Commit a65c22ae41ddfafbc614810356bab717cb0234a1
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Fix help for M-Shell datasets
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Instrument/CDPP-AMDA/Juice/Models.xml
... | ... | @@ -4,7 +4,7 @@ |
4 | 4 | <Instrument> |
5 | 5 | <ResourceID>spase://CNES/Instrument/CDPP-AMDA/Juice/Models</ResourceID> |
6 | 6 | <ResourceHeader> |
7 | - <ResourceName>Analytical Models</ResourceName> | |
7 | + <ResourceName>Jovian Magnetic Field Models</ResourceName> | |
8 | 8 | <AlternateName>Juice : Jupiter magnetic field model</AlternateName> |
9 | 9 | <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate> |
10 | 10 | <Description>A spherical harmonic model of the magnetic field of Jupiter is obtained from vector magnetic |
... | ... |
Instrument/CDPP-AMDA/Juno/Models.xml
... | ... | @@ -4,7 +4,7 @@ |
4 | 4 | <Instrument> |
5 | 5 | <ResourceID>spase://CNES/Instrument/CDPP-AMDA/Juno/Models</ResourceID> |
6 | 6 | <ResourceHeader> |
7 | - <ResourceName>Analytical Models</ResourceName> | |
7 | + <ResourceName>Jovian Magnetic Field Models</ResourceName> | |
8 | 8 | <AlternateName>Juno : Jupiter magnetic field model</AlternateName> |
9 | 9 | <ReleaseDate>2017-02-04T15:37:46Z</ReleaseDate> |
10 | 10 | <Description>A spherical harmonic model of the magnetic field of Jupiter is obtained from vector magnetic |
... | ... |
NumericalData/CDPP-AMDA/Galileo/Models/gll-mod-khurana.xml
... | ... | @@ -13,7 +13,7 @@ |
13 | 13 | <Role>PrincipalInvestigator</Role> |
14 | 14 | </Contact> |
15 | 15 | <InformationURL> |
16 | - <Name>Access to Khurana model</Name> | |
16 | + <Name>Access to Khurana model from LASP MOP website</Name> | |
17 | 17 | <URL>http://lasp.colorado.edu/home/mop/resources/graphics/code/</URL> |
18 | 18 | </InformationURL> |
19 | 19 | </ResourceHeader> |
... | ... |
NumericalData/CDPP-AMDA/Galileo/Models/gll-mod-mshell.xml
... | ... | @@ -7,8 +7,8 @@ |
7 | 7 | <ResourceName>JRM33 + Con2020 M-Shell</ResourceName> |
8 | 8 | <AlternateName>JRM33 + Con2020 M-Shell</AlternateName> |
9 | 9 | <ReleaseDate>2024-02-15T01:01:36Z</ReleaseDate> |
10 | - <Description>Galileo M-Shell calculated with JRM33+CON2020 between 1995-12-01 and 2003-09-21. | |
11 | - Spatial resolution is 1/250Rj ~ 300 km. Outer boundary is set to R = 40 Rj. | |
10 | + <Description>Galileo M-Shell calculated with JRM33+CON2020 between 1995-12-01 and 2003-09-21. | |
11 | + Spatial resolution is 1/250Rj ~ 300 km. Outer boundary is set to R = 40 Rj. | |
12 | 12 | </Description> |
13 | 13 | <Contact> |
14 | 14 | <PersonID>spase://CNES/Person/CDPP-AMDA/Jonas.Rabia</PersonID> |
... | ... | @@ -54,36 +54,37 @@ |
54 | 54 | <Cadence>PT15M</Cadence> |
55 | 55 | </TemporalDescription> |
56 | 56 | <ObservedRegion>Jupiter</ObservedRegion> |
57 | + <Caveats>Due to the limitation in the spatial resolution used for the computation, small stalls in M-Shell colatitude, longitude and curvilinear distance may occasionally occur close to the magnetic equator</Caveats> | |
57 | 58 | <Parameter> |
58 | 59 | <Name>M-Shell</Name> |
59 | 60 | <ParameterKey>mshell_gll_m</ParameterKey> |
60 | - <Description>M-Shell - Radial distance intersection field line/magnetic equator</Description> | |
61 | + <Description>M-Shell - Radial distance of the intersection between the magnetic field line and themagnetic equator</Description> | |
61 | 62 | <Support> |
62 | 63 | <SupportQuantity>Other</SupportQuantity> |
63 | 64 | </Support> |
64 | 65 | </Parameter> |
65 | 66 | <Parameter> |
66 | - <Name>colatitude</Name> | |
67 | + <Name>M-Shell colatitude</Name> | |
67 | 68 | <ParameterKey>mshell_gll_t</ParameterKey> |
68 | - <Description>Colatitude intersection field line/magnetic equator</Description> | |
69 | + <Description>Colatitude (S3RH) of the intersection between the magnetic field line and themagnetic equator</Description> | |
69 | 70 | <Units>deg</Units> |
70 | 71 | <Support> |
71 | 72 | <SupportQuantity>Positional</SupportQuantity> |
72 | 73 | </Support> |
73 | 74 | </Parameter> |
74 | 75 | <Parameter> |
75 | - <Name>longitude</Name> | |
