so-het-sun.1.xml
6.6 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
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
<?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://www.spase-group.org/data/schema/spase-2_3_0.xsd">
<Version>2.3.0</Version>
<NumericalData>
<ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-sun.1</ResourceID>
<ResourceHeader>
<ResourceName>from sun direction</ResourceName>
<AlternateName>Electron HighEnergy ( 38-96 MeV ) / He3 / He4 From Sun Direction ( mean Parker spiral )</AlternateName>
<ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate>
<Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates.
HET measures the upper part of the energetic particle spectrum. It is equipped with several solid
state detectors and a BGO crystal to provide identification of particle species from the relative energy
deposited in the different detectors. Thus, HET measures count rates for different ion species, as
well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun,
Anti-Sun, North and South)
</Description>
<Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
<Contact>
<PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<InformationURL>
<Name>SolO Archive Support Data</Name>
<URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL>
<Description></Description>
</InformationURL>
<Association>
<AssociationID>solo-epd-het.1</AssociationID>
<AssociationType>PartOf</AssociationType>
<Note>L2 : e- 38-96 MeV / he3 / he4 flux</Note>
</Association>
</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>http://soar.esac.esa.int/soar</ProviderName>
<ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName>
<ProviderAcknowlegment></ProviderAcknowlegment>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID>
<MeasurementType>EnergeticParticles</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2018-09-02T00:00:12Z</StartDate>
<StopDate>2025-08-12T23:59:55Z</StopDate>
</TimeSpan>
<CadenceMin>PT5S</CadenceMin>
<CadenceMax>PT30S</CadenceMax>
</TemporalDescription>
<ObservedRegion>Heliosphere.Inner</ObservedRegion>
<ObservedRegion>Sun.Corona</ObservedRegion>
<Parameter>
<Name>e- HE flux: sun</Name>
<ParameterKey>solo_het_sun_eheflux</ParameterKey>
<Description>Electron flux in 38 - 96 MeV energy range</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
</Parameter>
<Parameter>
<Name>e- HE flux unc: sun</Name>
<ParameterKey>solo_het_sun_eheunc</ParameterKey>
<Description>Uncertainty in electron flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
</Parameter>
<Parameter>
<Name>he3 flux: sun</Name>
<ParameterKey>solo_het_sun_he3flux</ParameterKey>
<Description>He3 flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>9</Size>
</Structure>
</Parameter>
<Parameter>
<Name>he3 flux unc: sun</Name>
<ParameterKey>solo_het_sun_he3unc</ParameterKey>
<Description>Uncertainty in He3 flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>9</Size>
</Structure>
</Parameter>
<Parameter>
<Name>he4 flux: sun</Name>
<ParameterKey>solo_het_sun_he4flux</ParameterKey>
<Description>He4 flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>15</Size>
</Structure>
</Parameter>
<Parameter>
<Name>he4 flux unc: sun</Name>
<ParameterKey>solo_het_sun_he4unc</ParameterKey>
<Description>Uncertainty in He4 flux</Description>
<Ucd/>
<Units>1/(s cm^2 sr MeV)</Units>
<UnitsConversion/>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>15</Size>
</Structure>
</Parameter>
<Parameter>
<Name>quality flag: sun</Name>
<ParameterKey>solo_het_sun_1_qf</ParameterKey>
<Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description>
<Ucd/>
<Units/>
<UnitsConversion/>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
</Parameter>
</NumericalData>
</Spase>