Commit c033aedb82529fe5d765c544cd48fa7015ef68d4
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so het 3
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NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-anti.3.xml
0 → 100644
... | ... | @@ -0,0 +1,106 @@ |
1 | +<?xml version="1.0" encoding="UTF-8"?> | |
2 | +<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"> | |
3 | + <Version>2.3.0</Version> | |
4 | + <NumericalData> | |
5 | + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-anti.3</ResourceID> | |
6 | + <ResourceHeader> | |
7 | + <ResourceName>sunward flow</ResourceName> | |
8 | + <AlternateName>Fe Flux From Antisun Direction ( mean Parker spiral )</AlternateName> | |
9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates. | |
11 | + | |
12 | +HET measures the upper part of the energetic particle spectrum. It is equipped with several solid | |
13 | +state detectors and a BGO crystal to provide identification of particle species from the relative energy | |
14 | +deposited in the different detectors. Thus, HET measures count rates for different ion species, as | |
15 | +well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun, | |
16 | +Anti-Sun, North and South) | |
17 | + | |
18 | +Parameter ID uses Detector looking directon. | |
19 | + </Description> | |
20 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
21 | + <Contact> | |
22 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
23 | + <Role>PrincipalInvestigator</Role> | |
24 | + </Contact> | |
25 | + <InformationURL> | |
26 | + <Name>SolO Archive Support Data</Name> | |
27 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
28 | + <Description></Description> | |
29 | + </InformationURL> | |
30 | + <Association> | |
31 | + <AssociationID>solo-epd-het.3</AssociationID> | |
32 | + <AssociationType>PartOf</AssociationType> | |
33 | + <Note>L2 : fe flux</Note> | |
34 | + </Association> | |
35 | + </ResourceHeader> | |
36 | + <AccessInformation> | |
37 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
38 | + <Availability>Online</Availability> | |
39 | + <AccessRights>Open</AccessRights> | |
40 | + <AccessURL> | |
41 | + <Name>AMDA at CDPP</Name> | |
42 | + <URL>http://amda.cdpp.eu</URL> | |
43 | + </AccessURL> | |
44 | + <Format>Text</Format> | |
45 | + <Acknowledgement> | |
46 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
47 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
48 | + Universite Paul Sabatier, Toulouse | |
49 | + </Acknowledgement> | |
50 | + </AccessInformation> | |
51 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
52 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
53 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
54 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID> | |
55 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
56 | + <TemporalDescription> | |
57 | + <TimeSpan> | |
58 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
59 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
60 | + </TimeSpan> | |
61 | + <CadenceMin>PT5M</CadenceMin> | |
62 | + <CadenceMax>PT10M</CadenceMax> | |
63 | + </TemporalDescription> | |
64 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
65 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
66 | + <Parameter> | |
67 | + <Name>fe flux: sunward</Name> | |
68 | + <ParameterKey>solo_het_asun_feflux</ParameterKey> | |
69 | + <Description>Ferrum flux</Description> | |
70 | + <Ucd/> | |
71 | + <Units>1/(s cm^2 sr MeV/n)</Units> | |
72 | + <UnitsConversion/> | |
73 | + <RenderingHints> | |
74 | + <DisplayType>Spectrogram</DisplayType> | |
75 | + </RenderingHints> | |
76 | + <Structure> | |
77 | + <Size>16</Size> | |
78 | + </Structure> | |
79 | + </Parameter> | |
80 | + <Parameter> | |
81 | + <Name>fe flux unc: sunward</Name> | |
82 | + <ParameterKey>solo_het_asun_feunc</ParameterKey> | |
83 | + <Description>Ferrum flux uncertainty</Description> | |
84 | + <Ucd/> | |
85 | + <Units>1/(s cm^2 sr MeV/n)</Units> | |
86 | + <UnitsConversion/> | |
87 | + <RenderingHints> | |
88 | + <DisplayType>Spectrogram</DisplayType> | |
89 | + </RenderingHints> | |
90 | + <Structure> | |