76 | + <Name>M-Shell longitude</Name> | |
76 | 77 | <ParameterKey>mshell_gll_p</ParameterKey> |
77 | - <Description>Colatitude intersection field line/magnetic equator</Description> | |
78 | + <Description>Longitude (S3RH) of the intersection between the magnetic field line and themagnetic equator</Description> | |
78 | 79 | <Units>deg</Units> |
79 | 80 | <Support> |
80 | 81 | <SupportQuantity>Positional</SupportQuantity> |
81 | 82 | </Support> |
82 | 83 | </Parameter> |
83 | 84 | <Parameter> |
84 | - <Name>distance</Name> | |
85 | + <Name>curvilinear distance s</Name> | |
85 | 86 | <ParameterKey>mshell_gll_s</ParameterKey> |
86 | - <Description>Distance along the field line between SC/magnetic equator</Description> | |
87 | + <Description>Curvilinear distance along the magnetic field line between the magnetic equator and the spacecraft</Description> | |
87 | 88 | <Units>Rj</Units> |
88 | 89 | <Support> |
89 | 90 | <SupportQuantity>Positional</SupportQuantity> |
... | ... |
NumericalData/CDPP-AMDA/Galileo/Models/gll-mod-onera.xml
... | ... | @@ -8,7 +8,8 @@ |
8 | 8 | <ReleaseDate>2012-07-24T07:05:02Z</ReleaseDate> |
9 | 9 | <Description>Data provided to CDPP from ONERA. |
10 | 10 | Magnetic parameters linked to the position of the spaceraft (L, B, Beq,...) have been calculated with a |
11 | - library developed at ONERA and using Khurana magnetic field model.</Description> | |
11 | + library developed at ONERA and using Khurana magnetic field model (K. Khurana and H.K. Schwarzl, Global structure of Jupiterโs magnetospheric current sheet, | |
12 | + Journal of Geophysical Research, vol. 110, A07227, doi: 10.1029/2004JA010757, 2005).</Description> | |
12 | 13 | <Contact> |
13 | 14 | <PersonID>spase://CNES/Person/CDPP-AMDA/A.Sicard</PersonID> |
14 | 15 | <Role>DataProducer</Role> |
... | ... | @@ -17,6 +18,10 @@ |
17 | 18 | <Name>ONERA report : Jupiter data base for AMDA</Name> |
18 | 19 | <URL>http://amda.irap.omp.eu/help/parameters/doc/ONERA_Jupiter_plasma_db_for_AMDA.pdf</URL> |
19 | 20 | </InformationURL> |
21 | + <InformationURL> | |
22 | + <Name>K. Khurana and H.K. Schwarzl, Global structure of Jupiterโs magnetospheric current sheet, Journal of Geophysical Research, vol. 110, A07227</Name> | |
23 | + <URL>https://doi.org/10.1029/2004JA010757</URL> | |
24 | + </InformationURL> | |
20 | 25 | </ResourceHeader> |
21 | 26 | <AccessInformation> |
22 | 27 | <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID> |
... | ... | @@ -62,7 +67,7 @@ |
62 | 67 | * B_Eq (magnitude of B equatorial) |
63 | 68 | * L (McIlwain parameter) |
64 | 69 | * L* (another way to compute L) |
65 | - * I | |
70 | + * I (first magnetic invariant) | |
66 | 71 | * MLT (Magnetic Local Time) |
67 | 72 | * Alpha (local pitch angle) |
68 | 73 | * Alpha_Eq (equatorial pitch angle) |
... | ... |
NumericalData/CDPP-AMDA/Juice/Models/juice51-jrm33-mshell.xml
... | ... | @@ -59,36 +59,37 @@ |
59 | 59 | <Cadence>PT5M</Cadence> |
60 | 60 | </TemporalDescription> |
61 | 61 | <ObservedRegion>Jupiter</ObservedRegion> |
62 | + <Caveats>Due to the limitation in the spatial resolution used for the computation, small stalls in M-Shell colatitude, longitude and curvilinear distance may occasionally occur close to the magnetic equator</Caveats> | |
62 | 63 | <Parameter> |
63 | 64 | <Name>M-Shell</Name> |
64 | 65 | <ParameterKey>mshell_juice51_m</ParameterKey> |
65 | - <Description>M-Shell - Radial distance intersection field line/magnetic equator</Description> | |
66 | + <Description>M-Shell - Radial distance of the intersection between the magnetic field line and themagnetic equator</Description> | |
66 | 67 | <Support> |
67 | 68 | <SupportQuantity>Other</SupportQuantity> |
68 | 69 | </Support> |
69 | 70 | </Parameter> |
70 | 71 | <Parameter> |
71 | - <Name>colatitude</Name> | |
72 | + <Name>M-Shell colatitude</Name> | |
72 | 73 | <ParameterKey>mshell_juice51_t</ParameterKey> |
73 | - <Description>Colatitude intersection field line/magnetic equator</Description> | |
74 | + <Description>Colatitude (S3RH) of the intersection between the magnetic field line and themagnetic equator</Description> | |
