diff --git a/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad.xml b/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad.xml
index f8f3d2a..78ea8e3 100644
--- a/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad.xml
+++ b/NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad.xml
@@ -6,7 +6,7 @@
<ResourceHeader>
<ResourceName>pitch-angle/energy distribution</ResourceName>
<AlternateName>2D Pitch-Angle/Energy distribution</AlternateName>
- <ReleaseDate>2015-10-19T10:51:45Z</ReleaseDate>
+ <ReleaseDate>2019-01-21T15:50:31Z</ReleaseDate>
<Description>Pitch-angle distributions (PADs) are given in particle flux units, as a function of the particle energy and pitch-angle (2D distributions), and their resolution is in 16 angular sectors covering the pitch angle range from 0° to 180°.
PADs are calculated for HIA magnetospheric modes. The dataset is provided with 31 energy bins resolution</Description>
<Acknowledgement>Principal Investigator: Dr. Iannis Dandouras</Acknowledgement>
@@ -42,7 +42,8 @@
<StartDate>2001-01-31T01:02:11Z</StartDate>
<StopDate>2015-12-29T14:04:21Z</StopDate>
</TimeSpan>
- <Cadence>PT4S</Cadence>
+ <Cadence_Min>PT4S</Cadence_Min>
+ <Cadence_Max>PT16S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosheath</ObservedRegion>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
@@ -71,7 +72,6 @@
<ParameterKey>c1_hia_pad</ParameterKey>
<Description>Hot ion pitch angle distribution</Description>
<Ucd/>
- <Cadence>PT4S</Cadence>
<Units>1/(cm**2-s-sr-keV)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
diff --git a/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-pad.xml b/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-pad.xml
index 372ea63..8067f41 100644
--- a/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-pad.xml
+++ b/NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-pad.xml
@@ -6,7 +6,7 @@
<ResourceHeader>
<ResourceName>pitch-angle/energy distribution</ResourceName>
<AlternateName>2D Pitch-Angle/Energy distribution</AlternateName>
- <ReleaseDate>2016-10-19T10:51:45Z</ReleaseDate>
+ <ReleaseDate>2017-07-03T10:19:25Z</ReleaseDate>
<Description>Pitch-angle distributions (PADs) are given in particle flux units, as a function of the particle energy and pitch-angle (2D distributions), and their resolution is in 16 angular sectors covering the pitch angle range from 0° to 180°.
PADs are calculated for HIA magnetospheric modes. The dataset is provided with 31 energy bins resolution</Description>
<Acknowledgement>Principal Investigator: Dr. Iannis Dandouras</Acknowledgement>
@@ -42,7 +42,8 @@
<StartDate>2001-01-31T01:02:10Z</StartDate>
<StopDate>2009-11-11T08:17:05Z</StopDate>
</TimeSpan>
- <Cadence>PT4S</Cadence>
+ <Cadence_Min>PT4S</Cadence_Min>
+ <Cadence_Max>PT16S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosheath</ObservedRegion>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
diff --git a/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2e.xml b/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2e.xml
index 5c71f21..adbcd3e 100644
--- a/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2e.xml
+++ b/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2e.xml
@@ -5,7 +5,7 @@
<ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2e</ResourceID>
<ResourceHeader>
<ResourceName>electron full mode</ResourceName>
- <ReleaseDate>2017-03-13T15:12:00</ReleaseDate>
+ <ReleaseDate>2019-03-10T21:07:55Z</ReleaseDate>
<Description/>
<Contact>
<PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -32,9 +32,10 @@
<TemporalDescription>
<TimeSpan>
<StartDate>2007-03-07T18:53:59Z</StartDate>
- <StopDate>2019-01-22T15:12:50Z</StopDate>
+ <StopDate>2019-03-09T06:12:30Z</StopDate>
</TimeSpan>
- <Cadence>PT96.27S</Cadence>
+ <Cadence_Min>PT96.27S</Cadence_Min>
+ <Cadence_Max>PT385.09S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
<Parameter>
diff --git a/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2i.xml b/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2i.xml
index 032bcc3..c42da43 100644
--- a/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2i.xml
+++ b/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2i.xml
@@ -2,10 +2,10 @@
<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://cdpp.irap.omp.eu/AMDA-NG/public/schemas/spase-amda-1_2_0.xsd">
<Version>2.2.6</Version>
<NumericalData>
- <ResourceID>spase://CDPP/NumericalData/AMDA/thaMIS/A/ESA/tha-esa-l2i</ResourceID>
