From 4a4efaa2ea1f8d9c8dfbd8d86172fb30dac74122 Mon Sep 17 00:00:00 2001 From: Elena.Budnik Date: Thu, 7 Jul 2016 14:51:08 +0200 Subject: [PATCH] work --- NumericalData/AMDA/ACE/MFI/ace-imf-all.xml | 2 +- NumericalData/AMDA/ACE/MFI/ace-mag-real.xml | 2 +- NumericalData/AMDA/ACE/SWEPAM/ace-swe-all.xml | 2 +- NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml | 2 +- NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml | 2 +- NumericalData/AMDA/ACE/ephemeris/ace-orb-all.xml | 2 +- NumericalData/AMDA/Cassini/MAG/Saturn_Orbit/cass-mag-krtphr.xml | 2 +- NumericalData/AMDA/Cassini/MAG/Saturn_Orbit/cass-mag-orb1.xml | 2 +- NumericalData/AMDA/Cluster/Cluster1/EFW/clust1-efw-ppp.xml | 11 ++++++----- NumericalData/AMDA/Cluster/Cluster1/Ephemeris/clust1-orb-all.xml | 2 +- NumericalData/AMDA/Cluster/Cluster2/EFW/clust2-efw-ppp.xml | 13 +++++++------ NumericalData/AMDA/Cluster/Cluster2/Ephemeris/clust2-orb-all.xml | 2 +- NumericalData/AMDA/Cluster/Cluster3/EFW/clust3-efw-ppp.xml | 13 +++++++------ NumericalData/AMDA/Cluster/Cluster3/Ephemeris/clust3-orb-all.xml | 2 +- NumericalData/AMDA/Cluster/Cluster4/EFW/clust4-efw-ppp.xml | 13 +++++++------ NumericalData/AMDA/Cluster/Cluster4/Ephemeris/clust4-orb-all.xml | 2 +- NumericalData/AMDA/Indices/Ground_Based/ground-based-aei.xml | 2 +- NumericalData/AMDA/Indices/Ground_Based/ground-based-asy.xml | 2 +- NumericalData/AMDA/Indices/Ground_Based/ground-based-dst.xml | 2 +- NumericalData/AMDA/Indices/Ground_Based/indices-pc-all.xml | 2 +- NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml | 2 +- NumericalData/AMDA/MAVEN/LPW/mvn-lpw-scpot.xml | 2 +- NumericalData/AMDA/MAVEN/LPW/mvn-lpw-wn.xml | 2 +- NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml | 2 +- NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c0.xml | 4 ++-- NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c6.xml | 4 ++-- NumericalData/AMDA/MAVEN/SWEA/mavpds-swea-svyspec.xml | 4 ++-- NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-momboard.xml | 2 +- NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-specboard.xml | 2 +- NumericalData/AMDA/MEX/ELS/mex-els-all.xml | 2 +- NumericalData/AMDA/MEX/IMA/mex-ima-extra.xml | 2 +- NumericalData/AMDA/MEX/IMA/mex-ima-param.xml | 2 +- NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml | 2 +- NumericalData/AMDA/OMNI/omni-5min-all.xml | 2 +- NumericalData/AMDA/OMNI/omni-hour-all.xml | 2 +- NumericalData/AMDA/Rosetta/Ephemeris/ros-orb-comet.xml | 2 +- NumericalData/AMDA/Rosetta/Ephemeris/sun-pol-cgck.xml | 2 +- NumericalData/AMDA/Rosetta/LAP/ros-lap-est.xml | 2 +- NumericalData/AMDA/Rosetta/LAP/ros-lap1-1d.xml | 2 +- NumericalData/AMDA/Rosetta/LAP/ros-lap1-sweep.xml | 2 +- NumericalData/AMDA/Rosetta/LAP/ros-lap2-1d.xml | 2 +- NumericalData/AMDA/Rosetta/LAP/ros-lap2-sweep.xml | 2 +- Observatory/AMDA/Cluster.xml | 2 +- Observatory/AMDA/Geotail.xml | 4 ++-- 44 files changed, 71 insertions(+), 67 deletions(-) diff --git a/NumericalData/AMDA/ACE/MFI/ace-imf-all.xml b/NumericalData/AMDA/ACE/MFI/ace-imf-all.xml index 5075f45..52bb718 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 - 2016-04-09T23:59:49Z + 2016-06-25T23:59:53Z PT16S diff --git a/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml b/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml index 559c51e..5c5ac50 100644 --- a/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml +++ b/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml @@ -50,7 +50,7 @@ 2014-01-06T00:00:00Z - 2015-08-13T06:59:59Z + 2016-07-06T23:59:59Z PT60S diff --git a/NumericalData/AMDA/ACE/SWEPAM/ace-swe-all.xml b/NumericalData/AMDA/ACE/SWEPAM/ace-swe-all.xml index fef6e27..e1b3fc0 100644 --- a/NumericalData/AMDA/ACE/SWEPAM/ace-swe-all.xml +++ b/NumericalData/AMDA/ACE/SWEPAM/ace-swe-all.xml @@ -58,7 +58,7 @@ 1998-02-04T00:00:31Z - 2013-06-07T23:59:03Z + 2016-01-08T23:59:41Z PT64S diff --git a/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml b/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml index db997eb..1be16bd 100644 --- a/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml +++ b/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml @@ -43,7 +43,7 @@ 2014-01-06T00:00:00Z - 2015-08-13T06:59:59Z + 2016-07-06T23:59:59Z PT60S diff --git a/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml b/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml index e5567b0..eec230c 100644 --- a/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml +++ b/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml @@ -58,7 +58,7 @@ 2001-01-01T00:00:00Z - 2015-08-01T23:55:00Z + 2016-06-25T23:55:00Z PT5M diff --git a/NumericalData/AMDA/ACE/ephemeris/ace-orb-all.xml b/NumericalData/AMDA/ACE/ephemeris/ace-orb-all.xml index 27b5ef8..a9b3d1f 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 - 2016-02-29T23:59:00Z + 2016-08-15T23:47:00Z PT12M diff --git a/NumericalData/AMDA/Cassini/MAG/Saturn_Orbit/cass-mag-krtphr.xml b/NumericalData/AMDA/Cassini/MAG/Saturn_Orbit/cass-mag-krtphr.xml index c46818f..4220821 100644 --- a/NumericalData/AMDA/Cassini/MAG/Saturn_Orbit/cass-mag-krtphr.xml +++ b/NumericalData/AMDA/Cassini/MAG/Saturn_Orbit/cass-mag-krtphr.xml @@ -33,7 +33,7 @@ 2004-05-14T00:00:24Z - 2015-04-01T00:00:09Z + 2015-07-01T00:00:09Z PT0.02S PT0.25S diff --git a/NumericalData/AMDA/Cassini/MAG/Saturn_Orbit/cass-mag-orb1.xml b/NumericalData/AMDA/Cassini/MAG/Saturn_Orbit/cass-mag-orb1.xml index 3253483..a30cb44 100644 --- a/NumericalData/AMDA/Cassini/MAG/Saturn_Orbit/cass-mag-orb1.xml +++ b/NumericalData/AMDA/Cassini/MAG/Saturn_Orbit/cass-mag-orb1.xml @@ -32,7 +32,7 @@ 2004-05-14T18:40:51Z - 2015-03-31T23:59:58Z + 2015-06-30T23:59:58Z PT1S diff --git a/NumericalData/AMDA/Cluster/Cluster1/EFW/clust1-efw-ppp.xml b/NumericalData/AMDA/Cluster/Cluster1/EFW/clust1-efw-ppp.xml index b96b20e..b669452 100644 --- a/NumericalData/AMDA/Cluster/Cluster1/EFW/clust1-efw-ppp.xml +++ b/NumericalData/AMDA/Cluster/Cluster1/EFW/clust1-efw-ppp.xml @@ -7,11 +7,12 @@ prime parameters Cluster 1 Prime Parameter EFW Data 2015-10-16T16:51:44Z - The EFW (Electric Field and Waves) instrument consists of four orthogonal spherical sensors deployed from 50 m cable booms in the spin plane of the spacecraft, plus four deployment units and a main electronics unit. Each deployment unit deploys a multiconductor cable and tip-mounted spherical sensor. Each opposing pair of cables will be symmetrically deployed to a tip-to-tip distance of approximately 100 m, except for about a week at the beginning of the mission when 70 m will be used for one boom pair (the Z-booms) and 100 m for the other pair. The potentials of the spherical sensor and nearby conductors are controlled by the microprocessor to minimize errors associated with photoelectron fluxes to and from the spheres. Output signals from the sensor preamplifiers are provided to the wave instruments for analysis of high frequency wave phenomena. There is a 1 MB burst memory and tow fast A/D conversion circuits for recording electric field wave forms for time resolutions of up to 36,000 samples/s. Data gathered in the burst memory will be played back through the telemetry stream allocated to the instrument by pre-empting a portion of the real-time data. Incoming data are continuously monitored by algorithms in the software to determine whether to trigger the burst-playback mode. A large number of sampling modes is possible, yielding four possible telemetry rates from 1.440-29.440 Kbps. This data stream is transferred via the DWP instrument. The main measured quantities will be, in various modes: (1) the instantaneous spin-plane components of the electric field vector, from 0.1-700 V/Km, with time resolution down to 0.1 ms, in four frequency ranges from DC to upper limits of 10 Hz, 180 Hz, 4 KHz, or 32 KHz; (2) the AC electric field components from 10 Hz to 8 KHz, within the dynamic range of ~3 mV/Km to 10 V/Km; (3) plasma density fluctuations within the range of 1-100/cm and in three frequency ranges from 0 Hz to upper limits of 10 Hz, 180 Hz, or 4 KHz; and, (4) density and temperature (in Langmuir sweeps) in the eV range, with a dynamic range of 1-100/cm. There is also a frequency counter covering the range 10-200 KHz. On-board calculations of least-square fits to the electric field data over one spacecraft spin period (4 s) will provide a baseline of high-quality two-dimensional electric field components that are present in the telemetry stream, except for periods when three or four sensors are in current mode. The spacecraft potential is calculated and transmitted via DWP to other instruments on board. The three components from the search coil instrument (WHISPER) are also available in EFW with a bandwidth of 4 KHz. 