/CDPP-AMDA/Indices/Ground_Based/ground-based-dst.xml
@@ -6,7 +6,7 @@
Dst
Disturbance Stormtime index
- 2024-05-22T02:04:58Z
+ 2024-05-23T02:05:04Z
Dst index is taken from the WDC (World Data Center) at Kyoto.
Processing Level :
* FINAL : 1970 - 2014
@@ -66,7 +66,7 @@
1970-01-01T00:00:00Z
- 2024-05-19T23:00:00Z
+ 2024-05-20T23:00:00Z
PT1H
diff --git a/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ele.xml b/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ele.xml
index fdf1a73..4e858aa 100644
--- a/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ele.xml
+++ b/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ele.xml
@@ -5,7 +5,7 @@
spase://CNES/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ele
electron counts
- 2024-05-22T03:17:19Z
+ 2024-05-23T03:12:49Z
High resolution particle count rate data from AMBRE instruments ELE1, ELE2, ELE3 and ELE4 detection heads onboard JASON3 satellite
spase://CNES/Person/CDPP-AMDA/Denis.Payan
diff --git a/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ion.xml b/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ion.xml
index c9a17d6..898c689 100644
--- a/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ion.xml
+++ b/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ion.xml
@@ -5,7 +5,7 @@
spase://CNES/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-ion
ion counts
- 2024-05-22T03:17:20Z
+ 2024-05-23T03:12:50Z
High resolution particle count rate data from AMBRE instruments ION1, ION2, ION3 and ION4 detection heads onboard JASON3 satellite
spase://CNES/Person/CDPP-AMDA/Denis.Payan
diff --git a/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-mag.xml b/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-mag.xml
index 56732b5..b0348cd 100644
--- a/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-mag.xml
+++ b/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-mag.xml
@@ -5,7 +5,7 @@
spase://CNES/NumericalData/CDPP-AMDA/JASON3/AMBRE/jason-amb-mag
mag
- 2024-05-22T03:17:19Z
+ 2024-05-23T03:12:48Z
Calculated magnetic field using ONERA-DESP library internal fields: DGRF/IGRF External field (Olson and Pfitzer, 1974)
spase://CNES/Person/CDPP-AMDA/Denis.Payan
diff --git a/NumericalData/CDPP-AMDA/JASON3/Ephemeris/jason-amb-pos.xml b/NumericalData/CDPP-AMDA/JASON3/Ephemeris/jason-amb-pos.xml
index fdfb59d..adb3193 100644
--- a/NumericalData/CDPP-AMDA/JASON3/Ephemeris/jason-amb-pos.xml
+++ b/NumericalData/CDPP-AMDA/JASON3/Ephemeris/jason-amb-pos.xml
@@ -6,7 +6,7 @@
orbit
JASON3 position in GEO coordinates, L and L* parameters
- 2024-05-22T03:17:21Z
+ 2024-05-23T03:12:50Z
xyz in GEO : Origin = Earth's center of mass. X = Intersec
tion of Greenwich meridian and geographic equator. Z = Geographic North Pole. Y = c
ompletes a right-handed Cartesian triad
diff --git a/NumericalData/CDPP-AMDA/MAVEN/SEP/mvn-sep1-clb.xml b/NumericalData/CDPP-AMDA/MAVEN/SEP/mvn-sep1-clb.xml
index 329d57e..031777d 100644
--- a/NumericalData/CDPP-AMDA/MAVEN/SEP/mvn-sep1-clb.xml
+++ b/NumericalData/CDPP-AMDA/MAVEN/SEP/mvn-sep1-clb.xml
@@ -6,7 +6,9 @@
diff fluxes
2024-04-02T00:23:56Z
- MAVEN SEP 1 Calibrated Ion (without mass discrimination) and Electron Spectra in Forward/Rear look directions (#/cm^2/sec/ster/keV) : Parker / anti-Parker spiral and perpendicular directions
+ MAVEN SEP 1 Calibrated Ion (without mass discrimination) and Electron Spectra in Forward/Rear look directions (#/cm^2/sec/ster/keV) : Parker / anti-Parker spiral and perpendicular directions.