+ <ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2i</ResourceID>
<ResourceHeader>
<ResourceName>ion full mode</ResourceName>
- <ReleaseDate>2017-03-13T15:42:30</ReleaseDate>
+ <ReleaseDate>2019-03-10T21:07:54Z</ReleaseDate>
<Description>"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").</Description>
<Contact>
<PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -32,9 +32,10 @@
<TemporalDescription>
<TimeSpan>
<StartDate>2007-03-07T18:53:59Z</StartDate>
- <StopDate>2019-01-22T15:12:36Z</StopDate>
+ <StopDate>2019-03-09T06:12:41Z</StopDate>
</TimeSpan>
- <Cadence>PT96.27S</Cadence>
+ <Cadence_Min>PT96.27S</Cadence_Min>
+ <Cadence_Max>PT385.09S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
<Parameter>
diff --git a/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2e.xml b/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2e.xml
index 58d5d3d..c59604a 100644
--- a/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2e.xml
+++ b/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2e.xml
@@ -5,7 +5,7 @@
<ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2e</ResourceID>
<ResourceHeader>
<ResourceName>electron full mode</ResourceName>
- <ReleaseDate>2015-10-13T15:12:00</ReleaseDate>
+ <ReleaseDate>2019-03-10T21:08:18Z</ReleaseDate>
<Description/>
<Contact>
<PersonID>spase://SMWG/Person/Elena.budnik</PersonID>
@@ -28,9 +28,10 @@
<TemporalDescription>
<TimeSpan>
<StartDate>2007-03-07T17:55:08Z</StartDate>
- <StopDate>2019-01-22T16:02:55Z</StopDate>
+ <StopDate>2019-03-09T08:20:19Z</StopDate>
</TimeSpan>
- <Cadence>PT96.27S</Cadence>
+ <Cadence_Min>PT96.27S</Cadence_Min>
+ <Cadence_Max>PT385.09S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
<Parameter>
diff --git a/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2i.xml b/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2i.xml
index 46b763e..d2a966a 100644
--- a/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2i.xml
+++ b/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2i.xml
@@ -5,7 +5,7 @@
<ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2i</ResourceID>
<ResourceHeader>
<ResourceName>ion full mode</ResourceName>
- <ReleaseDate>2015-10-13T15:42:30</ReleaseDate>
+ <ReleaseDate>2019-03-10T21:08:17Z</ReleaseDate>
<Description>"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").></Description>
<Contact>
<PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -32,9 +32,10 @@
<TemporalDescription>
<TimeSpan>
<StartDate>2007-03-07T17:55:08Z</StartDate>
- <StopDate>2019-01-22T16:01:34Z</StopDate>
+ <StopDate>2019-03-09T08:20:53Z</StopDate>
</TimeSpan>
- <Cadence>PT96.27S</Cadence>
+ <Cadence_Min>PT96.27S</Cadence_Min>
+ <Cadence_Max>PT385.09S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
<Parameter>
diff --git a/NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2e.xml b/NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2e.xml
index 3774f99..c04c605 100644
--- a/NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2e.xml
+++ b/NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2e.xml
@@ -5,7 +5,7 @@
<ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2e</ResourceID>
<ResourceHeader>
<ResourceName>electron full mode</ResourceName>
- <ReleaseDate>2015-10-13T15:12:00</ReleaseDate>
+ <ReleaseDate>2019-03-10T21:08:42Z</ReleaseDate>
<Description/>
<Contact>
<PersonID>spase://SMWG/Person/Elena.budnik</PersonID>
@@ -28,9 +28,10 @@
<TemporalDescription>
<TimeSpan>
<StartDate>2007-03-07T15:58:39Z</StartDate>
- <StopDate>2019-01-22T21:40:15Z</StopDate>
+ <StopDate>2019-03-09T01:37:27Z</StopDate>
</TimeSpan>
- <Cadence>PT96.27S</Cadence>
+ <Cadence_Min>PT96.27S</Cadence_Min>
+ <Cadence_Max>PT385.09S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
<Parameter>
diff --git a/NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2i.xml b/NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2i.xml
index 7edd090..7b66bcb 100644
--- a/NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2i.xml
+++ b/NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2i.xml
@@ -5,7 +5,7 @@
<ResourceID>spase://CDPP/NumericalData/AMDA/thaMIS/C/ESA/thc-esa-l2i</ResourceID>
<ResourceHeader>
<ResourceName>ion full mode</ResourceName>
- <ReleaseDate>2017-03-13T15:42:30</ReleaseDate>
+ <ReleaseDate>2019-03-10T21:08:42Z</ReleaseDate>
<Description>"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").</Description>
<Contact>
<PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -32,9 +32,10 @@
<TemporalDescription>
