diff --git a/NumericalData/AMDA/ACE/MFI/ace-imf-all.xml b/NumericalData/AMDA/ACE/MFI/ace-imf-all.xml
index ad8b9ca..c382ffe 100644
--- a/NumericalData/AMDA/ACE/MFI/ace-imf-all.xml
+++ b/NumericalData/AMDA/ACE/MFI/ace-imf-all.xml
@@ -58,7 +58,7 @@
1997-09-02T00:00:12Z
- 2016-07-23T23:59:48Z
+ 2016-08-13T23:59:44Z
PT16S
diff --git a/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml b/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml
index fc11a69..6e7971a 100644
--- a/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml
+++ b/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml
@@ -51,7 +51,7 @@
2014-01-06T00:00:00Z
- 2016-08-06T23:59:59Z
+ 2016-08-22T23:59:59Z
PT60S
diff --git a/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml b/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml
index fd7c12d..d3dc6f9 100644
--- a/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml
+++ b/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml
@@ -44,7 +44,7 @@
2014-01-06T00:00:00Z
- 2016-08-06T23:59:59Z
+ 2016-08-22T23:59:59Z
PT60S
diff --git a/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml b/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml
index 64877a3..6e5f63e 100644
--- a/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml
+++ b/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml
@@ -59,7 +59,7 @@
2001-01-01T00:00:00Z
- 2016-07-23T23:55:00Z
+ 2016-08-13T23:55:00Z
PT5M
diff --git a/NumericalData/AMDA/ACE/ephemeris/ace-orb-all.xml b/NumericalData/AMDA/ACE/ephemeris/ace-orb-all.xml
index 7d57a00..1fd61de 100644
--- a/NumericalData/AMDA/ACE/ephemeris/ace-orb-all.xml
+++ b/NumericalData/AMDA/ACE/ephemeris/ace-orb-all.xml
@@ -33,7 +33,7 @@
1997-08-26T00:00:00Z
- 2016-10-09T23:47:00Z
+ 2016-10-24T23:47:00Z
PT12M
diff --git a/NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml b/NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml
index 37f1018..74a8b96 100644
--- a/NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml
+++ b/NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml
@@ -42,7 +42,7 @@
2014-06-01T00:00:00Z
- 2016-05-17T19:47:00Z
+ 2016-08-16T19:37:00Z
PT1M
diff --git a/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml b/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml
index 07bf8b0..2e9775a 100644
--- a/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml
+++ b/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml
@@ -44,7 +44,7 @@
2014-10-10T00:00:00Z
- 2016-02-15T00:00:02Z
+ 2016-05-09T00:00:01Z
PT0.031S
diff --git a/NumericalData/AMDA/MEX/ELS/mex-els-all.xml b/NumericalData/AMDA/MEX/ELS/mex-els-all.xml
index 0c58fee..45b6099 100644
--- a/NumericalData/AMDA/MEX/ELS/mex-els-all.xml
+++ b/NumericalData/AMDA/MEX/ELS/mex-els-all.xml
@@ -41,7 +41,7 @@ Institute of Space Physics, PI, and the European Space Agency
2003-06-23T18:42:48Z
- 2016-06-06T05:29:07Z
+ 2016-08-13T21:35:21Z
PT4S
diff --git a/NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml b/NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml
index 105ff1b..ed579cb 100644
--- a/NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml
+++ b/NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml
@@ -27,7 +27,7 @@
2004-01-10T07:54:21Z
- 2016-07-31T13:17:49Z
+ 2016-10-09T05:10:11Z
PT60S
diff --git a/NumericalData/AMDA/OMNI/omni-5min-all.xml b/NumericalData/AMDA/OMNI/omni-5min-all.xml
index 48ab9e2..b7fd4f2 100644
--- a/NumericalData/AMDA/OMNI/omni-5min-all.xml
+++ b/NumericalData/AMDA/OMNI/omni-5min-all.xml
@@ -47,7 +47,7 @@ for creating the OMNI data set.