+
+ Attenuator state: 0=error, 1=open, 2=closed, 3=mixed
Principal Investigator : Davin Larson, SSL, Berkeley
diff --git a/NumericalData/CDPP-AMDA/MAVEN/SEP/mvn-sep2-clb.xml b/NumericalData/CDPP-AMDA/MAVEN/SEP/mvn-sep2-clb.xml
index 424f118..bf9cd4d 100644
--- a/NumericalData/CDPP-AMDA/MAVEN/SEP/mvn-sep2-clb.xml
+++ b/NumericalData/CDPP-AMDA/MAVEN/SEP/mvn-sep2-clb.xml
@@ -7,6 +7,8 @@
diff fluxes
2024-04-02T00:29:52Z
MAVEN SEP 1 Calibrated Ion (without mass discrimination) and Electron Spectra in Forward/Rear look directions (#/cm^2/sec/ster/keV) : Parker / anti-Parker spiral and perpendicular directions
+
+ Attenuator state: 0=error, 1=open, 2=closed, 3=mixed
Principal Investigator : Davin Larson, SSL, Berkeley
diff --git a/NumericalData/CDPP-AMDA/MGS/MAG/mgs-mag-mso.xml b/NumericalData/CDPP-AMDA/MGS/MAG/mgs-mag-mso.xml
index 3859f79..a5f307f 100644
--- a/NumericalData/CDPP-AMDA/MGS/MAG/mgs-mag-mso.xml
+++ b/NumericalData/CDPP-AMDA/MGS/MAG/mgs-mag-mso.xml
@@ -6,7 +6,7 @@
orbit mars
2014-05-02T16:10:17Z
- ToDo
+ Calibrated data set from the Magnetometer instrument on the Mars Global Surveyor spacecraft, collected during the Mapping phase of the mission and expressed in Sun-State and Planetocentric coordinates.
spase://SMWG/Person/John.E.P.Connerney
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-dce-brst.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-dce-brst.xml
index 38896b4..f8bc1c6 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-dce-brst.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-dce-brst.xml
@@ -7,7 +7,7 @@
dc e-field
dc electric field / burst / l2
2024-03-26T05:27:41Z
- ToDo
+ Electric Double Probe, Three-Dimensional Electric Field, Level 2, Burst Mode Data
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-dce.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-dce.xml
index fc8e2c6..292b140 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-dce.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-dce.xml
@@ -6,8 +6,8 @@
dc e-field
dc electric field / fast / l2
- 2024-05-22T02:39:41Z
- ToDo
+ 2024-05-23T02:39:00Z
+ Electric Double Probe, Quick-Look Three-Dimensional Electric Field, Level 2, Fast Survey Data
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-hfesp.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-hfesp.xml
index f24e7a8..adb50ae 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-hfesp.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-hfesp.xml
@@ -6,8 +6,8 @@
e spectral density
ac electric field spectral density / srvy / l2
- 2024-05-22T02:39:24Z
- ToDo
+ 2024-05-23T02:38:45Z
+ Electric Double Probe, High-Frequency AC Electric Field Spectra, Level 2, Survey Data, Level 1B AC Electric Field Data
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-scpot.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-scpot.xml
index 71c8cda..201cbf5 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-scpot.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/EDP/mms1-edp-scpot.xml
@@ -6,8 +6,8 @@
scpot
sc potential / fast / l2
- 2024-05-22T02:39:56Z
- ToDo
+ 2024-05-23T02:39:15Z
+ Electric Double Probe, Dual Probe Spacecraft Potential, Level 2, Fast Survey Data. Spacecraft potential is etstimatrd by averaging measurements of the probe-to-spacecraft potential from several probes.
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/Ephemeris/mms1-orb-t89d.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/Ephemeris/mms1-orb-t89d.xml
index 0694f4d..03e43a4 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/Ephemeris/mms1-orb-t89d.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/Ephemeris/mms1-orb-t89d.xml
@@ -5,7 +5,7 @@
spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS1/Ephemeris/mms1-orb-t89d
orbit t89d
- 2024-05-22T02:42:18Z
+ 2024-05-23T02:41:26Z
MMS1 position
spase://CNES/Person/CDPP-AMDA/M.G.Henderson
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/FGM/mms1-fgm-srvy.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/FGM/mms1-fgm-srvy.xml
index fe3bff6..0d17696 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/FGM/mms1-fgm-srvy.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/FGM/mms1-fgm-srvy.xml
@@ -6,7 +6,7 @@
survey
survey
- 2024-05-22T02:41:16Z
+ 2024-05-23T02:40:31Z
For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken
from AFG. Because AFG and DFG are cross-calibrated on an orbit-averaged basis,
small differences in offset may be observed between Level2 burst and survey mode
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-current.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-current.xml
index 2e0644f..855310c 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-current.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-current.xml
@@ -6,7 +6,7 @@
electric current
electric current : fast mode
- 2024-05-22T02:42:08Z
+ 2024-05-23T02:41:20Z
Derived parameter from electron and ion datasets of FPI instrument in Fast Survey Mode.
