Commit 6e10a02897b1339b07530b99fc05964c824325c0
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min / max samplig Cluster, Themis
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NumericalData/AMDA/Cluster/Cluster1/CIS-HIA/clust1-hia-pad.xml
... | ... | @@ -6,7 +6,7 @@ |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>pitch-angle/energy distribution</ResourceName> |
8 | 8 | <AlternateName>2D Pitch-Angle/Energy distribution</AlternateName> |
9 | - <ReleaseDate>2015-10-19T10:51:45Z</ReleaseDate> | |
9 | + <ReleaseDate>2019-01-21T15:50:31Z</ReleaseDate> | |
10 | 10 | <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°. |
11 | 11 | PADs are calculated for HIA magnetospheric modes. The dataset is provided with 31 energy bins resolution</Description> |
12 | 12 | <Acknowledgement>Principal Investigator: Dr. Iannis Dandouras</Acknowledgement> |
... | ... | @@ -42,7 +42,8 @@ |
42 | 42 | <StartDate>2001-01-31T01:02:11Z</StartDate> |
43 | 43 | <StopDate>2015-12-29T14:04:21Z</StopDate> |
44 | 44 | </TimeSpan> |
45 | - <Cadence>PT4S</Cadence> | |
45 | + <Cadence_Min>PT4S</Cadence_Min> | |
46 | + <Cadence_Max>PT16S</Cadence_Max> | |
46 | 47 | </TemporalDescription> |
47 | 48 | <ObservedRegion>Earth.Magnetosheath</ObservedRegion> |
48 | 49 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
... | ... | @@ -71,7 +72,6 @@ |
71 | 72 | <ParameterKey>c1_hia_pad</ParameterKey> |
72 | 73 | <Description>Hot ion pitch angle distribution</Description> |
73 | 74 | <Ucd/> |
74 | - <Cadence>PT4S</Cadence> | |
75 | 75 | <Units>1/(cm**2-s-sr-keV)</Units> |
76 | 76 | <RenderingHints> |
77 | 77 | <DisplayType>Spectrogram</DisplayType> |
... | ... |
NumericalData/AMDA/Cluster/Cluster3/CIS-HIA/clust3-hia-pad.xml
... | ... | @@ -6,7 +6,7 @@ |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>pitch-angle/energy distribution</ResourceName> |
8 | 8 | <AlternateName>2D Pitch-Angle/Energy distribution</AlternateName> |
9 | - <ReleaseDate>2016-10-19T10:51:45Z</ReleaseDate> | |
9 | + <ReleaseDate>2017-07-03T10:19:25Z</ReleaseDate> | |
10 | 10 | <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°. |
11 | 11 | PADs are calculated for HIA magnetospheric modes. The dataset is provided with 31 energy bins resolution</Description> |
12 | 12 | <Acknowledgement>Principal Investigator: Dr. Iannis Dandouras</Acknowledgement> |
... | ... | @@ -42,7 +42,8 @@ |
42 | 42 | <StartDate>2001-01-31T01:02:10Z</StartDate> |
43 | 43 | <StopDate>2009-11-11T08:17:05Z</StopDate> |
44 | 44 | </TimeSpan> |
45 | - <Cadence>PT4S</Cadence> | |
45 | + <Cadence_Min>PT4S</Cadence_Min> | |
46 | + <Cadence_Max>PT16S</Cadence_Max> | |
46 | 47 | </TemporalDescription> |
47 | 48 | <ObservedRegion>Earth.Magnetosheath</ObservedRegion> |
48 | 49 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
... | ... |
NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2e.xml
... | ... | @@ -5,7 +5,7 @@ |
5 | 5 | <ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2e</ResourceID> |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>electron full mode</ResourceName> |
8 | - <ReleaseDate>2017-03-13T15:12:00</ReleaseDate> | |
8 | + <ReleaseDate>2019-03-10T21:07:55Z</ReleaseDate> | |
9 | 9 | <Description/> |
10 | 10 | <Contact> |
11 | 11 | <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID> |
... | ... | @@ -32,9 +32,10 @@ |
32 | 32 | <TemporalDescription> |
33 | 33 | <TimeSpan> |