<TimeSpan>
<StartDate>2007-03-07T15:58:39Z</StartDate>
- <StopDate>2019-01-22T21:38:49Z</StopDate>
+ <StopDate>2019-03-09T01:37:35Z</StopDate>
</TimeSpan>
- <Cadence>PT96.27S</Cadence>
+ <Cadence_Min>PT96.27S</Cadence_Min>
+ <Cadence_Max>PT385.09S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
<Parameter>
diff --git a/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2e.xml b/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2e.xml
index c4f2ce2..437a013 100644
--- a/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2e.xml
+++ b/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2e.xml
@@ -5,7 +5,7 @@
<ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2e</ResourceID>
<ResourceHeader>
<ResourceName>electron full mode</ResourceName>
- <ReleaseDate>2015-10-13T15:12:00</ReleaseDate>
+ <ReleaseDate>2019-03-10T21:09:12Z</ReleaseDate>
<Description/>
<Contact>
<PersonID>spase://SMWG/Person/Elena.budnik</PersonID>
@@ -28,9 +28,10 @@
<TemporalDescription>
<TimeSpan>
<StartDate>2007-03-07T16:54:49Z</StartDate>
- <StopDate>2019-01-21T00:11:04Z</StopDate>
+ <StopDate>2019-03-08T23:55:47Z</StopDate>
</TimeSpan>
- <Cadence>PT96.27S</Cadence>
+ <Cadence_Min>PT96.27S</Cadence_Min>
+ <Cadence_Max>PT385.09S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
<Parameter>
diff --git a/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2i.xml b/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2i.xml
index 949ef32..cbba869 100644
--- a/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2i.xml
+++ b/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2i.xml
@@ -5,7 +5,7 @@
<ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2i</ResourceID>
<ResourceHeader>
<ResourceName>ion full mode</ResourceName>
- <ReleaseDate>2017-03-13T15:42:30</ReleaseDate>
+ <ReleaseDate>2019-03-10T21:09:10Z</ReleaseDate>
<Description>"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").</Description>
<Contact>
<PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -32,9 +32,10 @@
<TemporalDescription>
<TimeSpan>
<StartDate>2007-03-07T16:54:49Z</StartDate>
- <StopDate>2019-01-21T00:10:37Z</StopDate>
+ <StopDate>2019-03-08T23:54:13Z</StopDate>
</TimeSpan>
- <Cadence>PT96.27S</Cadence>
+ <Cadence_Min>PT96.27S</Cadence_Min>
+ <Cadence_Max>PT385.09S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
<Parameter>
diff --git a/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2e.xml b/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2e.xml
index 34c4462..3a99dec 100644
--- a/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2e.xml
+++ b/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2e.xml
@@ -5,7 +5,7 @@
<ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2e</ResourceID>
<ResourceHeader>
<ResourceName>electron full mode</ResourceName>
- <ReleaseDate>2015-10-13T15:12:00</ReleaseDate>
+ <ReleaseDate>2019-03-10T21:09:42Z</ReleaseDate>
<Description/>
<Contact>
<PersonID>spase://SMWG/Person/Elena.budnik</PersonID>
@@ -28,9 +28,10 @@
<TemporalDescription>
<TimeSpan>
<StartDate>2007-03-07T19:54:48Z</StartDate>
- <StopDate>2019-01-21T14:27:05Z</StopDate>
+ <StopDate>2019-03-08T13:23:36Z</StopDate>
</TimeSpan>
- <Cadence>PT96.27S</Cadence>
+ <Cadence_Min>PT96.27S</Cadence_Min>
+ <Cadence_Max>PT385.09S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
<Parameter>
diff --git a/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2i.xml b/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2i.xml
index 054a1d4..c96c686 100644
--- a/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2i.xml
+++ b/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2i.xml
@@ -5,7 +5,7 @@
<ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2i</ResourceID>
<ResourceHeader>
<ResourceName>ion full mode</ResourceName>
- <ReleaseDate>2017-03-13T15:42:30</ReleaseDate>
+ <ReleaseDate>2019-03-10T21:09:42Z</ReleaseDate>
<Description>"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").</Description>
<Contact>
<PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID>
@@ -32,9 +32,10 @@
<TemporalDescription>
<TimeSpan>
<StartDate>2007-03-07T19:54:48Z</StartDate>
- <StopDate>2019-01-21T14:26:19Z</StopDate>
+ <StopDate>2019-03-08T13:22:55Z</StopDate>
</TimeSpan>
- <Cadence>PT96.27S</Cadence>
+ <Cadence_Min>PT96.27S</Cadence_Min>
+ <Cadence_Max>PT385.09S</Cadence_Max>
</TemporalDescription>
<ObservedRegion>Earth.Magnetosphere</ObservedRegion>
<Parameter>
--
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