Electric current: mms1_fast_jgse = 1.6e-10*(mms1_des_ne+mms1_dis_ni)*0.5*(mms1_dis_vgse-mms1_des_vgse)
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-desmoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-desmoms.xml
index 5a20842..2ea848d 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-desmoms.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-desmoms.xml
@@ -6,7 +6,7 @@
DES : electrons
Dual Electron Spectrometers : fast mode
- 2024-05-22T02:42:08Z
+ 2024-05-23T02:41:20Z
FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-dismoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-dismoms.xml
index 5163d26..2e977db 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-dismoms.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/FPI/mms1-fpi-dismoms.xml
@@ -6,7 +6,7 @@
DIS : ions
Dual Ion Spectrometers : fast mode
- 2024-05-22T02:42:09Z
+ 2024-05-23T02:41:21Z
FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/HPCA/mms1-hpca-moms.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/HPCA/mms1-hpca-moms.xml
index 9f3b500..006137c 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/HPCA/mms1-hpca-moms.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/HPCA/mms1-hpca-moms.xml
@@ -6,7 +6,7 @@
ion moments : survey
ion moments : survey mode
- 2024-05-22T02:42:18Z
+ 2024-05-23T02:41:26Z
spase://SMWG/Person/James.L.Burch
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/Models/mms1-msph-models.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/Models/mms1-msph-models.xml
index fb41753..57b5167 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/Models/mms1-msph-models.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/Models/mms1-msph-models.xml
@@ -6,7 +6,7 @@
distance to neutral sheet
Distance to model neutral sheet
- 2024-05-22T02:42:18Z
+ 2024-05-23T02:41:26Z
* Distance (Re) from s/c location to Fairfield1970 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle. Valid for Ysm less than 15 Re.
* Distance (Re) from s/c location to Fairfield1980 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle.
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1/Models/mms1-t96-model.xml b/NumericalData/CDPP-AMDA/MMS/MMS1/Models/mms1-t96-model.xml
index fc61b77..eb9b4bd 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1/Models/mms1-t96-model.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1/Models/mms1-t96-model.xml
@@ -6,7 +6,7 @@
T96 field model
Tsyganenko96 geomagnetospheric magnetic field model
- 2024-05-22T02:42:18Z
+ 2024-05-23T02:41:26Z
A data-based Tsyganenko96 model computes the geomagnetospheric magnetic field with an explicitly defined realistic magnetopause, large-scale Region 1 and 2 Birkeland current systems, and the IMF penetration across the boundary. The model uses the following inputs :
* solar wind ram pressure
* IMF Y and Z-component
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1234/Ephemeris/mms1234-orb-t89d.xml b/NumericalData/CDPP-AMDA/MMS/MMS1234/Ephemeris/mms1234-orb-t89d.xml
index cbb04f4..e4dc876 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1234/Ephemeris/mms1234-orb-t89d.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1234/Ephemeris/mms1234-orb-t89d.xml
@@ -5,7 +5,7 @@
spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS1234/Ephemeris/mms1234-orb-t89d
orbit t89d
- 2024-05-22T02:42:18Z
+ 2024-05-23T02:41:26Z
MMS tetrahedron formation. This dataset contains the barycenter of the tetrahedron and positions of the spacecrafts relative to the barycenter. Positions are expressed in GSE and GSM coordinate systems.
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1234/mms1-fgm-brstcurl.xml b/NumericalData/CDPP-AMDA/MMS/MMS1234/mms1-fgm-brstcurl.xml
index e551eb0..d252cc6 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1234/mms1-fgm-brstcurl.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1234/mms1-fgm-brstcurl.xml
@@ -6,7 +6,7 @@
current
2024-05-03T03:31:05Z
- ToDo
+ Curlometer.
spase://CNES/Person/CDPP-AMDA/Penou
DataProducer
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS1234/mms1-fgm-current.xml b/NumericalData/CDPP-AMDA/MMS/MMS1234/mms1-fgm-current.xml
index f07ae87..03aae9b 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS1234/mms1-fgm-current.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS1234/mms1-fgm-current.xml
@@ -5,8 +5,8 @@
spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS1234/mms1-fgm-current
current
- 2024-05-22T02:39:19Z
- ToDo
+ 2024-05-23T02:38:40Z
+ Curlometer.
spase://CNES/Person/CDPP-AMDA/Penou
DataProducer
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-dce.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-dce.xml
index 9670eaa..f0030a2 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-dce.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-dce.xml
@@ -6,8 +6,8 @@
dc e-field
dc electric field / fast / l2
- 2024-05-22T02:40:14Z
- ToDo
+ 2024-05-23T02:39:32Z
+ Electric Double Probe, Quick-Look Three-Dimensional Electric Field, Level 2, Fast Survey Data
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-hfesp.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-hfesp.xml
index d78b694..75525e2 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-hfesp.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-hfesp.xml
@@ -6,8 +6,8 @@
e spectral density
ac electric field spectral density / srvy / l2
- 2024-05-22T02:39:59Z
- ToDo
+ 2024-05-23T02:39:18Z
+ Electric Double Probe, High-Frequency AC Electric Field Spectra, Level 2, Survey Data, Level 1B AC Electric Field Data
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-scpot.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-scpot.xml
index dd01891..fb95273 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-scpot.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/EDP/mms2-edp-scpot.xml
@@ -6,8 +6,8 @@
scpot
sc potential / fast / l2
- 2024-05-22T02:40:23Z
- ToDo
+ 2024-05-23T02:39:40Z
+ Electric Double Probe, Dual Probe Spacecraft Potential, Level 2, Fast Survey Data. Spacecraft potential is etstimatrd by averaging measurements of the probe-to-spacecraft potential from several probes.