34 | 34 | <StartDate>2007-03-07T18:53:59Z</StartDate> |
35 | - <StopDate>2019-01-22T15:12:50Z</StopDate> | |
35 | + <StopDate>2019-03-09T06:12:30Z</StopDate> | |
36 | 36 | </TimeSpan> |
37 | - <Cadence>PT96.27S</Cadence> | |
37 | + <Cadence_Min>PT96.27S</Cadence_Min> | |
38 | + <Cadence_Max>PT385.09S</Cadence_Max> | |
38 | 39 | </TemporalDescription> |
39 | 40 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
40 | 41 | <Parameter> |
... | ... |
NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2i.xml
... | ... | @@ -2,10 +2,10 @@ |
2 | 2 | <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"> |
3 | 3 | <Version>2.2.6</Version> |
4 | 4 | <NumericalData> |
5 | - <ResourceID>spase://CDPP/NumericalData/AMDA/thaMIS/A/ESA/tha-esa-l2i</ResourceID> | |
5 | + <ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/A/ESA/tha-esa-l2i</ResourceID> | |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>ion full mode</ResourceName> |
8 | - <ReleaseDate>2017-03-13T15:42:30</ReleaseDate> | |
8 | + <ReleaseDate>2019-03-10T21:07:54Z</ReleaseDate> | |
9 | 9 | <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> |
10 | 10 | <Contact> |
11 | 11 | <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID> |
... | ... | @@ -32,9 +32,10 @@ |
32 | 32 | <TemporalDescription> |
33 | 33 | <TimeSpan> |
34 | 34 | <StartDate>2007-03-07T18:53:59Z</StartDate> |
35 | - <StopDate>2019-01-22T15:12:36Z</StopDate> | |
35 | + <StopDate>2019-03-09T06:12:41Z</StopDate> | |
36 | 36 | </TimeSpan> |
37 | - <Cadence>PT96.27S</Cadence> | |
37 | + <Cadence_Min>PT96.27S</Cadence_Min> | |
38 | + <Cadence_Max>PT385.09S</Cadence_Max> | |
38 | 39 | </TemporalDescription> |
39 | 40 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
40 | 41 | <Parameter> |
... | ... |
NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2e.xml
... | ... | @@ -5,7 +5,7 @@ |
5 | 5 | <ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2e</ResourceID> |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>electron full mode</ResourceName> |
8 | - <ReleaseDate>2015-10-13T15:12:00</ReleaseDate> | |
8 | + <ReleaseDate>2019-03-10T21:08:18Z</ReleaseDate> | |
9 | 9 | <Description/> |
10 | 10 | <Contact> |
11 | 11 | <PersonID>spase://SMWG/Person/Elena.budnik</PersonID> |
... | ... | @@ -28,9 +28,10 @@ |
28 | 28 | <TemporalDescription> |
29 | 29 | <TimeSpan> |
30 | 30 | <StartDate>2007-03-07T17:55:08Z</StartDate> |
31 | - <StopDate>2019-01-22T16:02:55Z</StopDate> | |
31 | + <StopDate>2019-03-09T08:20:19Z</StopDate> | |
32 | 32 | </TimeSpan> |
33 | - <Cadence>PT96.27S</Cadence> | |
33 | + <Cadence_Min>PT96.27S</Cadence_Min> | |
34 | + <Cadence_Max>PT385.09S</Cadence_Max> | |
34 | 35 | </TemporalDescription> |
35 | 36 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
36 | 37 | <Parameter> |
... | ... |
NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2i.xml
... | ... | @@ -5,7 +5,7 @@ |
5 | 5 | <ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/B/ESA/thb-esa-l2i</ResourceID> |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>ion full mode</ResourceName> |
8 | - <ReleaseDate>2015-10-13T15:42:30</ReleaseDate> | |
8 | + <ReleaseDate>2019-03-10T21:08:17Z</ReleaseDate> | |
9 | 9 | <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> |
10 | 10 | <Contact> |
11 | 11 | <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID> |
... | ... | @@ -32,9 +32,10 @@ |
32 | 32 | <TemporalDescription> |