1981-01-01T00:00:00Z
- 2016-07-13T23:55:00Z
+ 2016-07-31T23:55:00Z
PT5M
diff --git a/NumericalData/AMDA/OMNI/omni-hour-all.xml b/NumericalData/AMDA/OMNI/omni-hour-all.xml
index 438455e..f4086d6 100644
--- a/NumericalData/AMDA/OMNI/omni-hour-all.xml
+++ b/NumericalData/AMDA/OMNI/omni-hour-all.xml
@@ -47,7 +47,7 @@ for creating the OMNI data set.
1970-01-01T00:00:00Z
- 2016-07-15T14:00:00Z
+ 2016-08-04T14:00:00Z
PT1H
diff --git a/NumericalOutput/AMDA/CAIN/b_cain.xml b/NumericalOutput/AMDA/CAIN/b_cain.xml
index 0cc0895..cb0f0af 100644
--- a/NumericalOutput/AMDA/CAIN/b_cain.xml
+++ b/NumericalOutput/AMDA/CAIN/b_cain.xml
@@ -4,19 +4,19 @@
spase://CDPP/NumericalOutput/AMDA/CAIN/b_cain
- Cain B
- 2014-07-08T16:49:29Z
- TBD
+ Cain B along s/c orbit
+ 2016-08-23T00:00:00Z
+ Cain model martian crustal magnetic field along s/c orbit is being real-time calculated.
+ S/c and sampling time should be defined by user.
+
TBD
-
- TBD
- PrincipalInvestigator
+
+ spase://SMWG/Person/Elena.Budnik
+ TechnicalContact
Rules of use, and caveats
-
- TBD
-
+ TBD
TBD
@@ -31,9 +31,7 @@
Text.ASCII
-
- TBD
-
+ TBD
spase://CDPP/SimulationRun/AMDA/CAIN/CainRun
MagneticField
@@ -42,7 +40,7 @@
1970-01-01T00:00:00Z
1970-01-01T00:00:00Z
-
+ UserDefined
Mars
@@ -61,7 +59,7 @@
3
bx
-
+ Component.I
bcain_mso(0)
@@ -70,7 +68,7 @@
by
-
+ Component.J
bcain_mso(1)
@@ -79,7 +77,7 @@
bz
-
+ Component.K
bcain_mso(2)
@@ -88,6 +86,9 @@
NaN
+
+ Magnetic
+
b tot
@@ -98,6 +99,9 @@
nT
NaN
+
+ Magnetic
+
-
+
diff --git a/NumericalOutput/AMDA/TAO/Jupiter/tao-jupiter-omni.xml b/NumericalOutput/AMDA/TAO/Jupiter/tao-jupiter-omni.xml
index 5db980b..9e5bcdb 100644
--- a/NumericalOutput/AMDA/TAO/Jupiter/tao-jupiter-omni.xml
+++ b/NumericalOutput/AMDA/TAO/Jupiter/tao-jupiter-omni.xml
@@ -4,8 +4,8 @@
spase://CDPP/NumericalOutput/AMDA/TAO/Jupiter/tao-jupiter-omni
- Tao SW Jupiter
- 2014-07-08T16:49:29Z
+ Tao SW Jupiter / OMNI input
+ 2016-08-22T00:00:00Z
TBD
TBD
@@ -44,11 +44,11 @@
PT1H
- Saturn
+ Jupiter
TBD
- spase://CDPP/NumericalData/AMDA/OMNI/omni-5min-all
+ spase://CDPP/NumericalData/AMDA/OMNI/omni-hour-all
Proton Number Density
jupiter_omni_n
diff --git a/NumericalOutput/AMDA/TSYG96/b_t96.xml b/NumericalOutput/AMDA/TSYG96/b_t96.xml
new file mode 100644
index 0000000..6e92341
--- /dev/null
+++ b/NumericalOutput/AMDA/TSYG96/b_t96.xml
@@ -0,0 +1,106 @@
+
+
+ 2.2.6
+
+ spase://CDPP/NumericalOutput/AMDA/TSYG96/b_t96
+
+ T96 Bgsm along s/c orbit
+ 2016-08-23T00:00:00Z
+ .