91 | + <Size>16</Size> | |
92 | + </Structure> | |
93 | + </Parameter> | |
94 | + <Parameter> | |
95 | + <Name>quality flag: sunward</Name> | |
96 | + <ParameterKey>solo_het_asun_3_qf</ParameterKey> | |
97 | + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description> | |
98 | + <Ucd/> | |
99 | + <Units/> | |
100 | + <UnitsConversion/> | |
101 | + <RenderingHints> | |
102 | + <DisplayType>TimeSeries</DisplayType> | |
103 | + </RenderingHints> | |
104 | + </Parameter> | |
105 | +</NumericalData> | |
106 | +</Spase> | |
... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-north.3.xml
0 → 100644
... | ... | @@ -0,0 +1,106 @@ |
1 | +<?xml version="1.0" encoding="UTF-8"?> | |
2 | +<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"> | |
3 | + <Version>2.3.0</Version> | |
4 | + <NumericalData> | |
5 | + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-north.3</ResourceID> | |
6 | + <ResourceHeader> | |
7 | + <ResourceName>southward flow</ResourceName> | |
8 | + <AlternateName>Fe Flux From North Hemisphere Direction</AlternateName> | |
9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates. | |
11 | + | |
12 | +HET measures the upper part of the energetic particle spectrum. It is equipped with several solid | |
13 | +state detectors and a BGO crystal to provide identification of particle species from the relative energy | |
14 | +deposited in the different detectors. Thus, HET measures count rates for different ion species, as | |
15 | +well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun, | |
16 | +Anti-Sun, North and South) | |
17 | + | |
18 | +Parameter ID uses Detector looking directon. | |
19 | + </Description> | |
20 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
21 | + <Contact> | |
22 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
23 | + <Role>PrincipalInvestigator</Role> | |
24 | + </Contact> | |
25 | + <InformationURL> | |
26 | + <Name>SolO Archive Support Data</Name> | |
27 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
28 | + <Description></Description> | |
29 | + </InformationURL> | |
30 | + <Association> | |
31 | + <AssociationID>solo-epd-het.3</AssociationID> | |
32 | + <AssociationType>PartOf</AssociationType> | |
33 | + <Note>L2 : fe flux</Note> | |
34 | + </Association> | |
35 | + </ResourceHeader> | |
36 | + <AccessInformation> | |
37 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
38 | + <Availability>Online</Availability> | |
39 | + <AccessRights>Open</AccessRights> | |
40 | + <AccessURL> | |
41 | + <Name>AMDA at CDPP</Name> | |
42 | + <URL>http://amda.cdpp.eu</URL> | |
43 | + </AccessURL> | |
44 | + <Format>Text</Format> | |
45 | + <Acknowledgement> | |
46 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
47 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
48 | + Universite Paul Sabatier, Toulouse | |
49 | + </Acknowledgement> | |
50 | + </AccessInformation> | |
51 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
52 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
53 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
54 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID> | |
55 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
56 | + <TemporalDescription> | |
57 | + <TimeSpan> | |
58 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
59 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
60 | + </TimeSpan> | |
61 | + <CadenceMin>PT5M</CadenceMin> | |
62 | + <CadenceMax>PT10M</CadenceMax> | |
63 | + </TemporalDescription> | |
64 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
65 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
66 | + <Parameter> | |
67 | + <Name>fe flux: southward</Name> | |
68 | + <ParameterKey>solo_het_north_feflux</ParameterKey> | |
69 | + <Description>Ferrum flux</Description> | |
70 | + <Ucd/> | |
71 | + <Units>1/(s cm^2 sr MeV/n)</Units> | |
72 | + <UnitsConversion/> | |
73 | + <RenderingHints> | |
74 | + <DisplayType>Spectrogram</DisplayType> | |
75 | + </RenderingHints> | |
76 | + <Structure> | |
77 | + <Size>16</Size> | |
78 | + </Structure> | |
79 | + </Parameter> | |
80 | + <Parameter> | |
81 | + <Name>fe flux unc: southward</Name> | |