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 The Spherical Probe Electric Field and Waves experiment for the Cluster Mission, by G. Gustafsson et al., from which this information was obtained. - NASA, Georg Gustafsson + Preliminary electric field parameters + Please acknowledge the EFW team and ESA CAA in any + publication based upon use of these data - spase://SMWG/Person/Elena.Budnik - TechnicalContact + spase://SMWG/Person/Mats.Andre + PI NSSDC Master Catalog listing for Cluster II Rumba Electric Field and Waves (EFW) @@ -30,7 +31,7 @@ NetCDF NASA, Georg Gustafsson - CSA + CSA : C1_PP_EFW Calibrated Cluster II Rumba Prime Parameter Electric Field and Waves (EFW) Data Calibrated diff --git a/NumericalData/AMDA/Cluster/Cluster1/Ephemeris/clust1-orb-all.xml b/NumericalData/AMDA/Cluster/Cluster1/Ephemeris/clust1-orb-all.xml index 131a863..8209bab 100644 --- a/NumericalData/AMDA/Cluster/Cluster1/Ephemeris/clust1-orb-all.xml +++ b/NumericalData/AMDA/Cluster/Cluster1/Ephemeris/clust1-orb-all.xml @@ -28,7 +28,7 @@ 2000-08-22T00:00:00Z - 2015-08-07T23:24:00Z + 2016-05-09T22:20:00Z PT1M diff --git a/NumericalData/AMDA/Cluster/Cluster2/EFW/clust2-efw-ppp.xml b/NumericalData/AMDA/Cluster/Cluster2/EFW/clust2-efw-ppp.xml index 40d9c33..8699c66 100644 --- a/NumericalData/AMDA/Cluster/Cluster2/EFW/clust2-efw-ppp.xml +++ b/NumericalData/AMDA/Cluster/Cluster2/EFW/clust2-efw-ppp.xml @@ -7,11 +7,12 @@ prime parameters Cluster 2 Prime Parameter EFW Data 2015-10-19T15:51:44Z - The EFW (Electric Field and Waves) instrument consists of four orthogonal spherical sensors deployed from 50 m cable booms in the spin plane of the spacecraft, plus four deployment units and a main electronics unit. Each deployment unit deploys a multiconductor cable and tip-mounted spherical sensor. Each opposing pair of cables will be symmetrically deployed to a tip-to-tip distance of approximately 100 m, except for about a week at the beginning of the mission when 70 m will be used for one boom pair (the Z-booms) and 100 m for the other pair. The potentials of the spherical sensor and nearby conductors are controlled by the microprocessor to minimize errors associated with photoelectron fluxes to and from the spheres. Output signals from the sensor preamplifiers are provided to the wave instruments for analysis of high frequency wave phenomena. There is a 1 MB burst memory and tow fast A/D conversion circuits for recording electric field wave forms for time resolutions of up to 36,000 samples/s. Data gathered in the burst memory will be played back through the telemetry stream allocated to the instrument by pre-empting a portion of the real-time data. Incoming data are continuously monitored by algorithms in the software to determine whether to trigger the burst-playback mode. A large number of sampling modes is possible, yielding four possible telemetry rates from 1.440-29.440 Kbps. This data stream is transferred via the DWP instrument. The main measured quantities will be, in various modes: (1) the instantaneous spin-plane components of the electric field vector, from 0.1-700 V/Km, with time resolution down to 0.1 ms, in four frequency ranges from DC to upper limits of 10 Hz, 180 Hz, 4 KHz, or 32 KHz; (2) the AC electric field components from 10 Hz to 8 KHz, within the dynamic range of ~3 mV/Km to 10 V/Km; (3) plasma density fluctuations within the range of 1-100/cm and in three frequency ranges from 0 Hz to upper limits of 10 Hz, 180 Hz, or 4 KHz; and, (4) density and temperature (in Langmuir sweeps) in the eV range, with a dynamic range of 1-100/cm. There is also a frequency counter covering the range 10-200 KHz. On-board calculations of least-square fits to the electric field data over one spacecraft spin period (4 s) will provide a baseline of high-quality two-dimensional electric field components that are present in the telemetry stream, except for periods when three or four sensors are in current mode. The spacecraft potential is calculated and transmitted via DWP to other instruments on board. The three components from the search coil instrument (WHISPER) are also available in EFW with a bandwidth of 4 KHz. 