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/Ephemeris/mms2-orb-t89d.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/Ephemeris/mms2-orb-t89d.xml
index 184b0de..5c42bec 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS2/Ephemeris/mms2-orb-t89d.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/Ephemeris/mms2-orb-t89d.xml
@@ -5,7 +5,7 @@
spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS2/Ephemeris/mms2-orb-t89d
orbit t89d
- 2024-05-22T02:42:19Z
+ 2024-05-23T02:41:26Z
MMS2 position
spase://CNES/Person/CDPP-AMDA/M.G.Henderson
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/FGM/mms2-fgm-srvy.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/FGM/mms2-fgm-srvy.xml
index c8a1c86..4c954a2 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS2/FGM/mms2-fgm-srvy.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/FGM/mms2-fgm-srvy.xml
@@ -6,7 +6,7 @@
survey
survey
- 2024-05-22T02:41:28Z
+ 2024-05-23T02:40:42Z
For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken
from AFG. Because AFG and DFG are cross-calibrated on an orbit-averaged basis,
small differences in offset may be observed between Level2 burst and survey mode
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-current.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-current.xml
index 8be50a5..f13c686 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-current.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-current.xml
@@ -6,7 +6,7 @@
electric current
electric current : fast mode
- 2024-05-22T02:42:09Z
+ 2024-05-23T02:41:22Z
Derived parameter from electron and ion datasets of FPI instrument in Fast Survey Mode.
Electric current: mms2_fast_jgse = 1.6e-10*(mms2_des_ne+mms2_dis_ni)*0.5*(mms2_dis_vgse-mms2_des_vgse)
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-desmoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-desmoms.xml
index 7929d67..4467354 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-desmoms.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-desmoms.xml
@@ -6,7 +6,7 @@
DES : electrons
Dual Electron Spectrometers : fast mode
- 2024-05-22T02:42:09Z
+ 2024-05-23T02:41:22Z
FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-dismoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-dismoms.xml
index 14791f1..b2de784 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-dismoms.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/FPI/mms2-fpi-dismoms.xml
@@ -6,7 +6,7 @@
DIS : ions
Dual Ion Spectrometers : fast mode
- 2024-05-22T02:42:10Z
+ 2024-05-23T02:41:22Z
FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/Models/mms2-msph-models.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/Models/mms2-msph-models.xml
index 057063d..1396a83 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS2/Models/mms2-msph-models.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/Models/mms2-msph-models.xml
@@ -6,7 +6,7 @@
distance to neutral sheet
Distance to model neutral sheet
- 2024-05-22T02:42:19Z
+ 2024-05-23T02:41:26Z
* Distance (Re) from s/c location to Fairfield1970 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle. Valid for Ysm less than 15 Re.
* Distance (Re) from s/c location to Fairfield1980 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle.
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS2/Models/mms2-t96-model.xml b/NumericalData/CDPP-AMDA/MMS/MMS2/Models/mms2-t96-model.xml
index 21a6e91..0a8231e 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS2/Models/mms2-t96-model.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS2/Models/mms2-t96-model.xml
@@ -6,7 +6,7 @@
T96 field model
Tsyganenko96 geomagnetospheric magnetic field model
- 2024-05-22T02:42:19Z
+ 2024-05-23T02:41:26Z
A data-based Tsyganenko96 model computes the geomagnetospheric magnetic field with an explicitly defined realistic magnetopause, large-scale Region 1 and 2 Birkeland current systems, and the IMF penetration across the boundary. The model uses the following inputs :
* solar wind ram pressure
* IMF Y and Z-component
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-dce.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-dce.xml
index de94e89..ec10268 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-dce.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-dce.xml
@@ -6,8 +6,8 @@
dc e-field
dc electric field / fast / l2
- 2024-05-22T02:40:27Z
- ToDo
+ 2024-05-23T02:39:44Z
+ Electric Double Probe, Quick-Look Three-Dimensional Electric Field, Level 2, Fast Survey Data
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-hfesp.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-hfesp.xml
index 6c56060..ae04d5b 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-hfesp.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-hfesp.xml
@@ -6,8 +6,8 @@
e spectral density
ac electric field spectral density / srvy / l2
- 2024-05-22T02:40:24Z
- ToDo
+ 2024-05-23T02:39:41Z
+ Electric Double Probe, High-Frequency AC Electric Field Spectra, Level 2, Survey Data, Level 1B AC Electric Field Data
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-scpot.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-scpot.xml
index abad504..080bf2f 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-scpot.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/EDP/mms3-edp-scpot.xml
@@ -6,8 +6,8 @@
scpot
sc potential / fast / l2
- 2024-05-22T02:40:30Z
- ToDo
+ 2024-05-23T02:39:47Z
+ Electric Double Probe, Dual Probe Spacecraft Potential, Level 2, Fast Survey Data. Spacecraft potential is etstimatrd by averaging measurements of the probe-to-spacecraft potential from several probes.
