solo-sisa-slow.xml
10.4 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
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
241
242
243
244
245
246
247
248
249
250
251
252
253
254
255
256
257
258
259
260
261
262
263
264
265
266
267
268
269
<?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-2.4.1.xsd">
<Version>2.4.1</Version>
<NumericalData>
<ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/solo-sisa-slow</ResourceID>
<ResourceHeader>
<ResourceName>slow mode</ResourceName>
<AlternateName>SIS-A ion anti-sunward flux </AlternateName>
<ReleaseDate>2024-05-20T02:47:15Z</ReleaseDate>
<Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, Suprathermal Ion Spectrograph, Rates.
SIS relies in the time-of-flight technique for identifying ions, providing particle counts for several ion
species in the energy range between 14 keV/n and 20 MeV/n. It consists of 2 telescopes: SIS-A
looking in the sunward direction, along the mean Parker spiral and SIS-B looking anti-sunward. The
main scientific measurements that SIS provides are:
* Particle rates. Count rates of 12 ion species (H, He3, He4, C, N, O, Ne, Mg, Si, S, Ca and Fe) in 21 energy channels.
* Helium histogram. Helium events is collected in a mass histogram for better separation of He3 and He4 intensities.
* PHA data with information about individual events.
</Description>
<Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement>
<Contact>
<PersonID>spase://CNES/Person/CDPP-AMDA/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>
</InformationURL>
<Association>
<AssociationID>solo-epd-sisa</AssociationID>
<AssociationType>PartOf</AssociationType>
<Note>L2 : sis-a ; anti-sunward flow</Note>
</Association>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Open</AccessRights>
<AccessURL>
<Name>CDPP/AMDA HAPI Server</Name>
<URL>https://amda.irap.omp.eu/service/hapi</URL>
<Style>HAPI</Style>
<ProductKey>solo-sisa-slow</ProductKey>
<Description>Web Service to this product using the HAPI interface.</Description>
</AccessURL>
<Format>CSV</Format>
<Acknowledgement>Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.</Acknowledgement>
</AccessInformation>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Open</AccessRights>
<AccessURL>
<Name>CDPP/AMDA Web application</Name>
<URL>https://amda.cdpp.eu</URL>
<Description>Access to Data via CDPP/AMDA Web application.</Description>
</AccessURL>
<Format>CSV</Format>
<Format>VOTable</Format>
<Format>CDF</Format>
<Format>PNG</Format>
<Acknowledgement>Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.</Acknowledgement>
</AccessInformation>
<ProviderName>http://soar.esac.esa.int/soar</ProviderName>
<ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-SIS</InstrumentID>
<MeasurementType>EnergeticParticles</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2020-04-02T10:52:18Z</StartDate>
<StopDate>2024-02-29T23:50:37Z</StopDate>
</TimeSpan>
<Cadence>PT30M</Cadence>
</TemporalDescription>
<ObservedRegion>Heliosphere.Inner</ObservedRegion>
<ObservedRegion>Sun.Corona</ObservedRegion>
<Parameter>
<Name>h flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_hflux</ParameterKey>
<Description>Hydrogen flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>11</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>he3 flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_he3flux</ParameterKey>
<Description>Helium-3 flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>12</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>he4 flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_he4flux</ParameterKey>
<Description>Heliun-4 flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>13</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>c flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_cflux</ParameterKey>
<Description>Carbon flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>n flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_nflux</ParameterKey>
<Description>Nitrogen flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>o flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_oflux</ParameterKey>
<Description>Oxygen flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>ne flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_neflux</ParameterKey>
<Description>Neon flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>mg flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_mgflux</ParameterKey>
<Description>Magnesium flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>si flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_siflux</ParameterKey>
<Description>Silicium flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>17</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>s flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_sflux</ParameterKey>
<Description>Sulfur flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>17</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>ca flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_caflux</ParameterKey>
<Description>Calcium flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>16</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>fe flux: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_feflux</ParameterKey>
<Description>Ferrum flux</Description>
<Units>1/(s cm^2 sr MeV/n)</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>15</Size>
</Structure>
<Particle>
<ParticleQuantity>EnergyFlux</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>quality flag: anti-sunward</Name>
<ParameterKey>solo_sisa_slow_qf</ParameterKey>
<Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Support>
<SupportQuantity>DataQuality</SupportQuantity>
</Support>
</Parameter>
</NumericalData>
</Spase>