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 The Spherical Probe Electric Field and Waves experiment for the Cluster Mission, by G. Gustafsson et al., from which this information was obtained. - NASA, Georg Gustafsson + Preliminary electric field parameters + Please acknowledge the EFW team and ESA CAA in any + publication based upon use of these data - spase://SMWG/Person/Elena.Budnik - TechnicalContact + spase://SMWG/Person/Mats.Andre + PI NSSDC Master Catalog listing for Cluster II Salsa Electric Field and Waves (EFW) @@ -28,9 +29,9 @@ http://amda.cdpp.eu NetCDF - NASA, Georg Gustafsson + - CSA + CSA : C2_PP_EFW Calibrated Cluster II Salsa Prime Parameter Electric Field and Waves (EFW) Data Calibrated diff --git a/NumericalData/AMDA/Cluster/Cluster2/Ephemeris/clust2-orb-all.xml b/NumericalData/AMDA/Cluster/Cluster2/Ephemeris/clust2-orb-all.xml index 5a8ec17..8c78e15 100644 --- a/NumericalData/AMDA/Cluster/Cluster2/Ephemeris/clust2-orb-all.xml +++ b/NumericalData/AMDA/Cluster/Cluster2/Ephemeris/clust2-orb-all.xml @@ -28,7 +28,7 @@ 2000-08-22T00:00:00Z - 2015-10-27T00:00:00Z + 2016-05-03T00:00:00Z PT1M diff --git a/NumericalData/AMDA/Cluster/Cluster3/EFW/clust3-efw-ppp.xml b/NumericalData/AMDA/Cluster/Cluster3/EFW/clust3-efw-ppp.xml index 707ee85..60baf93 100644 --- a/NumericalData/AMDA/Cluster/Cluster3/EFW/clust3-efw-ppp.xml +++ b/NumericalData/AMDA/Cluster/Cluster3/EFW/clust3-efw-ppp.xml @@ -7,11 +7,12 @@ prime parameters Cluster 3 Prime Parameter EFW Data 2015-10-19T15:51:44Z - The EFW (Electric Field and Waves) instrument consists of four orthogonal spherical sensors deployed from 50 m cable booms in the spin plane of the spacecraft, plus four deployment units and a main electronics unit. Each deployment unit deploys a multiconductor cable and tip-mounted spherical sensor. Each opposing pair of cables will be symmetrically deployed to a tip-to-tip distance of approximately 100 m, except for about a week at the beginning of the mission when 70 m will be used for one boom pair (the Z-booms) and 100 m for the other pair. The potentials of the spherical sensor and nearby conductors are controlled by the microprocessor to minimize errors associated with photoelectron fluxes to and from the spheres. Output signals from the sensor preamplifiers are provided to the wave instruments for analysis of high frequency wave phenomena. There is a 1 MB burst memory and tow fast A/D conversion circuits for recording electric field wave forms for time resolutions of up to 36,000 samples/s. Data gathered in the burst memory will be played back through the telemetry stream allocated to the instrument by pre-empting a portion of the real-time data. Incoming data are continuously monitored by algorithms in the software to determine whether to trigger the burst-playback mode. A large number of sampling modes is possible, yielding four possible telemetry rates from 1.440-29.440 Kbps. This data stream is transferred via the DWP instrument. The main measured quantities will be, in various modes: (1) the instantaneous spin-plane components of the electric field vector, from 0.1-700 V/Km, with time resolution down to 0.1 ms, in four frequency ranges from DC to upper limits of 10 Hz, 180 Hz, 4 KHz, or 32 KHz; (2) the AC electric field components from 10 Hz to 8 KHz, within the dynamic range of ~3 mV/Km to 10 V/Km; (3) plasma density fluctuations within the range of 1-100/cm and in three frequency ranges from 0 Hz to upper limits of 10 Hz, 180 Hz, or 4 KHz; and, (4) density and temperature (in Langmuir sweeps) in the eV range, with a dynamic range of 1-100/cm. There is also a frequency counter covering the range 10-200 KHz. On-board calculations of least-square fits to the electric field data over one spacecraft spin period (4 s) will provide a baseline of high-quality two-dimensional electric field components that are present in the telemetry stream, except for periods when three or four sensors are in current mode. The spacecraft potential is calculated and transmitted via DWP to other instruments on board. The three components from the search coil instrument (WHISPER) are also available in EFW with a bandwidth of 4 KHz. 