CDPP / CNES

Commit 2297f4c67d755c82e2f24d470c204d47c1cbfaf6

Authored by Elena.Budnik
1 parent 7832a2e3
Exists in master and in 12 other branches amdadev, aschulz, autocommit, bepi_master, bepi_update, branch_q, cleanup_registry, cleanup_registry_master, cleanup_registry_merged, juice_jdc, juno_jade, soar

Interball description

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Instrument/AMDA/Interball-1/CORALL.xml
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5 5 <ResourceID>spase://CDPP/Instrument/AMDA/Interball-1/CORALL</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>Corall</ResourceName>
8   - <AlternateName>3D Ion Spectrometer</AlternateName>
  8 + <AlternateName>quasi-3D Ion Spectrometer</AlternateName>
9 9 <ReleaseDate>2010-02-04T12:34:56.789</ReleaseDate>
10   - <Description>CORALL is a hemispherical electrostatic ion energy spectrometer with a fan-shaped field-of-view of 10 x 150 degrees. Satellite rotation with period about 2 minutes enables one to perform quasi-3D measurements of the energy/charge ion distribution function in the range from 30 to 24200 eV/q in 32 steps. The accumulation time on 1 energy step is 1/1024-th of the satellite rotation period, i.e. about 100 msec, and the scan period of 1 energy spectrum (32 steps) is equal to about 4 minutes. Energy resolution is +/- 5%, and the separation of the energy channels is 24%. There are 5 polar channels, at angles of 45, 70, 95, 120, and 145 degrees from the sun. Angular resolution is +/- 25 degrees in the polar angle and +/- 5 degrees in the azimuthal angle.
11   - Instrument CORALL was designed and fabricated jointly by IKI RAN and INTERCOSMOS of the Republic of Cuba.
12   - The instrument began operating August 14, 1995. However, there were problems with the telemetry system BNS which provides satellite rotation pulses. CORALL uses this pulse for performance of measurements in the inertial coordinate system. As of August 31, 1995 the complex BNS + CORALL is operating properly.</Description>
  10 + <Description>Hemispherical electrostatic ion energy spectrometer CORALL has fan-shaped field-of-view of 10 x 150 degrees.
  11 + Satellite rotation with period about 2 min enables one to perform quasi-3D measurements of Energy/Charge ion distribution function in
  12 + the range from 30 to 24200 eV/q with good energy resolution. The accumulation time on 1 energy step is
  13 + 1/1024-th of the satellite rotation period, i.e. about 100 msec, and the scan period of 1 energy spectrum (32 steps)
  14 + is equal to about 4 min.
  15 + </Description>
  16 + <Contact>
  17 + <PersonID>spase://CDPP/Person/Andrey.Fedorov</PersonID>
  18 + <Role>PrincipalInvestigator</Role>
  19 + </Contact>
13 20 <Contact>
14 21 <PersonID>spase://SMWG/Person/Reynal.Jimenez</PersonID>
15 22 <Role>PrincipalInvestigator</Role>
16 23 </Contact>
17 24 <InformationURL>
18   - <Name>NSSDC's Master Catalog</Name>
19   - <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=1995-039A-05</URL>
20   - <Description>Information about the Wide-range 3D Ion Spectrometer (CORALL) experiment on the Interball Tail Probe mission.</Description>
  25 + <Name>Corall Home Page at IKI</Name>
  26 + <URL>http://www.iki.rssi.ru/interball/vdpcrl/corall.html</URL>
  27 + <Description>Information about the Wide-range 3D Ion Spectrometer (CORALL) experiment on the Interball Tail Probe mission</Description>
21 28 </InformationURL>
22 29 </ResourceHeader>
23   - <InstrumentType>EnergeticParticleInstrument</InstrumentType>
  30 + <InstrumentType>ElectrostaticAnalyser</InstrumentType>
24 31 <InvestigationName>Wide-range 3D Ion Spectrometer (CORALL) on Interball Tail Probe</InvestigationName>
25 32 <ObservatoryID>spase://CDPP/Observatory/AMDA/Interball-Tail</ObservatoryID>
26 33 </Instrument>
... ...