33 | 33 | <TimeSpan> |
34 | 34 | <StartDate>2007-03-07T17:55:08Z</StartDate> |
35 | - <StopDate>2019-01-22T16:01:34Z</StopDate> | |
35 | + <StopDate>2019-03-09T08:20:53Z</StopDate> | |
36 | 36 | </TimeSpan> |
37 | - <Cadence>PT96.27S</Cadence> | |
37 | + <Cadence_Min>PT96.27S</Cadence_Min> | |
38 | + <Cadence_Max>PT385.09S</Cadence_Max> | |
38 | 39 | </TemporalDescription> |
39 | 40 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
40 | 41 | <Parameter> |
... | ... |
NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2e.xml
... | ... | @@ -5,7 +5,7 @@ |
5 | 5 | <ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2e</ResourceID> |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>electron full mode</ResourceName> |
8 | - <ReleaseDate>2015-10-13T15:12:00</ReleaseDate> | |
8 | + <ReleaseDate>2019-03-10T21:08:42Z</ReleaseDate> | |
9 | 9 | <Description/> |
10 | 10 | <Contact> |
11 | 11 | <PersonID>spase://SMWG/Person/Elena.budnik</PersonID> |
... | ... | @@ -28,9 +28,10 @@ |
28 | 28 | <TemporalDescription> |
29 | 29 | <TimeSpan> |
30 | 30 | <StartDate>2007-03-07T15:58:39Z</StartDate> |
31 | - <StopDate>2019-01-22T21:40:15Z</StopDate> | |
31 | + <StopDate>2019-03-09T01:37:27Z</StopDate> | |
32 | 32 | </TimeSpan> |
33 | - <Cadence>PT96.27S</Cadence> | |
33 | + <Cadence_Min>PT96.27S</Cadence_Min> | |
34 | + <Cadence_Max>PT385.09S</Cadence_Max> | |
34 | 35 | </TemporalDescription> |
35 | 36 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
36 | 37 | <Parameter> |
... | ... |
NumericalData/AMDA/THEMIS/C/ESA/thc-esa-l2i.xml
... | ... | @@ -5,7 +5,7 @@ |
5 | 5 | <ResourceID>spase://CDPP/NumericalData/AMDA/thaMIS/C/ESA/thc-esa-l2i</ResourceID> |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>ion full mode</ResourceName> |
8 | - <ReleaseDate>2017-03-13T15:42:30</ReleaseDate> | |
8 | + <ReleaseDate>2019-03-10T21:08:42Z</ReleaseDate> | |
9 | 9 | <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> |
10 | 10 | <Contact> |
11 | 11 | <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID> |
... | ... | @@ -32,9 +32,10 @@ |
32 | 32 | <TemporalDescription> |
33 | 33 | <TimeSpan> |
34 | 34 | <StartDate>2007-03-07T15:58:39Z</StartDate> |
35 | - <StopDate>2019-01-22T21:38:49Z</StopDate> | |
35 | + <StopDate>2019-03-09T01:37:35Z</StopDate> | |
36 | 36 | </TimeSpan> |
37 | - <Cadence>PT96.27S</Cadence> | |
37 | + <Cadence_Min>PT96.27S</Cadence_Min> | |
38 | + <Cadence_Max>PT385.09S</Cadence_Max> | |
38 | 39 | </TemporalDescription> |
39 | 40 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
40 | 41 | <Parameter> |
... | ... |
NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2e.xml
... | ... | @@ -5,7 +5,7 @@ |
5 | 5 | <ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2e</ResourceID> |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>electron full mode</ResourceName> |
8 | - <ReleaseDate>2015-10-13T15:12:00</ReleaseDate> | |
8 | + <ReleaseDate>2019-03-10T21:09:12Z</ReleaseDate> | |
9 | 9 | <Description/> |
10 | 10 | <Contact> |
11 | 11 | <PersonID>spase://SMWG/Person/Elena.budnik</PersonID> |
... | ... | @@ -28,9 +28,10 @@ |
28 | 28 | <TemporalDescription> |
29 | 29 | <TimeSpan> |
30 | 30 | <StartDate>2007-03-07T16:54:49Z</StartDate> |
31 | - <StopDate>2019-01-21T00:11:04Z</StopDate> | |
31 | + <StopDate>2019-03-08T23:55:47Z</StopDate> | |
32 | 32 | </TimeSpan> |
33 | - <Cadence>PT96.27S</Cadence> | |
33 | + <Cadence_Min>PT96.27S</Cadence_Min> | |