82 | + <ParameterKey>solo_het_north_feunc</ParameterKey> | |
83 | + <Description>Ferrum flux uncertainty</Description> | |
84 | + <Ucd/> | |
85 | + <Units>1/(s cm^2 sr MeV/n)</Units> | |
86 | + <UnitsConversion/> | |
87 | + <RenderingHints> | |
88 | + <DisplayType>Spectrogram</DisplayType> | |
89 | + </RenderingHints> | |
90 | + <Structure> | |
91 | + <Size>16</Size> | |
92 | + </Structure> | |
93 | + </Parameter> | |
94 | + <Parameter> | |
95 | + <Name>quality flag: southward</Name> | |
96 | + <ParameterKey>solo_het_north_3_qf</ParameterKey> | |
97 | + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description> | |
98 | + <Ucd/> | |
99 | + <Units/> | |
100 | + <UnitsConversion/> | |
101 | + <RenderingHints> | |
102 | + <DisplayType>TimeSeries</DisplayType> | |
103 | + </RenderingHints> | |
104 | + </Parameter> | |
105 | +</NumericalData> | |
106 | +</Spase> | |
... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-south.3.xml
0 → 100644
... | ... | @@ -0,0 +1,106 @@ |
1 | +<?xml version="1.0" encoding="UTF-8"?> | |
2 | +<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"> | |
3 | + <Version>2.3.0</Version> | |
4 | + <NumericalData> | |
5 | + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-south.3</ResourceID> | |
6 | + <ResourceHeader> | |
7 | + <ResourceName>northward flow</ResourceName> | |
8 | + <AlternateName>Fe Flux From South Hemisphere Direction</AlternateName> | |
9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates. | |
11 | + | |
12 | +HET measures the upper part of the energetic particle spectrum. It is equipped with several solid | |
13 | +state detectors and a BGO crystal to provide identification of particle species from the relative energy | |
14 | +deposited in the different detectors. Thus, HET measures count rates for different ion species, as | |
15 | +well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun, | |
16 | +Anti-Sun, North and South) | |
17 | + | |
18 | +Parameter ID uses Detector looking directon. | |
19 | + </Description> | |
20 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
21 | + <Contact> | |
22 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
23 | + <Role>PrincipalInvestigator</Role> | |
24 | + </Contact> | |
25 | + <InformationURL> | |
26 | + <Name>SolO Archive Support Data</Name> | |
27 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
28 | + <Description></Description> | |
29 | + </InformationURL> | |
30 | + <Association> | |
31 | + <AssociationID>solo-epd-het.3</AssociationID> | |
32 | + <AssociationType>PartOf</AssociationType> | |
33 | + <Note>L2 : fe flux</Note> | |
34 | + </Association> | |
35 | + </ResourceHeader> | |
36 | + <AccessInformation> | |
37 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
38 | + <Availability>Online</Availability> | |
39 | + <AccessRights>Open</AccessRights> | |
40 | + <AccessURL> | |
41 | + <Name>AMDA at CDPP</Name> | |
42 | + <URL>http://amda.cdpp.eu</URL> | |
43 | + </AccessURL> | |
44 | + <Format>Text</Format> | |
45 | + <Acknowledgement> | |
46 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
47 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
48 | + Universite Paul Sabatier, Toulouse | |
49 | + </Acknowledgement> | |
50 | + </AccessInformation> | |
51 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
52 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
53 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
54 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID> | |
55 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
56 | + <TemporalDescription> | |
57 | + <TimeSpan> | |
58 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
59 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
60 | + </TimeSpan> | |
61 | + <CadenceMin>PT5M</CadenceMin> | |
62 | + <CadenceMax>PT10M</CadenceMax> | |
63 | + </TemporalDescription> | |
64 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
65 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
66 | + <Parameter> | |
67 | + <Name>fe flux: northward</Name> | |
68 | + <ParameterKey>solo_het_south_feflux</ParameterKey> | |
69 | + <Description>Ferrum flux</Description> | |