Instrument/AMDA/Interball-1/Ephemeris.xml
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12 12 <PersonID>spase://SMWG/Person/Victoria.I.Prokhorenko</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14 14 </Contact>
15   - <Contact>
16   - <PersonID>spase://SMWG/Person/Jan.Merka</PersonID>
17   - <Role>MetadataContact</Role>
18   - </Contact>
19 15 <InformationURL>
20 16 <Name>IKI Satellite Situation Center</Name>
21 17 <URL>http://www.iki.rssi.ru/vprokhor/</URL>
... ...
NumericalData/AMDA/INTERBALL-Tail/CORALL/intt-crl-kp.xml
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8 8 <ReleaseDate>2015-10-16T19:34:56.789</ReleaseDate>
9 9 <Description/>
10 10 <Contact>
11   - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
12   - <Role>TechnicalContact</Role>
  11 + <PersonID>spase://CDPP/Person/Andrey.Fedorov</PersonID>
  12 + <Role>PrincipalInvestigator</Role>
13 13 </Contact>
14 14 </ResourceHeader>
15 15 <AccessInformation>
... ... @@ -33,7 +33,6 @@
33 33 </TimeSpan>
34 34 <Cadence>PT2M</Cadence>
35 35 </TemporalDescription>
36   - <ObservedRegion>Heliosphere.NearEarth</ObservedRegion>
37 36 <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
38 37 <ObservedRegion>Earth.Magnetosphere</ObservedRegion>
39 38 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
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NumericalData/AMDA/INTERBALL-Tail/Ephemeris/intt-orb-all.xml
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11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Victoria.I.Prokhorenko</PersonID>
13 13 <Role>PrincipalInvestigator</Role>
14   - </Contact>
15   - <Contact>
16   - <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
17   - <Role>TechnicalContact</Role>
18   - </Contact>
  14 + </Contact>
19 15 <InformationURL>
20 16 <Name>IKI Satellite Situation Center</Name>
21 17 <URL>http://www.iki.rssi.ru/vprokhor</URL>
... ... @@ -51,7 +47,7 @@
51 47 <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
52 48 <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
53 49 <ObservedRegion>Heliosphere.NearEarth</ObservedRegion>
54   - <Caveats>The data cadence varies.</Caveats>
  50 + <Caveats>The data cadence varies</Caveats>
55 51 <Parameter>
56 52 <Name>xyz_gse</Name>
57 53 <ParameterKey>it_xyz</ParameterKey>
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Observatory/AMDA/Interball-Tail.xml
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6 6 <ResourceHeader>
7 7 <ResourceName>Interball Tail</ResourceName>
8 8 <ReleaseDate>2010-09-27T18:40:58Z</ReleaseDate>
9   - <Description>The Interball Project is a multi-national effort that consists of four spacecraft: two main spacecraft of the Prognoz series, made in Russia, each with a small subsatellite made in Czechoslovakia. The main objective is to study the physical mechanisms responsible for the transmission of solar wind energy to the magnetosphere, its storage there, and subsequent dissipation in the tail and auroral regions of the magnetosphere, ionosphere, and atmosphere during magnetospheric substorms. One pair of spacecraft, Tail Probe and its subsatellite S2-X (X for the first letter of the Russian word for ``Tail''), will be launched into the magnetospheric tail. The second pair, Auroral Probe and S2-A (A for ``Auroral''), will have an orbit that crosses the auroral oval to observe the acceleration of auroral particles and the flow of electric currents that connect the magnetospheric tail with the conducting ionosphere.</Description>
  9 + <Description></Description>
10 10 <Contact>
11   - <PersonID>spase://SMWG/Person/Jan.Merka</PersonID>
12   - <Role>MetadataContact</Role>
  11 + <PersonID>spase://CDPP/Person/Lev.Zeleny</PersonID>
  12 + <Role>PrincipalInvestigator</Role>
13 13 </Contact>
14 14 </ResourceHeader>
15 15 <ObservatoryGroupID>spase://CDPP/Observatory/AMDA/Interball</ObservatoryGroupID>