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 The Spherical Probe Electric Field and Waves experiment for the Cluster Mission, by G. Gustafsson et al., from which this information was obtained. - NASA, Georg Gustafsson + Preliminary electric field parameters + Please acknowledge the EFW team and ESA CAA in any + publication based upon use of these data - spase://SMWG/Person/Elena.Budnik - TechnicalContact + spase://SMWG/Person/Mats.Andre + PI NSSDC Master Catalog listing for Cluster II Samba Electric Field and Waves (EFW) @@ -28,9 +29,9 @@ http://amda.cdpp.eu NetCDF - NASA, Georg Gustafsson + - CSDS-CNES + CSA : C3_PP_EFW Calibrated Cluster II Samba Prime Parameter Electric Field and Waves (EFW) Data Calibrated diff --git a/NumericalData/AMDA/Cluster/Cluster3/Ephemeris/clust3-orb-all.xml b/NumericalData/AMDA/Cluster/Cluster3/Ephemeris/clust3-orb-all.xml index 0e71fc2..e5135a5 100644 --- a/NumericalData/AMDA/Cluster/Cluster3/Ephemeris/clust3-orb-all.xml +++ b/NumericalData/AMDA/Cluster/Cluster3/Ephemeris/clust3-orb-all.xml @@ -28,7 +28,7 @@ 2000-08-22T00:00:00Z - 2015-10-27T00:00:00Z + 2016-05-03T00:00:00Z PT1M diff --git a/NumericalData/AMDA/Cluster/Cluster4/EFW/clust4-efw-ppp.xml b/NumericalData/AMDA/Cluster/Cluster4/EFW/clust4-efw-ppp.xml index 3b160df..5e455a2 100644 --- a/NumericalData/AMDA/Cluster/Cluster4/EFW/clust4-efw-ppp.xml +++ b/NumericalData/AMDA/Cluster/Cluster4/EFW/clust4-efw-ppp.xml @@ -7,11 +7,12 @@ prime parameters Cluster 4 Prime Parameter EFW Data 2015-10-16T16:51:44Z - The EFW (Electric Field and Waves) instrument consists of four orthogonal spherical sensors deployed from 50 m cable booms in the spin plane of the spacecraft, plus four deployment units and a main electronics unit. Each deployment unit deploys a multiconductor cable and tip-mounted spherical sensor. Each opposing pair of cables will be symmetrically deployed to a tip-to-tip distance of approximately 100 m, except for about a week at the beginning of the mission when 70 m will be used for one boom pair (the Z-booms) and 100 m for the other pair. The potentials of the spherical sensor and nearby conductors are controlled by the microprocessor to minimize errors associated with photoelectron fluxes to and from the spheres. Output signals from the sensor preamplifiers are provided to the wave instruments for analysis of high frequency wave phenomena. There is a 1 MB burst memory and tow fast A/D conversion circuits for recording electric field wave forms for time resolutions of up to 36,000 samples/s. Data gathered in the burst memory will be played back through the telemetry stream allocated to the instrument by pre-empting a portion of the real-time data. Incoming data are continuously monitored by algorithms in the software to determine whether to trigger the burst-playback mode. A large number of sampling modes is possible, yielding four possible telemetry rates from 1.440-29.440 Kbps. This data stream is transferred via the DWP instrument. The main measured quantities will be, in various modes: (1) the instantaneous spin-plane components of the electric field vector, from 0.1-700 V/Km, with time resolution down to 0.1 ms, in four frequency ranges from DC to upper limits of 10 Hz, 180 Hz, 4 KHz, or 32 KHz; (2) the AC electric field components from 10 Hz to 8 KHz, within the dynamic range of ~3 mV/Km to 10 V/Km; (3) plasma density fluctuations within the range of 1-100/cm and in three frequency ranges from 0 Hz to upper limits of 10 Hz, 180 Hz, or 4 KHz; and, (4) density and temperature (in Langmuir sweeps) in the eV range, with a dynamic range of 1-100/cm. There is also a frequency counter covering the range 10-200 KHz. On-board calculations of least-square fits to the electric field data over one spacecraft spin period (4 s) will provide a baseline of high-quality two-dimensional electric field components that are present in the telemetry stream, except for periods when three or four sensors are in current mode. The spacecraft potential is calculated and transmitted via DWP to other instruments on board. The three components from the search coil instrument (WHISPER) are also available in EFW with a bandwidth of 4 KHz. 