+
+ TBD
+
+ spase://SMWG/Person/Elena.Budnik
+ TechnicalContact
+
+
+ Rules of use, and caveats
+ TBD
+ TBD
+
+
+
+ spase://SMWG/Repository/CDPP/AMDA
+ Online
+ Open
+
+ AMDA at CDPP
+
+ http://amda.cdpp.eu
+
+
+ Text.ASCII
+ TBD
+
+ spase://CDPP/SimulationRun/AMDA/TSYG96/Tsyg96Run
+ MagneticField
+
+
+ 1970-01-01T00:00:00Z
+ 1970-01-01T00:00:00Z
+
+ UserDefined
+
+ Mars
+
+ TBD
+
+
+
+ b gsm
+ b_t96gsm
+
+
+ TBD
+
+ nT
+
+ 3
+
+ bx
+ Component.I
+
+ b_t96gsm(0)
+
+
+
+
+
+ by
+ Component.J
+
+ b_t96gsm(1)
+
+
+
+
+
+ bz
+ Component.K
+
+ b_t96gsm(2)
+
+
+
+
+
+ NaN
+
+ Magnetic
+
+
+
+ b tot
+ b_t96tot
+ TBD
+
+ TBD
+
+ nT
+ NaN
+
+ Magnetic
+
+
+
+
diff --git a/SimulationModel/AMDA/Cain.xml b/SimulationModel/AMDA/Cain.xml
index cbd4ef8..b2be4d6 100644
--- a/SimulationModel/AMDA/Cain.xml
+++ b/SimulationModel/AMDA/Cain.xml
@@ -5,7 +5,7 @@
spase://CDPP/SimulationModel/AMDA/Cain
Cain Model
- Cain Mars Crustal magnetic Field Model
+ Cain martian crustal magnetic field model
2014-07-08T14:48:29Z
Spherical Harmonic
@@ -15,7 +15,7 @@
Model_Magnetic_Field
PartOf
- Mars Crustal Magnetic Field Models
+ Magnetic Field Models
Spherical Harmonic
diff --git a/SimulationModel/AMDA/Michigan.xml b/SimulationModel/AMDA/Michigan.xml
index 1ad5f8a..a18ba9d 100644
--- a/SimulationModel/AMDA/Michigan.xml
+++ b/SimulationModel/AMDA/Michigan.xml
@@ -14,7 +14,7 @@
SW_Propagation
PartOf
- Model SW Propagation
+ Solar Wind Propagation
MHD
diff --git a/SimulationModel/AMDA/Morschhauser.xml b/SimulationModel/AMDA/Morschhauser.xml
index c89c972..e5e52ca 100644
--- a/SimulationModel/AMDA/Morschhauser.xml
+++ b/SimulationModel/AMDA/Morschhauser.xml
@@ -9,13 +9,13 @@
2014-07-08T14:48:29Z
Spherical Harmonic
- TBD
+ Morschhauser
PrincipalInvestigator
Model_Magnetic_Field
PartOf
- Mars Crustal Magnetic Field Models
+ Magnetic Field Models
Spherical Harmonic
diff --git a/SimulationModel/AMDA/Tao.xml b/SimulationModel/AMDA/Tao.xml
index 2717478..4a8d7bb 100644
--- a/SimulationModel/AMDA/Tao.xml
+++ b/SimulationModel/AMDA/Tao.xml
@@ -14,7 +14,7 @@
SW_Propagation
PartOf
- Model SW Propagation
+ Solar Wind Propagation
MHD
diff --git a/SimulationModel/AMDA/Tsyganenko96.xml b/SimulationModel/AMDA/Tsyganenko96.xml
new file mode 100644
index 0000000..a5f77a1
--- /dev/null
+++ b/SimulationModel/AMDA/Tsyganenko96.xml
@@ -0,0 +1,23 @@
+
+
+ 2.2.6
+
+ spase://CDPP/SimulationModel/AMDA/Tsyganenko96
+
+ T96 Model
+ T96 geomagnetic field model
+ 2014-07-08T14:48:29Z
+
+
+ TBD
+ PrincipalInvestigator
+
+
+ Model_Magnetic_Field
+ PartOf
+ Magnetic Field Models
+
+
+
+
+
diff --git a/SimulationRun/AMDA/CAIN/CainRun.xml b/SimulationRun/AMDA/CAIN/CainRun.xml
index 33493fe..57395ab 100644
--- a/SimulationRun/AMDA/CAIN/CainRun.xml
+++ b/SimulationRun/AMDA/CAIN/CainRun.xml
@@ -5,12 +5,38 @@
spase://CDPP/SimulationRun/AMDA/CAIN/CainRun
Cain Model
