psp-spi-Hsp.xml
4.41 KB
1
2
3
4
5
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
51
52
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
97
98
99
100
101
102
103
104
105
106
<?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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
<Version>2.3.1</Version>
<NumericalData>
<ResourceID>spase://CNES/NumericalData/CDPP-AMDA/PSP/SPI/psp-spi-Hsp</ResourceID>
<ResourceHeader>
<ResourceName>spectrograms</ResourceName>
<AlternateName>SWEAP SPANAi Level 3 moments</AlternateName>
<ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
<Description>
This data set provides spectra of the energy flux versus Energy, Elevation and Azimuth angle in RTN coordinates.
</Description>
<Acknowledgement>
Please acknowledge the NASA Parker Solar Probe Mission and SWEAP team
led by Justin Kasper for use of data.
</Acknowledgement>
<Contact>
<PersonID>spase://SMWG/Person/Justin.C.Kasper</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<Contact>
<PersonID>spase://SMWG/Person/Davin.Larson</PersonID>
<Role>DeputyPI</Role>
</Contact>
<Association>
<AssociationID>psp-spi-proton</AssociationID>
<AssociationType>PartOf</AssociationType>
<Note>protons</Note>
</Association>
<InformationURL>
<Name>Investigation Publication</Name>
<URL>https://link.springer.com/article/10.1007%2Fs11214-015-0206-3</URL>
<Description>
Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus
</Description>
</InformationURL>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Open</AccessRights>
<AccessURL>
<Name>AMDA at CDPP</Name>
<URL>
http://amda.cdpp.eu
</URL>
</AccessURL>
<Format>Text</Format>
<Acknowledgement>
AMDA is a science analysis system provided by the Centre de Donnees de la
Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and
Universite Paul Sabatier, Toulouse
</Acknowledgement>
</AccessInformation>
<ProviderName>SPDF</ProviderName>
<ProviderResourceName>psp/sweap/spi/l3/spi_sf00_mom_inst/</ProviderResourceName>
<ProviderAcknowlegment>
Please acknowledge the CDAWeb team at GSFC/SPDF.</ProviderAcknowlegment>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/PSP/SPI</InstrumentID>
<MeasurementType>ThermalPlasma</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2018-09-02T00:00:12Z</StartDate>
<StopDate>2025-08-12T23:59:55Z</StopDate>
</TimeSpan>
<CadenceMin>PT0.2S</CadenceMin>
<CadenceMax>PT30S</CadenceMax>
</TemporalDescription>
<ObservedRegion>Heliosphere.Inner</ObservedRegion>
<ObservedRegion>Sun.Corona</ObservedRegion>
<Parameter>
<Name>h+ e_flux/ener</Name>
<ParameterKey>psp_spi_Hee</ParameterKey>
<Description>
Differential Energy Flux vs Energy
</Description>
<Units>eV/cm2-s-ster-eV</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
</Parameter>
<Parameter>
<Name>h+ e_flux/theta</Name>
<ParameterKey>psp_spi_Heth</ParameterKey>
<Description>
Differential Energy Flux vs Elevation RTN
</Description>
<Units>eV/cm2-s-ster-eV</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
</Parameter>
<Parameter>
<Name>h+ e_flux/phi</Name>
<ParameterKey>psp_spi_Heph</ParameterKey>
<Description>
Differential Energy Flux vs Azimuth RTN
</Description>
<Units>eV/cm2-s-ster-eV</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
</Parameter>
</NumericalData>
</Spase>