Blame view

NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp.xml 5.47 KB
1bcff323   Elena.Budnik   NumericalData
1
2
3
4
<?xml version="1.0" encoding="UTF-8"?>
<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://cdpp1.cesr.fr/AMDA-NG/public/schemas/spase-amda-1_2_0.xsd">
    <Version>2.2.6</Version>
    <NumericalData>
1d33d1a0   Elena.Budnik   work
5
        <ResourceID>spase://CDPP/NumericalData/AMDA/Cluster/Cluster4/RAPID/clust4-rap-psp</ResourceID>
1bcff323   Elena.Budnik   NumericalData
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
        <ResourceHeader>
            <ResourceName>Cluster II Tango Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ResourceName>
            <AlternateName>Cluster 4 Prime Parameter RAPID Data</AlternateName>
            <ReleaseDate>2015-10-16T16:51:46Z</ReleaseDate>
            <Description>The dual-sensor spectrometer RAPID (Research with Adaptive Particle Imaging 
                Detectors) analyzes suprathermal plasma distributions in the energy range from 20-400 KeV 
                for electrons and from 2 KeV/nucleon to 1.50 MeV/nucleon for ions. 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 RAPID:
                The Imaging Energetic Particle Spectrometer on Cluster, by B. Wilken et al., from which 
                this information was obtained.</Description>
            <Acknowledgement>NASA, Dr. Berend Wilken, European Space Agency</Acknowledgement>
            <Contact>
                <PersonID>spase://SMWG/Person/Elena.Budnik</PersonID>
                <Role>TechnicalContact</Role>
            </Contact>            
            <InformationURL>
                <Name>NSSDC Master Catalog listing for Cluster II Tango Research with Adaptive Particle Imaging Detectors (RAPID)</Name>
                <URL>http://nssdc.gsfc.nasa.gov/nmc/experimentDisplay.do?id=2000-045A-06</URL>
                <Description>This site provides information concerning the Cluster II Tango Research with Adaptive Particle Imaging Detectors Instrument.</Description>
            </InformationURL>
            <Association>
                <AssociationID>spase://SMWG/Observatory/Cluster-Tango</AssociationID>
                <AssociationType>ObservedBy</AssociationType>
            </Association>
         </ResourceHeader>
        <AccessInformation>
            <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
            <Availability>Online</Availability>
            <AccessRights>Open</AccessRights>
            <AccessURL>
                <Name>AMDA at CDPP</Name>
                <URL>http://amda.cdpp.eu</URL>                
            </AccessURL>
            <Format>NetCDF</Format>
            <Acknowledgement>NASA, Dr. Berend Wilken</Acknowledgement>
        </AccessInformation>
        <ProviderName>CSA</ProviderName>
        <ProcessingLevel>Calibrated</ProcessingLevel>
        <ProviderResourceName>Cluster II Tango Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data</ProviderResourceName>
        <ProviderProcessingLevel>Calibrated</ProviderProcessingLevel>
        <InstrumentID>spase://CDPP/Instrument/AMDA/Cluster-Tango/RAPID</InstrumentID>
        <MeasurementType>EnergeticParticles</MeasurementType>
        <TemporalDescription>
            <TimeSpan>
447d3a6e   Elena.Budnik   work
51
52
                <StartDate>2001-01-01T00:00:03Z</StartDate>
                <StopDate>2006-12-31T23:59:58Z</StopDate>                
1bcff323   Elena.Budnik   NumericalData
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
            </TimeSpan>
            <Cadence>PT4S</Cadence>
        </TemporalDescription>
        <ObservedRegion>Earth.Magnetosheath</ObservedRegion>
        <ObservedRegion>Earth.Magnetosphere</ObservedRegion>
        <ObservedRegion>Earth.Magnetosphere.Magnetotail</ObservedRegion>
        <ObservedRegion>Earth.Magnetosphere.Main</ObservedRegion>
        <ObservedRegion>Earth.Magnetosphere.Polar</ObservedRegion>
        <ObservedRegion>Earth.Magnetosphere.RadiationBelt</ObservedRegion>
        <ObservedRegion>Earth.NearSurface.AuroralRegion</ObservedRegion>
        <ObservedRegion>Earth.NearSurface.Ionosphere</ObservedRegion>
        <ObservedRegion>Earth.NearSurface.Plasmasphere</ObservedRegion>
        <ObservedRegion>Earth.NearSurface.PolarCap</ObservedRegion>
        <ObservedRegion>Heliosphere.NearEarth</ObservedRegion>
        <Keyword>4 second</Keyword>
        <Keyword>magnetosphere</Keyword>
        <Keyword>auroral region</Keyword>
        <Keyword>polar cap</Keyword>
        <Keyword>cusp</Keyword>
        <Keyword>bow shock</Keyword>
        <Keyword>solar wind</Keyword>
        <Keyword>magnetosheath</Keyword>
        <Keyword>Cluster</Keyword>
        <Keyword>magnetotail</Keyword>
        <Keyword>lobe</Keyword>
        <Parameter>
            <Name>Proton Flux </Name>
            <ParameterKey>c4_rap_p</ParameterKey>
            <Description>Cluster II Tango Prime Parameter Research with Adaptive Particle Imaging Detectors electron flux at spin time resolution</Description>
            <Ucd>phys.flux.density;phys.count;phys.atmol.ionStage</Ucd>
            <Cadence>PT4S</Cadence>
            <Units>1/cm^2_sr_s_keV</Units>
            <RenderingHints>
                <DisplayType>Spectrogram</DisplayType>
            </RenderingHints>
            <FillValue>-1.0000e+31</FillValue>
            <Particle>
                <ParticleType>Proton</ParticleType>
                <Qualifier>Scalar</Qualifier>
                <ParticleQuantity>EnergyFlux</ParticleQuantity>
            </Particle>
        </Parameter>
     </NumericalData>
</Spase>