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/Ephemeris/mms3-orb-t89d.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/Ephemeris/mms3-orb-t89d.xml
index f568bfc..a1f6857 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS3/Ephemeris/mms3-orb-t89d.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/Ephemeris/mms3-orb-t89d.xml
@@ -5,7 +5,7 @@
spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS3/Ephemeris/mms3-orb-t89d
orbit t89d
- 2024-05-22T02:42:19Z
+ 2024-05-23T02:41:27Z
MMS3 position
spase://CNES/Person/CDPP-AMDA/M.G.Henderson
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/FGM/mms3-fgm-srvy.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/FGM/mms3-fgm-srvy.xml
index 6818f2f..441d6ff 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS3/FGM/mms3-fgm-srvy.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/FGM/mms3-fgm-srvy.xml
@@ -6,7 +6,7 @@
survey
survey
- 2024-05-22T02:41:40Z
+ 2024-05-23T02:40:54Z
For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken
from AFG. Because AFG and DFG are cross-calibrated on an orbit-averaged basis,
small differences in offset may be observed between Level2 burst and survey mode
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-current.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-current.xml
index a98817b..247398f 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-current.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-current.xml
@@ -6,7 +6,7 @@
electric current
electric current : fast mode
- 2024-05-22T02:42:15Z
+ 2024-05-23T02:41:23Z
Derived parameter from electron and ion datasets of FPI instrument in Fast Survey Mode.
Electric current: mms3_fast_jgse = 1.6e-10*(mms3_des_ne+mms3_dis_ni)*0.5*(mms3_dis_vgse-mms3_des_vgse)
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-desmoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-desmoms.xml
index fd2dffe..0e805ba 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-desmoms.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-desmoms.xml
@@ -6,7 +6,7 @@
DES : electrons
Dual Electron Spectrometers : fast mode
- 2024-05-22T02:42:15Z
+ 2024-05-23T02:41:23Z
FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-dismoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-dismoms.xml
index cde348e..68f395e 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-dismoms.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-dismoms.xml
@@ -6,7 +6,7 @@
DIS : ions
Dual Ion Spectrometers : fast mode
- 2024-05-22T02:42:16Z
+ 2024-05-23T02:41:24Z
FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/Models/mms3-msph-models.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/Models/mms3-msph-models.xml
index c45afa7..c809193 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS3/Models/mms3-msph-models.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/Models/mms3-msph-models.xml
@@ -6,7 +6,7 @@
distance to neutral sheet
Distance to model neutral sheet
- 2024-05-22T02:42:19Z
+ 2024-05-23T02:41:27Z
* Distance (Re) from s/c location to Fairfield1970 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle. Valid for Ysm less than 15 Re.
* Distance (Re) from s/c location to Fairfield1980 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle.
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS3/Models/mms3-t96-model.xml b/NumericalData/CDPP-AMDA/MMS/MMS3/Models/mms3-t96-model.xml
index a1d68a0..b90a061 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS3/Models/mms3-t96-model.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS3/Models/mms3-t96-model.xml
@@ -6,7 +6,7 @@
T96 field model
Tsyganenko96 geomagnetospheric magnetic field model
- 2024-05-22T02:42:19Z
+ 2024-05-23T02:41:27Z
A data-based Tsyganenko96 model computes the geomagnetospheric magnetic field with an explicitly defined realistic magnetopause, large-scale Region 1 and 2 Birkeland current systems, and the IMF penetration across the boundary. The model uses the following inputs :
* solar wind ram pressure
* IMF Y and Z-component
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-dce.xml b/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-dce.xml
index 8ab8e74..6d3d892 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-dce.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-dce.xml
@@ -6,8 +6,8 @@
dc e-field
dc electric field / fast / l2
- 2024-05-22T02:40:47Z
- ToDo
+ 2024-05-23T02:40:03Z
+ Electric Double Probe, Quick-Look Three-Dimensional Electric Field, Level 2, Fast Survey Data
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-hfesp.xml b/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-hfesp.xml
index 78a7950..8886160 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-hfesp.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-hfesp.xml
@@ -6,8 +6,8 @@
e spectral density
ac electric field spectral density / srvy / l2
- 2024-05-22T02:40:31Z
- ToDo
+ 2024-05-23T02:39:48Z
+ Electric Double Probe, High-Frequency AC Electric Field Spectra, Level 2, Survey Data, Level 1B AC Electric Field Data
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-scpot.xml b/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-scpot.xml
index 173e713..f30c180 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-scpot.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS4/EDP/mms4-edp-scpot.xml
@@ -6,8 +6,8 @@
scpot
sc potential / fast / l2
- 2024-05-22T02:41:04Z
- ToDo
+ 2024-05-23T02:40:19Z
+ Electric Double Probe, Dual Probe Spacecraft Potential, Level 2, Fast Survey Data. Spacecraft potential is etstimatrd by averaging measurements of the probe-to-spacecraft potential from several probes.