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 The Spherical Probe Electric Field and Waves experiment for the Cluster Mission, by G. Gustafsson et al., from which this information was obtained. - NASA, Georg Gustafsson + Preliminary electric field parameters + Please acknowledge the EFW team and ESA CAA in any + publication based upon use of these data - spase://SMWG/Person/Elena.Budnik - TechnicalContact + spase://SMWG/Person/Mats.Andre + PI NSSDC Master Catalog listing for Cluster II Tango Electric Field and Waves (EFW) @@ -28,9 +29,9 @@ http://amda.cdpp.eu NetCDF - NASA, Georg Gustafsson + - CSDS-CNES + CSA : C4_PP_EFW Calibrated Cluster II Tango Prime Parameter Electric Field and Waves (EFW) Data Calibrated diff --git a/NumericalData/AMDA/Cluster/Cluster4/Ephemeris/clust4-orb-all.xml b/NumericalData/AMDA/Cluster/Cluster4/Ephemeris/clust4-orb-all.xml index bdc72e3..75b7642 100644 --- a/NumericalData/AMDA/Cluster/Cluster4/Ephemeris/clust4-orb-all.xml +++ b/NumericalData/AMDA/Cluster/Cluster4/Ephemeris/clust4-orb-all.xml @@ -28,7 +28,7 @@ 2000-08-22T00:00:00Z - 2015-11-01T23:59:00Z + 2016-05-09T23:48:00Z PT1M diff --git a/NumericalData/AMDA/Indices/Ground_Based/ground-based-aei.xml b/NumericalData/AMDA/Indices/Ground_Based/ground-based-aei.xml index b7294ae..938bffd 100644 --- a/NumericalData/AMDA/Indices/Ground_Based/ground-based-aei.xml +++ b/NumericalData/AMDA/Indices/Ground_Based/ground-based-aei.xml @@ -49,7 +49,7 @@ 1975-01-01T00:00:00Z - 2015-03-31T23:59:00Z + 2015-11-30T23:59:00Z PT1M diff --git a/NumericalData/AMDA/Indices/Ground_Based/ground-based-asy.xml b/NumericalData/AMDA/Indices/Ground_Based/ground-based-asy.xml index 729cc45..0a8e7da 100644 --- a/NumericalData/AMDA/Indices/Ground_Based/ground-based-asy.xml +++ b/NumericalData/AMDA/Indices/Ground_Based/ground-based-asy.xml @@ -42,7 +42,7 @@ 1981-01-01T00:00:00Z - 2015-04-30T23:59:00Z + 2016-04-30T23:59:00Z PT1M diff --git a/NumericalData/AMDA/Indices/Ground_Based/ground-based-dst.xml b/NumericalData/AMDA/Indices/Ground_Based/ground-based-dst.xml index 54fbd66..ea57867 100644 --- a/NumericalData/AMDA/Indices/Ground_Based/ground-based-dst.xml +++ b/NumericalData/AMDA/Indices/Ground_Based/ground-based-dst.xml @@ -47,7 +47,7 @@ 1970-01-01T00:00:00Z - 2015-04-30T23:59:59Z + 2016-05-31T23:59:59Z PT1H Earth.Magnetosphere.Main diff --git a/NumericalData/AMDA/Indices/Ground_Based/indices-pc-all.xml b/NumericalData/AMDA/Indices/Ground_Based/indices-pc-all.xml index dafbf84..4e7c481 100644 --- a/NumericalData/AMDA/Indices/Ground_Based/indices-pc-all.xml +++ b/NumericalData/AMDA/Indices/Ground_Based/indices-pc-all.xml @@ -49,7 +49,7 @@ 1975-01-01T00:00:00Z - 2015-12-05T23:59:00Z + 2016-05-25T23:59:00Z PT1M diff --git a/NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml b/NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml index 01477a9..37f1018 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 - 2016-03-22T17:16:59Z + 2016-05-17T19:47:00Z PT1M diff --git a/NumericalData/AMDA/MAVEN/LPW/mvn-lpw-scpot.xml b/NumericalData/AMDA/MAVEN/LPW/mvn-lpw-scpot.xml index bca4035..fd5d50a 100644 --- a/NumericalData/AMDA/MAVEN/LPW/mvn-lpw-scpot.xml +++ b/NumericalData/AMDA/MAVEN/LPW/mvn-lpw-scpot.xml @@ -46,7 +46,7 @@ 2014-10-08T00:00:01Z - 2015-08-14T23:59:56Z + 2016-02-15T00:00:01Z PT2S PT4S diff --git a/NumericalData/AMDA/MAVEN/LPW/mvn-lpw-wn.xml b/NumericalData/AMDA/MAVEN/LPW/mvn-lpw-wn.xml index 987e953..fc226cf 100644 --- a/NumericalData/AMDA/MAVEN/LPW/mvn-lpw-wn.xml +++ b/NumericalData/AMDA/MAVEN/LPW/mvn-lpw-wn.xml @@ -46,7 +46,7 @@ 2014-10-06T19:40:30Z - 2015-08-15T00:00:00Z + 2016-02-02T19:29:42Z PT2S PT4S diff --git a/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml b/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml index 8b218f2..d838ce3 100644 --- a/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml +++ b/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml @@ -42,7 +42,7 @@ 2014-10-10T00:00:00Z - 2015-11-15T00:00:01Z + 2016-02-15T00:00:02Z PT0.031SPT8S Mars diff --git a/NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c0.xml b/NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c0.xml index 7287be3..021d13f 100644 --- a/NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c0.xml +++ b/NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c0.xml @@ -41,8 +41,8 @@ IonComposition - 2014-11-15T00:00:19Z - 2015-11-15T00:00:18Z + 2014-10-13T00:00:20Z + 2016-02-15T00:00:11Z PT4S diff --git a/NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c6.xml b/NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c6.xml index 513af94..09b114f 100644 --- a/NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c6.xml +++ b/NumericalData/AMDA/MAVEN/STATIC/mavpds-sta-c6.xml @@ -41,8 +41,8 @@ IonComposition - 2014-11-15T00:00:03Z - 2015-11-15T00:00:02Z + 2014-10-13T00:00:04Z + 2016-02-15T00:00:03Z PT4S diff --git a/NumericalData/AMDA/MAVEN/SWEA/mavpds-swea-svyspec.xml b/NumericalData/AMDA/MAVEN/SWEA/mavpds-swea-svyspec.xml index d3598fe..5c38823 100644 --- a/NumericalData/AMDA/MAVEN/SWEA/mavpds-swea-svyspec.xml +++ b/NumericalData/AMDA/MAVEN/SWEA/mavpds-swea-svyspec.xml @@ -41,8 +41,8 @@ ThermalPlasma - 2014-11-01T00:00:02Z - 2015-11-14T23:59:57Z + 2014-03-19T14:15:52Z + 2016-02-15T00:00:00Z PT4S Mars diff --git a/NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-momboard.xml b/NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-momboard.xml index ef8d324..5f433d3 100644 --- a/NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-momboard.xml +++ b/NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-momboard.xml @@ -42,7 +42,7 @@ 2014-03-19T14:19:43Z - 2015-11-15T00:00:20Z + 2016-02-15T00:00:37Z PT4S Mars diff --git a/NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-specboard.xml b/NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-specboard.xml index e714be1..3a7d761 100644 --- a/NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-specboard.xml +++ b/NumericalData/AMDA/MAVEN/SWIA/mavpds-swia-specboard.xml @@ -42,7 +42,7 @@ 2014-03-19T14:20:43Z - 2015-10-18T00:00:27Z + 2016-02-15T00:00:29Z PT4S Mars diff --git a/NumericalData/AMDA/MEX/ELS/mex-els-all.xml b/NumericalData/AMDA/MEX/ELS/mex-els-all.xml index 03483ad..0c58fee 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 - 2016-01-10T04:54:08Z + 2016-06-06T05:29:07Z PT4S diff --git a/NumericalData/AMDA/MEX/IMA/mex-ima-extra.xml b/NumericalData/AMDA/MEX/IMA/mex-ima-extra.xml index c170a87..93b0391 100644 --- a/NumericalData/AMDA/MEX/IMA/mex-ima-extra.xml +++ b/NumericalData/AMDA/MEX/IMA/mex-ima-extra.xml @@ -33,7 +33,7 @@ 2004-01-05T06:16:06Z - 2016-01-09T17:24:15Z + 2016-05-22T04:21:42Z PT192S diff --git a/NumericalData/AMDA/MEX/IMA/mex-ima-param.xml b/NumericalData/AMDA/MEX/IMA/mex-ima-param.xml index 7d536d8..8493d67 100644 --- a/NumericalData/AMDA/MEX/IMA/mex-ima-param.xml +++ b/NumericalData/AMDA/MEX/IMA/mex-ima-param.xml @@ -27,7 +27,7 @@ 2004-06-26T19:37:50Z - 2016-01-09T17:27:26Z + 2016-05-22T04:21:41Z PT192S diff --git a/NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml b/NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml index 983349b..105ff1b 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 - 2016-03-11T07:16:20Z + 2016-07-31T13:17:49Z PT60S diff --git a/NumericalData/AMDA/OMNI/omni-5min-all.xml b/NumericalData/AMDA/OMNI/omni-5min-all.xml index 3dd9b98..a6dc968 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 - 2015-12-31T23:55:00Z + 2016-06-12T23:55:00Z PT5M diff --git a/NumericalData/AMDA/OMNI/omni-hour-all.xml b/NumericalData/AMDA/OMNI/omni-hour-all.xml index 4baac33..5ff19f0 