- Mars Model Crustal magnetic Field alog s/c orbit
- 2014-07-08T14:48:29Z
-
+ Cain model of martian crustal magnetic field
+ 2016-08-22T00:00:00Z
+ [1] A potential function using spherical harmonics up to degree and order 90 was derived
+from a selection of Mars Global Surveyor vector data. These included all three
+components of those taken below 200 km altitude during the two aerobraking phases
+(AB1 and AB2), the Science Phase Orbits (SPO), and the higher-altitude (367–435 km)
+data taken on the nightside during the Mapping Phase Orbits (MPO). The merger of these
+sets of data provided total global coverage. The technique used was a least squares
+minimization developed for Earth field analysis whereby the relative weighting of each
+data source was determined by the width of a Gaussian fit to the residual distribution about
+the potential function. Also, data selection by area and area weight functions were used to
+improve normalization. The residual misfit distributions for the vertical component for
+different data sources are (nT) AB1, 6.5; AB2 (in shadow), 6.7; AB2 (sunlit), 10.3; SPO,
+6.4; and MPO, 5.9. The horizontal component misfits are about the same for MPO and
+AB2 in shadow, but for data taken in sunlight the scatter of horizontal component residuals
+increases by 50% for AB1, a factor of two for SPO, and 30% for AB2. The energy density
+spectrum evaluated at 3535 km radius (the mean altitude of the AB and SPO data)
+decreased from a high of 0.2 J/km3 near n = 20 to an order of magnitude less at n = 90.
+Most of the power in the spectrum lies between n = 15 and n = 40. The dipole moment
+was only 8 Â 1016 A Á m2, which is likely close to the noise of the coefficients. This
+spectrum is 40 times greater than that of Earth at the scale sizes represented by values of n
+from 20 to 40. Comparisons with other published maps and models for Mars show general
+agreement with the field representations at MPO altitudes, but disagreements up to several
+INhundred nT in components calculated for areodetic altitudes below 200 km.
+
-
+ spase://CDPP/Person/Joseph.C.Cain
PrincipalInvestigator
+
+
+ spase://SMWG/Person/Elena.Budnik
+ TechnicalContact
@@ -23,10 +49,13 @@
MSO
3
-
-
+ km
+
- Orbit
+ Orbit
+
+ Ephemeris
+
diff --git a/SimulationRun/AMDA/TSYG96/Tsyg96Run.xml b/SimulationRun/AMDA/TSYG96/Tsyg96Run.xml
new file mode 100644
index 0000000..ee2d867
--- /dev/null
+++ b/SimulationRun/AMDA/TSYG96/Tsyg96Run.xml
@@ -0,0 +1,40 @@
+
+
+ 2.2.6
+
+ spase://CDPP/SimulationRun/AMDA/TSYG96/Tsyg96Run
+
+ T96 Model
+
+ 2016-08-22T00:00:00Z
+
+
+
+ spase://CDPP/Person/Nikolai.Tsyganenko
+ PrincipalInvestigator
+
+
+ spase://SMWG/Person/Elena.Budnik
+ TechnicalContact
+
+
+
+ spase://CDPP/SimulationModel/AMDA/Tsyganenko96
+
+ Earth
+
+
+ Cartesian
+ GSM
+
+ 3
+ km
+
+
+ Orbit
+
+ Ephemeris
+
+
+
+
--
libgit2 0.21.2