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS4/Ephemeris/mms4-orb-t89d.xml b/NumericalData/CDPP-AMDA/MMS/MMS4/Ephemeris/mms4-orb-t89d.xml
index 6ac722d..63a632b 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS4/Ephemeris/mms4-orb-t89d.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS4/Ephemeris/mms4-orb-t89d.xml
@@ -5,7 +5,7 @@
spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS4/Ephemeris/mms4-orb-t89d
orbit t89d
- 2024-05-22T02:42:19Z
+ 2024-05-23T02:41:27Z
MMS4 position
spase://CNES/Person/CDPP-AMDA/M.G.Henderson
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS4/FGM/mms4-fgm-srvy.xml b/NumericalData/CDPP-AMDA/MMS/MMS4/FGM/mms4-fgm-srvy.xml
index d8c122c..a24068b 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS4/FGM/mms4-fgm-srvy.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS4/FGM/mms4-fgm-srvy.xml
@@ -6,7 +6,7 @@
survey
survey
- 2024-05-22T02:42:05Z
+ 2024-05-23T02:41:17Z
For the purpose of creating a unified FGM Level 2 data product, burst mode data is taken from DFG and survey mode data is taken
from AFG. Because AFG and DFG are cross-calibrated on an orbit-averaged basis,
small differences in offset may be observed between Level2 burst and survey mode
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-dismoms.xml b/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-dismoms.xml
index 4feb821..7b3ab9f 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-dismoms.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS4/FPI/mms4-fpi-dismoms.xml
@@ -6,7 +6,7 @@
DIS : ions
Dual Ion Spectrometers : fast mode
- 2024-05-22T02:42:17Z
+ 2024-05-23T02:41:24Z
FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS4/Models/mms4-msph-models.xml b/NumericalData/CDPP-AMDA/MMS/MMS4/Models/mms4-msph-models.xml
index 53c535b..7a9d3b7 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS4/Models/mms4-msph-models.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS4/Models/mms4-msph-models.xml
@@ -6,7 +6,7 @@
distance to neutral sheet
Distance to model neutral sheet
- 2024-05-22T02:42:19Z
+ 2024-05-23T02:41:27Z
* Distance (Re) from s/c location to Fairfield1970 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle. Valid for Ysm less than 15 Re.
* Distance (Re) from s/c location to Fairfield1980 neutral sheet position. Depends on spacecraft location in SM coordinates and dipole tilt angle.