... ... @@ -20,5 +20,9 @@
20 20 <ObservatoryRegion>Earth.Magnetosphere.Main</ObservatoryRegion>
21 21 <ObservatoryRegion>Earth.Magnetosphere.Polar</ObservatoryRegion>
22 22 </Location>
  23 + <OperatingSpan>
  24 + <StartDate>1995-08-02T23:59:11</StartDate>
  25 + <StopDate>2000-10-16T00:00:00</StopDate>
  26 + </OperatingSpan>
23 27 </Observatory>
24 28 </Spase>
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Observatory/AMDA/Interball.xml
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6 6 <ResourceHeader>
7 7 <ResourceName>Interball</ResourceName>
8 8 <ReleaseDate>2017-09-27T18:40:58Z</ReleaseDate>
9   - <Description>The Interball Project is a multi-national effort that consists of four spacecraft: two main spacecraft of the Prognoz series, made in Russia, each with a small subsatellite made in Czechoslovakia. The main objective is to study the physical mechanisms responsible for the transmission of solar wind energy to the magnetosphere, its storage there, and subsequent dissipation in the tail and auroral regions of the magnetosphere, ionosphere, and atmosphere during magnetospheric substorms. One pair of spacecraft, Tail Probe and its subsatellite S2-X (X for the first letter of the Russian word for ``Tail''), will be launched into the magnetospheric tail. The second pair, Auroral Probe and S2-A (A for ``Auroral''), will have an orbit that crosses the auroral oval to observe the acceleration of auroral particles and the flow of electric currents that connect the magnetospheric tail with the conducting ionosphere.</Description>
  9 + <Description>The Interball Project was a multi-national effort that consists of four spacecraft:
  10 + two main spacecraft of the Prognoz series, made in Russia, each with a small subsatellite made in Czechoslovakia.
  11 + The main objective was to study the physical mechanisms responsible for the transmission of solar wind energy to the magnetosphere,
  12 + its storage there, and subsequent dissipation in the tail and auroral regions of the magnetosphere, ionosphere, and atmosphere during
  13 + magnetospheric substorms. One pair of spacecraft, Tail Probe and its subsatellite S2-X
  14 + (X for the first letter of the Russian word for "Tail"), has been launched into the magnetospheric tail.
  15 + The second pair, Auroral Probe and S2-A (A for "Auroral"), had an orbit that crossed the auroral oval to observe the acceleration of
  16 + auroral particles and the flow of electric currents that connect the magnetospheric tail with the conducting ionosphere.</Description>
10 17 <Contact>
11 18 <PersonID>spase://CDPP/Person/Lev.Zeleny</PersonID>
12 19 <Role>PrincipalInvestigator</Role>
... ... @@ -14,11 +21,13 @@
14 21 </ResourceHeader>
15 22 <Location>
16 23 <ObservatoryRegion>Earth.Magnetosphere</ObservatoryRegion>
17   - <ObservatoryRegion>Heliosphere.NearEarth</ObservatoryRegion>
18 24 <ObservatoryRegion>Earth.Magnetosheath</ObservatoryRegion>
19   - <ObservatoryRegion>Earth.Magnetosphere</ObservatoryRegion>
20 25 <ObservatoryRegion>Earth.Magnetosphere.Main</ObservatoryRegion>
21 26 <ObservatoryRegion>Earth.Magnetosphere.Polar</ObservatoryRegion>
22 27 </Location>
  28 + <OperatingSpan>
  29 + <StartDate>1995-08-02T23:59:11</StartDate>
  30 + <StopDate>2000-10-16T00:00:00</StopDate>
  31 + </OperatingSpan>
23 32 </Observatory>
24 33 </Spase>
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Person/Lev.Zeleny.xml 0 → 100644
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  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_2_0.xsd">
  3 + <Version>2.2.0</Version>
  4 + <Person>
  5 + <ResourceID>spase://CDPP/Person/Lev.Zeleny</ResourceID>
  6 + <PersonName>Prof. Lev Zeleny</PersonName>
  7 + <OrganizationName>IKI RAN, Moscow</OrganizationName>
  8 + <Email>lzeleny@iki.rssi.ru</Email>
  9 + </Person>
  10 +</Spase>
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