74 | 75 | <Units>deg</Units> |
75 | 76 | <Support> |
76 | 77 | <SupportQuantity>Positional</SupportQuantity> |
77 | 78 | </Support> |
78 | 79 | </Parameter> |
79 | 80 | <Parameter> |
80 | - <Name>longitude</Name> | |
81 | + <Name>M-Shell longitude</Name> | |
81 | 82 | <ParameterKey>mshell_juice51_p</ParameterKey> |
82 | - <Description>Colatitude intersection field line/magnetic equator</Description> | |
83 | + <Description>Longitude (S3RH) of the intersection between the magnetic field line and themagnetic equator</Description> | |
83 | 84 | <Units>deg</Units> |
84 | 85 | <Support> |
85 | 86 | <SupportQuantity>Positional</SupportQuantity> |
86 | 87 | </Support> |
87 | 88 | </Parameter> |
88 | 89 | <Parameter> |
89 | - <Name>distance</Name> | |
90 | + <Name>curvilinear distance s</Name> | |
90 | 91 | <ParameterKey>mshell_juice51_s</ParameterKey> |
91 | - <Description>Distance along the field line between SC/magnetic equator</Description> | |
92 | + <Description>Curvilinear distance along the magnetic field line between the magnetic equator and the spacecraft</Description> | |
92 | 93 | <Units>Rj</Units> |
93 | 94 | <Support> |
94 | 95 | <SupportQuantity>Positional</SupportQuantity> |
... | ... |
NumericalData/CDPP-AMDA/Juno/Models/jun-jrm33-mshell.xml
... | ... | @@ -54,44 +54,37 @@ |
54 | 54 | <Cadence>PT1S</Cadence> |
55 | 55 | </TemporalDescription> |
56 | 56 | <ObservedRegion>Jupiter</ObservedRegion> |
57 | - <Parameter> | |
58 | - <Name>orbit number</Name> | |
59 | - <ParameterKey>mshell_juno_orb</ParameterKey> | |
60 | - <Description>Orbit number</Description> | |
61 | - <Support> | |
62 | - <SupportQuantity>Other</SupportQuantity> | |
63 | - </Support> | |
64 | - </Parameter> | |
57 | + <Caveats>Due to the limitation in the spatial resolution used for the computation, small stalls in M-Shell colatitude, longitude and curvilinear distance may occasionally occur close to the magnetic equator</Caveats> | |
65 | 58 | <Parameter> |
66 | 59 | <Name>M-Shell</Name> |
67 | 60 | <ParameterKey>mshell_juno_m</ParameterKey> |
68 | - <Description>M-Shell - Radial distance intersection field line/magnetic equator</Description> | |
61 | + <Description>M-Shell - Radial distance of the intersection between the magnetic field line and themagnetic equator</Description> | |
69 | 62 | <Support> |
70 | 63 | <SupportQuantity>Other</SupportQuantity> |
71 | 64 | </Support> |
72 | 65 | </Parameter> |
73 | 66 | <Parameter> |
74 | - <Name>colatitude</Name> | |
67 | + <Name>M-Shell colatitude</Name> | |
75 | 68 | <ParameterKey>mshell_juno_t</ParameterKey> |
76 | - <Description>Colatitude intersection field line/magnetic equator</Description> | |
69 | + <Description>Colatitude (S3RH) of the intersection between the magnetic field line and themagnetic equator</Description> | |
77 | 70 | <Units>deg</Units> |
78 | 71 | <Support> |
79 | 72 | <SupportQuantity>Positional</SupportQuantity> |
80 | 73 | </Support> |
81 | 74 | </Parameter> |
82 | 75 | <Parameter> |
83 | - <Name>longitude</Name> | |
76 | + <Name>M-Shell longitude</Name> | |
84 | 77 | <ParameterKey>mshell_juno_p</ParameterKey> |
85 | - <Description>Colatitude intersection field line/magnetic equator</Description> | |
78 | + <Description>Longitude (S3RH) of the intersection between the magnetic field line and themagnetic equator</Description> | |
86 | 79 | <Units>deg</Units> |
87 | 80 | <Support> |
88 | 81 | <SupportQuantity>Positional</SupportQuantity> |
89 | 82 | </Support> |
90 | 83 | </Parameter> |
91 | 84 | <Parameter> |
92 | - <Name>distance</Name> | |
85 | + <Name>curvilinear distance s</Name> | |
93 | 86 | <ParameterKey>mshell_juno_s</ParameterKey> |
94 | - <Description>Distance along the field line between SC/magnetic equator</Description> | |
87 | + <Description>Curvilinear distance along the magnetic field line between the magnetic equator and the spacecraft</Description> | |
95 | 88 | <Units>Rj</Units> |
96 | 89 | <Support> |
97 | 90 | <SupportQuantity>Positional</SupportQuantity> |
... | ... |