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 - 2016-03-15T23:00:00Z + 2016-06-13T13:00:00Z PT1H diff --git a/NumericalData/AMDA/Rosetta/Ephemeris/ros-orb-comet.xml b/NumericalData/AMDA/Rosetta/Ephemeris/ros-orb-comet.xml index 2c66928..e39ec82 100644 --- a/NumericalData/AMDA/Rosetta/Ephemeris/ros-orb-comet.xml +++ b/NumericalData/AMDA/Rosetta/Ephemeris/ros-orb-comet.xml @@ -82,7 +82,7 @@ 2014-01-01T00:00:00Z - 2015-11-17T23:59:00Z + 2016-06-25T23:59:00Z PT60S diff --git a/NumericalData/AMDA/Rosetta/Ephemeris/sun-pol-cgck.xml b/NumericalData/AMDA/Rosetta/Ephemeris/sun-pol-cgck.xml index 7f3ca20..136713e 100644 --- a/NumericalData/AMDA/Rosetta/Ephemeris/sun-pol-cgck.xml +++ b/NumericalData/AMDA/Rosetta/Ephemeris/sun-pol-cgck.xml @@ -28,7 +28,7 @@ 2014-01-01T00:00:00Z - 2016-03-04T23:59:00Z + 2016-07-16T23:59:00Z PT60S diff --git a/NumericalData/AMDA/Rosetta/LAP/ros-lap-est.xml b/NumericalData/AMDA/Rosetta/LAP/ros-lap-est.xml index eaff611..953c78f 100644 --- a/NumericalData/AMDA/Rosetta/LAP/ros-lap-est.xml +++ b/NumericalData/AMDA/Rosetta/LAP/ros-lap-est.xml @@ -42,7 +42,7 @@ 2014-05-09T15:23:00Z - 2016-04-15T01:38:09Z + 2016-05-28T02:30:26Z 4s512 diff --git a/NumericalData/AMDA/Rosetta/LAP/ros-lap1-1d.xml b/NumericalData/AMDA/Rosetta/LAP/ros-lap1-1d.xml index 85c29ca..b3ede9f 100644 --- a/NumericalData/AMDA/Rosetta/LAP/ros-lap1-1d.xml +++ b/NumericalData/AMDA/Rosetta/LAP/ros-lap1-1d.xml @@ -42,7 +42,7 @@ 2014-05-09T15:22:56Z - 2016-04-15T01:40:00Z + 2016-05-28T02:34:24Z 32s diff --git a/NumericalData/AMDA/Rosetta/LAP/ros-lap1-sweep.xml b/NumericalData/AMDA/Rosetta/LAP/ros-lap1-sweep.xml index 38f5d34..6742148 100644 --- a/NumericalData/AMDA/Rosetta/LAP/ros-lap1-sweep.xml +++ b/NumericalData/AMDA/Rosetta/LAP/ros-lap1-sweep.xml @@ -42,7 +42,7 @@ 2014-05-09T15:23:00Z - 2016-04-15T01:40:16Z + 2016-05-28T02:32:33Z 64s512 diff --git a/NumericalData/AMDA/Rosetta/LAP/ros-lap2-1d.xml b/NumericalData/AMDA/Rosetta/LAP/ros-lap2-1d.xml index 39f1a18..71000bf 100644 --- a/NumericalData/AMDA/Rosetta/LAP/ros-lap2-1d.xml +++ b/NumericalData/AMDA/Rosetta/LAP/ros-lap2-1d.xml @@ -42,7 +42,7 @@ 2014-05-09T15:22:56Z - 2016-04-15T01:40:00Z + 2016-05-28T02:34:24Z 32s diff --git a/NumericalData/AMDA/Rosetta/LAP/ros-lap2-sweep.xml b/NumericalData/AMDA/Rosetta/LAP/ros-lap2-sweep.xml index 3067ae0..4b4c1ec 100644 --- a/NumericalData/AMDA/Rosetta/LAP/ros-lap2-sweep.xml +++ b/NumericalData/AMDA/Rosetta/LAP/ros-lap2-sweep.xml @@ -42,7 +42,7 @@ 2014-05-09T15:23:32Z - 2016-04-15T01:38:08Z + 2016-05-28T02:33:05Z 64s512 diff --git a/Observatory/AMDA/Cluster.xml b/Observatory/AMDA/Cluster.xml index aecaf77..e52599b 100644 --- a/Observatory/AMDA/Cluster.xml +++ b/Observatory/AMDA/Cluster.xml @@ -5,7 +5,7 @@ spase://CDPP/Observatory/AMDA/Cluster Cluster - Cluster II, ESA Magnetospheric Mission + Cluster, ESA Magnetospheric Mission 2011-02-07T00:50:41Z Cluster is a constellation of four spacecraft flying in formation around Earth. They relay the most detailed information ever about diff --git a/Observatory/AMDA/Geotail.xml b/Observatory/AMDA/Geotail.xml index e1b3d65..1ac7ed1 100644 --- a/Observatory/AMDA/Geotail.xml +++ b/Observatory/AMDA/Geotail.xml @@ -5,11 +5,11 @@ spase://CDPP/Observatory/AMDA/Geotail Geotail + Geomagnetic Tail Lab 1992-044A GTL ISTP/Geotail - GGS/Geotail - Geomagnetic Tail Lab + GGS/Geotail 2010-08-05T18:19:18Z The solar wind draws the Earth's magnetic field into a long tail on the nightside of the Earth and stores energy in the stretched field lines of the magnetotail. During active periods, the tail couples with the near-Earth magnetosphere, sometimes releasing energy stored in the tail and activating auroras in the polar ionosphere. The Geotail mission measures global energy flow and transformation in the magnetotail to increase understanding of fundamental magnetospheric processes. This includes the physics of the magnetopause magnetospheric boundary regions, the lobe and plasma sheet, and reconnection and neutral line formation, i.e., the mechanisms processes of input, transport, storage, release and conversion of mass, momentum and energy in the magnetotail. -- libgit2 0.21.2