70 | + <Ucd/> | |
71 | + <Units>1/(s cm^2 sr MeV/n)</Units> | |
72 | + <UnitsConversion/> | |
73 | + <RenderingHints> | |
74 | + <DisplayType>Spectrogram</DisplayType> | |
75 | + </RenderingHints> | |
76 | + <Structure> | |
77 | + <Size>16</Size> | |
78 | + </Structure> | |
79 | + </Parameter> | |
80 | + <Parameter> | |
81 | + <Name>fe flux unc: northward</Name> | |
82 | + <ParameterKey>solo_het_south_feunc</ParameterKey> | |
83 | + <Description>Ferrum flux uncertainty</Description> | |
84 | + <Ucd/> | |
85 | + <Units>1/(s cm^2 sr MeV/n)</Units> | |
86 | + <UnitsConversion/> | |
87 | + <RenderingHints> | |
88 | + <DisplayType>Spectrogram</DisplayType> | |
89 | + </RenderingHints> | |
90 | + <Structure> | |
91 | + <Size>16</Size> | |
92 | + </Structure> | |
93 | + </Parameter> | |
94 | + <Parameter> | |
95 | + <Name>quality flag: northward</Name> | |
96 | + <ParameterKey>solo_het_south_3_qf</ParameterKey> | |
97 | + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description> | |
98 | + <Ucd/> | |
99 | + <Units/> | |
100 | + <UnitsConversion/> | |
101 | + <RenderingHints> | |
102 | + <DisplayType>TimeSeries</DisplayType> | |
103 | + </RenderingHints> | |
104 | + </Parameter> | |
105 | +</NumericalData> | |
106 | +</Spase> | |
... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-sun.3.xml
0 → 100644
... | ... | @@ -0,0 +1,106 @@ |
1 | +<?xml version="1.0" encoding="UTF-8"?> | |
2 | +<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"> | |
3 | + <Version>2.3.0</Version> | |
4 | + <NumericalData> | |
5 | + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-sun.3</ResourceID> | |
6 | + <ResourceHeader> | |
7 | + <ResourceName>anti-sunward flow</ResourceName> | |
8 | + <AlternateName>Fe From Sun Direction ( mean Parker spiral )</AlternateName> | |
9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates. | |
11 | + | |
12 | +HET measures the upper part of the energetic particle spectrum. It is equipped with several solid | |
13 | +state detectors and a BGO crystal to provide identification of particle species from the relative energy | |
14 | +deposited in the different detectors. Thus, HET measures count rates for different ion species, as | |
15 | +well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun, | |
16 | +Anti-Sun, North and South) | |
17 | + | |
18 | +Parameter ID uses Detector looking directon. | |
19 | + </Description> | |
20 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
21 | + <Contact> | |
22 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
23 | + <Role>PrincipalInvestigator</Role> | |
24 | + </Contact> | |
25 | + <InformationURL> | |
26 | + <Name>SolO Archive Support Data</Name> | |
27 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
28 | + <Description></Description> | |
29 | + </InformationURL> | |
30 | + <Association> | |
31 | + <AssociationID>solo-epd-het.3</AssociationID> | |
32 | + <AssociationType>PartOf</AssociationType> | |
33 | + <Note>L2 : fe flux</Note> | |
34 | + </Association> | |
35 | + </ResourceHeader> | |
36 | + <AccessInformation> | |
37 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
38 | + <Availability>Online</Availability> | |
39 | + <AccessRights>Open</AccessRights> | |
40 | + <AccessURL> | |
41 | + <Name>AMDA at CDPP</Name> | |
42 | + <URL>http://amda.cdpp.eu</URL> | |
43 | + </AccessURL> | |
44 | + <Format>Text</Format> | |
45 | + <Acknowledgement> | |
46 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
47 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
48 | + Universite Paul Sabatier, Toulouse | |
49 | + </Acknowledgement> | |
50 | + </AccessInformation> | |
51 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
52 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
53 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
54 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID> | |
55 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
56 | + <TemporalDescription> | |
57 | + <TimeSpan> | |
58 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
59 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
60 | + </TimeSpan> | |
61 | + <CadenceMin>PT5M</CadenceMin> | |