34 | + <Cadence_Max>PT385.09S</Cadence_Max> | |
34 | 35 | </TemporalDescription> |
35 | 36 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
36 | 37 | <Parameter> |
... | ... |
NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2i.xml
... | ... | @@ -5,7 +5,7 @@ |
5 | 5 | <ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/D/ESA/thd-esa-l2i</ResourceID> |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>ion full mode</ResourceName> |
8 | - <ReleaseDate>2017-03-13T15:42:30</ReleaseDate> | |
8 | + <ReleaseDate>2019-03-10T21:09:10Z</ReleaseDate> | |
9 | 9 | <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> |
10 | 10 | <Contact> |
11 | 11 | <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID> |
... | ... | @@ -32,9 +32,10 @@ |
32 | 32 | <TemporalDescription> |
33 | 33 | <TimeSpan> |
34 | 34 | <StartDate>2007-03-07T16:54:49Z</StartDate> |
35 | - <StopDate>2019-01-21T00:10:37Z</StopDate> | |
35 | + <StopDate>2019-03-08T23:54:13Z</StopDate> | |
36 | 36 | </TimeSpan> |
37 | - <Cadence>PT96.27S</Cadence> | |
37 | + <Cadence_Min>PT96.27S</Cadence_Min> | |
38 | + <Cadence_Max>PT385.09S</Cadence_Max> | |
38 | 39 | </TemporalDescription> |
39 | 40 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
40 | 41 | <Parameter> |
... | ... |
NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2e.xml
... | ... | @@ -5,7 +5,7 @@ |
5 | 5 | <ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2e</ResourceID> |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>electron full mode</ResourceName> |
8 | - <ReleaseDate>2015-10-13T15:12:00</ReleaseDate> | |
8 | + <ReleaseDate>2019-03-10T21:09:42Z</ReleaseDate> | |
9 | 9 | <Description/> |
10 | 10 | <Contact> |
11 | 11 | <PersonID>spase://SMWG/Person/Elena.budnik</PersonID> |
... | ... | @@ -28,9 +28,10 @@ |
28 | 28 | <TemporalDescription> |
29 | 29 | <TimeSpan> |
30 | 30 | <StartDate>2007-03-07T19:54:48Z</StartDate> |
31 | - <StopDate>2019-01-21T14:27:05Z</StopDate> | |
31 | + <StopDate>2019-03-08T13:23:36Z</StopDate> | |
32 | 32 | </TimeSpan> |
33 | - <Cadence>PT96.27S</Cadence> | |
33 | + <Cadence_Min>PT96.27S</Cadence_Min> | |
34 | + <Cadence_Max>PT385.09S</Cadence_Max> | |
34 | 35 | </TemporalDescription> |
35 | 36 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
36 | 37 | <Parameter> |
... | ... |
NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2i.xml
... | ... | @@ -5,7 +5,7 @@ |
5 | 5 | <ResourceID>spase://CDPP/NumericalData/AMDA/THEMIS/E/ESA/the-esa-l2i</ResourceID> |
6 | 6 | <ResourceHeader> |
7 | 7 | <ResourceName>ion full mode</ResourceName> |
8 | - <ReleaseDate>2017-03-13T15:42:30</ReleaseDate> | |
8 | + <ReleaseDate>2019-03-10T21:09:42Z</ReleaseDate> | |
9 | 9 | <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> |
10 | 10 | <Contact> |
11 | 11 | <PersonID>spase://SMWG/Person/Charles.W.Carlson</PersonID> |
... | ... | @@ -32,9 +32,10 @@ |
32 | 32 | <TemporalDescription> |
33 | 33 | <TimeSpan> |
34 | 34 | <StartDate>2007-03-07T19:54:48Z</StartDate> |
35 | - <StopDate>2019-01-21T14:26:19Z</StopDate> | |
35 | + <StopDate>2019-03-08T13:22:55Z</StopDate> | |
36 | 36 | </TimeSpan> |
37 | - <Cadence>PT96.27S</Cadence> | |
37 | + <Cadence_Min>PT96.27S</Cadence_Min> | |
38 | + <Cadence_Max>PT385.09S</Cadence_Max> | |
38 | 39 | </TemporalDescription> |
39 | 40 | <ObservedRegion>Earth.Magnetosphere</ObservedRegion> |
40 | 41 | <Parameter> |
... | ... |