bepi-mia-mercury1.vm.sw.xml
8.44 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
<?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/BepiColombo/Mio/MIA/bepi-mia-mercury1.vm.sw</ResourceID>
<ResourceHeader>
<ResourceName>L1 - velocity moment SW</ResourceName>
<ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
<Description>The BepiColombo mission conducted the first of its six flybys of Mercury on 1 October 2021 and explored the southern hemisphere of the magnetosphere of Mercury. BepiColombo entered the dusk side magnetosphere from the nightside and exited in the dayside through the dawn side magnetosphere.
L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode).</Description>
<Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
<Contact>
<PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<Contact>
<PersonID>spase://CNES/Person/CDPP-AMDA/Sae.Aizawa</PersonID>
<Role>DataProducer</Role>
</Contact>
<Contact>
<PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
<Role>DataProducer</Role>
</Contact>
<InformationURL>
<Name>Aizawa, S., Harada, Y., André, N., Saito, Y., Barabash, S., Delcourt, D., Sauvaud, J.-A., Barthe, A., Fedorov, A., Penou, E., Yokota, S., Miyake, W., Persson, M., Nenon, Q., Rojo, M., Futaana, Y., Asamura, K., Shimoyama, M., Hadid, L., … Murakami, G. (2023). Direct evidence of substorm-related impulsive injections of electrons at Mercury (version 1) [Data set]. Zenodo.</Name>
<URL>https://doi.org/10.5281/zenodo.7926905</URL>
</InformationURL>
<Association>
<AssociationID>bepi-mia-mercury1</AssociationID>
<AssociationType>PartOf</AssociationType>
<Note>Mercury flyby #1</Note>
</Association>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Restricted</AccessRights>
<AccessURL>
<Name>CDPP/AMDA HAPI Server</Name>
<URL>http://amda.irap.omp.eu/service/hapi</URL>
<Style>HAPI</Style>
<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 http://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>Restricted</AccessRights>
<AccessURL>
<Name>CDPP/AMDA Web application</Name>
<URL>http://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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers.</Acknowledgement>
</AccessInformation>
<ProviderName>JAXA</ProviderName>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA</InstrumentID>
<MeasurementType>ThermalPlasma</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2020-10-15T00:00:00Z</StartDate>
<StopDate>2020-10-15T07:13:20Z</StopDate>
</TimeSpan>
<CadenceMin>PT4S</CadenceMin>
</TemporalDescription>
<ObservedRegion>Mercury</ObservedRegion>
<Parameter>
<Name>n</Name>
<ParameterKey>mia_mercury1_vmsw_n</ParameterKey>
<Description>Uncalibrated density</Description>
<Units>count/cm^3</Units>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<FillValue>-1.0e+31</FillValue>
<Particle>
<ParticleType>Ion</ParticleType>
<ParticleQuantity>NumberDensity</ParticleQuantity>
</Particle>
</Parameter><Parameter>
<Name>v_spc</Name>
<ParameterKey>mia_mercury1_vmsw_v</ParameterKey>
<Description>Uncalibrated velocity in SPC coordinates</Description>
<Units>km/s</Units>
<CoordinateSystem>
<CoordinateRepresentation>Cartesian</CoordinateRepresentation>
<CoordinateSystemName>SC</CoordinateSystemName>
</CoordinateSystem>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Structure>
<Size>3</Size>
<Element>
<Name>vx</Name>
<Qualifier>Component.I</Qualifier>
<Index>1</Index>
<ParameterKey>mia_mercury1_vmsw_v(0)</ParameterKey>
</Element>
<Element>
<Name>vy</Name>
<Qualifier>Component.J</Qualifier>
<Index>2</Index>
<ParameterKey>mia_mercury1_vmsw_v(1)</ParameterKey>
</Element>
<Element>
<Name>vz</Name>
<Qualifier>Component.K</Qualifier>
<Index>3</Index>
<ParameterKey>mia_mercury1_vmsw_v(2)</ParameterKey>
</Element>
</Structure>
<FillValue>-1.0e+31</FillValue>
<Particle>
<ParticleType>Ion</ParticleType>
<Qualifier>Vector</Qualifier>
<ParticleQuantity>Velocity</ParticleQuantity>
</Particle>
</Parameter> <Parameter>
<Name>|v|</Name>
<ParameterKey>mia_mercury1_vmsw_vtot</ParameterKey>
<Description>Uncalibrated velocity magnitude</Description>
<Units>km/s</Units>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Particle>
<ParticleType>Ion</ParticleType>
<Qualifier>Magnitude</Qualifier>
<ParticleQuantity>Velocity</ParticleQuantity>
</Particle>
</Parameter> <Parameter>
<Name>t_spc</Name>
<ParameterKey>mia_mercury1_vmsw_t</ParameterKey>
<Description>Uncalibrated temperature in SPC coordinates</Description>
<Units>eV</Units>
<CoordinateSystem>
<CoordinateRepresentation>Cartesian</CoordinateRepresentation>
<CoordinateSystemName>SC</CoordinateSystemName>
</CoordinateSystem>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Structure>
<Size>6</Size>
<Element>
<Name>Txx</Name>
<Index>1</Index>
<ParameterKey>mia_mercury1_vmsw_t(0)</ParameterKey>
</Element>
<Element>
<Name>Tyy</Name>
<Index>2</Index>
<ParameterKey>mia_mercury1_vmsw_t(1)</ParameterKey>
</Element>
<Element>
<Name>Tzz</Name>
<Index>3</Index>
<ParameterKey>mia_mercury1_vmsw_t(2)</ParameterKey>
</Element>
<Element>
<Name>Txy</Name>
<Index>4</Index>
<ParameterKey>mia_mercury1_vmsw_t(3)</ParameterKey>
</Element>
<Element>
<Name>Tyz</Name>
<Index>5</Index>
<ParameterKey>mia_mercury1_vmsw_t(4)</ParameterKey>
</Element>
<Element>
<Name>Tzx</Name>
<Index>6</Index>
<ParameterKey>mia_mercury1_vmsw_t(5)</ParameterKey>
</Element>
</Structure>
<FillValue>-1.0e+31</FillValue>
<Particle>
<ParticleType>Ion</ParticleType>
<Qualifier>Scalar</Qualifier>
<ParticleQuantity>Temperature</ParticleQuantity>
</Particle>
</Parameter>
</NumericalData>
</Spase>