diff --git a/NumericalData/CDPP-AMDA/MMS/MMS4/Models/mms4-t96-model.xml b/NumericalData/CDPP-AMDA/MMS/MMS4/Models/mms4-t96-model.xml
index a7b3188..c782dcd 100644
--- a/NumericalData/CDPP-AMDA/MMS/MMS4/Models/mms4-t96-model.xml
+++ b/NumericalData/CDPP-AMDA/MMS/MMS4/Models/mms4-t96-model.xml
@@ -6,7 +6,7 @@
T96 field model
Tsyganenko96 geomagnetospheric magnetic field model
- 2024-05-22T02:42:19Z
+ 2024-05-23T02:41:27Z
A data-based Tsyganenko96 model computes the geomagnetospheric magnetic field with an explicitly defined realistic magnetopause, large-scale Region 1 and 2 Birkeland current systems, and the IMF penetration across the boundary. The model uses the following inputs :
* solar wind ram pressure
* IMF Y and Z-component
diff --git a/NumericalData/CDPP-AMDA/Phobos2/ASPERA/pho-asp-el.xml b/NumericalData/CDPP-AMDA/Phobos2/ASPERA/pho-asp-el.xml
index 2d52cf6..f8ea45d 100644
--- a/NumericalData/CDPP-AMDA/Phobos2/ASPERA/pho-asp-el.xml
+++ b/NumericalData/CDPP-AMDA/Phobos2/ASPERA/pho-asp-el.xml
@@ -6,7 +6,7 @@
elec spectra
2019-12-06T11:02:13Z
- ToDo
+ Electron spectra
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Phobos2/ASPERA/pho-asp-ion.xml b/NumericalData/CDPP-AMDA/Phobos2/ASPERA/pho-asp-ion.xml
index ee621c7..e131655 100644
--- a/NumericalData/CDPP-AMDA/Phobos2/ASPERA/pho-asp-ion.xml
+++ b/NumericalData/CDPP-AMDA/Phobos2/ASPERA/pho-asp-ion.xml
@@ -6,7 +6,7 @@
ion spectra
2019-12-06T10:20:33Z
- ToDo
+ Ion spectra
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Phobos2/MAG/pho-mag-data.xml b/NumericalData/CDPP-AMDA/Phobos2/MAG/pho-mag-data.xml
index 19a32b1..fa8f136 100644
--- a/NumericalData/CDPP-AMDA/Phobos2/MAG/pho-mag-data.xml
+++ b/NumericalData/CDPP-AMDA/Phobos2/MAG/pho-mag-data.xml
@@ -6,7 +6,7 @@
b field
2012-11-15T12:38:35Z
- ToDo
+ Magnetic field data
spase://SMWG/Person/Konrad.Schwingenschuh
PrincipalInvestigator
diff --git a/NumericalData/CDPP-AMDA/Pioneer10/CPI/p10-cpi-ele.xml b/NumericalData/CDPP-AMDA/Pioneer10/CPI/p10-cpi-ele.xml
index 9ce933a..0116707 100644
--- a/NumericalData/CDPP-AMDA/Pioneer10/CPI/p10-cpi-ele.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer10/CPI/p10-cpi-ele.xml
@@ -6,7 +6,10 @@
electron flux
2012-09-13T15:07:27Z
- ToDo
+ Pionner 10
+ CPI - Charge Particle Instrument -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Pioneer10/CPI/p10-cpi-ion.xml b/NumericalData/CDPP-AMDA/Pioneer10/CPI/p10-cpi-ion.xml
index cee0edc..1d1445b 100644
--- a/NumericalData/CDPP-AMDA/Pioneer10/CPI/p10-cpi-ion.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer10/CPI/p10-cpi-ion.xml
@@ -6,7 +6,10 @@
ion flux
2012-09-13T15:54:27Z
- ToDo
+ Pionner 10
+ CPI - Charge Particle Instrument -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Pioneer10/CRT/p10-crt-ele.xml b/NumericalData/CDPP-AMDA/Pioneer10/CRT/p10-crt-ele.xml
index e2eedd9..36c49fa 100644
--- a/NumericalData/CDPP-AMDA/Pioneer10/CRT/p10-crt-ele.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer10/CRT/p10-crt-ele.xml
@@ -6,7 +6,10 @@
electron flux
2012-09-14T07:05:51Z
- ToDo
+ Pionner 10
+ CRT - Cosmic Ray Telescope -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Pioneer10/CRT/p10-crt-ion.xml b/NumericalData/CDPP-AMDA/Pioneer10/CRT/p10-crt-ion.xml
index f88e691..038514a 100644
--- a/NumericalData/CDPP-AMDA/Pioneer10/CRT/p10-crt-ion.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer10/CRT/p10-crt-ion.xml
@@ -6,7 +6,10 @@
ion flux
2012-09-14T07:24:24Z
- ToDo
+ Pionner 10
+ CRT - Cosmic Ray Telescope -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Pioneer10/GTT/p10-gtt-ele.xml b/NumericalData/CDPP-AMDA/Pioneer10/GTT/p10-gtt-ele.xml
index 3aef77b..bc72e9f 100644
--- a/NumericalData/CDPP-AMDA/Pioneer10/GTT/p10-gtt-ele.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer10/GTT/p10-gtt-ele.xml
@@ -6,7 +6,10 @@
electron flux
2012-09-13T14:26:47Z
- ToDo
+ Pionner 10
+ GTT - Geiger Tube Telescope -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Pioneer10/GTT/p10-gtt-ion.xml b/NumericalData/CDPP-AMDA/Pioneer10/GTT/p10-gtt-ion.xml
index b87d7f1..9efebe5 100644
--- a/NumericalData/CDPP-AMDA/Pioneer10/GTT/p10-gtt-ion.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer10/GTT/p10-gtt-ion.xml
@@ -6,7 +6,10 @@
ion flux
2012-09-13T14:47:05Z
- ToDo
+ Pionner 10
+ GTT - Geiger Tube Telescope -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Pioneer11/CPI/p11-cpi-ele.xml b/NumericalData/CDPP-AMDA/Pioneer11/CPI/p11-cpi-ele.xml
index 10683ad..0b01a87 100644
--- a/NumericalData/CDPP-AMDA/Pioneer11/CPI/p11-cpi-ele.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer11/CPI/p11-cpi-ele.xml
@@ -6,7 +6,10 @@
electron flux
2012-09-14T09:51:58Z
- ToDo
+ Pionner 11
+ CPI - Charge Particle Instrument -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Pioneer11/CPI/p11-cpi-ion.xml b/NumericalData/CDPP-AMDA/Pioneer11/CPI/p11-cpi-ion.xml
index 2099483..d89b18a 100644
--- a/NumericalData/CDPP-AMDA/Pioneer11/CPI/p11-cpi-ion.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer11/CPI/p11-cpi-ion.xml
@@ -6,7 +6,10 @@
ion flux
2012-09-14T09:57:18Z
- ToDo
+ Pionner 11
+ CPI - Charge Particle Instrument -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Pioneer11/CRT/p11-crt-ele.xml b/NumericalData/CDPP-AMDA/Pioneer11/CRT/p11-crt-ele.xml
index a04ccc7..327973b 100644
--- a/NumericalData/CDPP-AMDA/Pioneer11/CRT/p11-crt-ele.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer11/CRT/p11-crt-ele.xml
@@ -6,7 +6,10 @@
electron flux
2012-09-14T13:25:05Z
- ToDo
+ Pionner 11
+ CRT - Cosmic Ray Telescope -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Pioneer11/CRT/p11-crt-ion.xml b/NumericalData/CDPP-AMDA/Pioneer11/CRT/p11-crt-ion.xml
index 13a0558..94e4b5b 100644
--- a/NumericalData/CDPP-AMDA/Pioneer11/CRT/p11-crt-ion.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer11/CRT/p11-crt-ion.xml
@@ -6,7 +6,10 @@
ion flux
2012-09-14T13:28:40Z
- ToDo
+ Pionner 11
+ CRT - Cosmic Ray Telescope -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Pioneer11/GTT/p11-gtt-ele.xml b/NumericalData/CDPP-AMDA/Pioneer11/GTT/p11-gtt-ele.xml
index 0c766ab..6337b7b 100644
--- a/NumericalData/CDPP-AMDA/Pioneer11/GTT/p11-gtt-ele.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer11/GTT/p11-gtt-ele.xml
@@ -6,7 +6,10 @@
electron flux
2012-09-14T08:51:46Z
- ToDo
+ Pionner 11
+ GTT - Geiger Tube Telescope -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Pioneer11/GTT/p11-gtt-ion.xml b/NumericalData/CDPP-AMDA/Pioneer11/GTT/p11-gtt-ion.xml
index fa70521..a0f1ac3 100644
--- a/NumericalData/CDPP-AMDA/Pioneer11/GTT/p11-gtt-ion.xml
+++ b/NumericalData/CDPP-AMDA/Pioneer11/GTT/p11-gtt-ion.xml
@@ -6,7 +6,10 @@
ion flux
2012-09-14T08:58:03Z
- ToDo
+ Pionner 11
+ GTT - Geiger Tube Telescope -
+ Data provided to CDPP by ONERA. All information included in this report:
+ http://amda.cdpp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf
spase://SMWG/Person/Elena.Budnik
GeneralContact
diff --git a/NumericalData/CDPP-AMDA/Rosetta/AUXILLIARY/ros-aux-all.xml b/NumericalData/CDPP-AMDA/Rosetta/AUXILLIARY/ros-aux-all.xml
index cebb7e5..2948a9a 100644
--- a/NumericalData/CDPP-AMDA/Rosetta/AUXILLIARY/ros-aux-all.xml
+++ b/NumericalData/CDPP-AMDA/Rosetta/AUXILLIARY/ros-aux-all.xml
@@ -6,7 +6,7 @@
Orbit/Attitude
2017-07-18T22:15:05Z
- ToDo
+ Orbit/Attitude
spase://CNES/Person/CDPP-AMDA/L.Foldy
TechnicalContact
diff --git a/NumericalData/CDPP-AMDA/Rosetta/MAG/ros-magib-1s.xml b/NumericalData/CDPP-AMDA/Rosetta/MAG/ros-magib-1s.xml
index 99585c5..943a602 100644
--- a/NumericalData/CDPP-AMDA/Rosetta/MAG/ros-magib-1s.xml
+++ b/NumericalData/CDPP-AMDA/Rosetta/MAG/ros-magib-1s.xml
@@ -7,7 +7,7 @@
1 s
Inboard calibrated; burst mode
2019-03-26T19:09:18Z
- ToDo
+ Inboard calibrated; burst mode