62 | + <CadenceMax>PT10M</CadenceMax> | |
63 | + </TemporalDescription> | |
64 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
65 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
66 | + <Parameter> | |
67 | + <Name>fe flux: anti-sunward</Name> | |
68 | + <ParameterKey>solo_het_sun_feflux</ParameterKey> | |
69 | + <Description>Ferrum flux</Description> | |
70 | + <Ucd/> | |
71 | + <Units>1/(s cm^2 sr MeV/n)</Units> | |
72 | + <UnitsConversion/> | |
73 | + <RenderingHints> | |
74 | + <DisplayType>Spectrogram</DisplayType> | |
75 | + </RenderingHints> | |
76 | + <Structure> | |
77 | + <Size>16</Size> | |
78 | + </Structure> | |
79 | + </Parameter> | |
80 | + <Parameter> | |
81 | + <Name>fe flux unc: anti-sunward</Name> | |
82 | + <ParameterKey>solo_het_sun_feunc</ParameterKey> | |
83 | + <Description>Ferrum flux uncertainty</Description> | |
84 | + <Ucd/> | |
85 | + <Units>1/(s cm^2 sr MeV/n)</Units> | |
86 | + <UnitsConversion/> | |
87 | + <RenderingHints> | |
88 | + <DisplayType>Spectrogram</DisplayType> | |
89 | + </RenderingHints> | |
90 | + <Structure> | |
91 | + <Size>16</Size> | |
92 | + </Structure> | |
93 | + </Parameter> | |
94 | + <Parameter> | |
95 | + <Name>quality flag: anti-sunward</Name> | |
96 | + <ParameterKey>solo_het_sun_3_qf</ParameterKey> | |
97 | + <Description>0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent</Description> | |
98 | + <Ucd/> | |
99 | + <Units/> | |
100 | + <UnitsConversion/> | |
101 | + <RenderingHints> | |
102 | + <DisplayType>TimeSeries</DisplayType> | |
103 | + </RenderingHints> | |
104 | + </Parameter> | |
105 | +</NumericalData> | |
106 | +</Spase> | |
... | ... |
NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-total.3.xml
0 → 100644
... | ... | @@ -0,0 +1,83 @@ |
1 | +<?xml version="1.0" encoding="UTF-8"?> | |
2 | +<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"> | |
3 | + <Version>2.3.0</Version> | |
4 | + <NumericalData> | |
5 | + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-het-total.3</ResourceID> | |
6 | + <ResourceHeader> | |
7 | + <ResourceName>total flux</ResourceName> | |
8 | + <AlternateName>Fe Total Flux</AlternateName> | |
9 | + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> | |
10 | + <Description>Solar Orbiter, Level 2 Data, Energetic Particle Detector, High Energy Telescope, Rates. | |
11 | + | |
12 | +HET measures the upper part of the energetic particle spectrum. It is equipped with several solid | |
13 | +state detectors and a BGO crystal to provide identification of particle species from the relative energy | |
14 | +deposited in the different detectors. Thus, HET measures count rates for different ion species, as | |
15 | +well as electrons. HET provides measurements in the same 4 fields of view covered by EPT (Sun, | |
16 | +Anti-Sun, North and South) | |
17 | + </Description> | |
18 | + <Acknowledgement>See http://espada.uah.es/epd/EPD_data.php</Acknowledgement> | |
19 | + <Contact> | |
20 | + <PersonID>spase://CDPP/Person/J.Rodrigues-Pacheco</PersonID> | |
21 | + <Role>PrincipalInvestigator</Role> | |
22 | + </Contact> | |
23 | + <InformationURL> | |
24 | + <Name>SolO Archive Support Data</Name> | |
25 | + <URL>https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</URL> | |
26 | + <Description></Description> | |
27 | + </InformationURL> | |
28 | + <Association> | |
29 | + <AssociationID>solo-epd-het.3</AssociationID> | |
30 | + <AssociationType>PartOf</AssociationType> | |
31 | + <Note>L2 : fe flux</Note> | |
32 | + </Association> | |
33 | + <PriorID>so-het-sun.3</PriorID> | |
34 | + <PriorID>so-het-anti.3</PriorID> | |
35 | + <PriorID>so-het-north.3</PriorID> | |
36 | + <PriorID>so-het-south.3</PriorID> | |
37 | + </ResourceHeader> | |
38 | + <AccessInformation> | |
39 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
40 | + <Availability>Online</Availability> | |
41 | + <AccessRights>Open</AccessRights> | |
42 | + <AccessURL> | |
43 | + <Name>AMDA at CDPP</Name> | |
44 | + <URL>http://amda.cdpp.eu</URL> | |
45 | + </AccessURL> | |
46 | + <Format>Text</Format> | |
47 | + <Acknowledgement> | |
48 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
49 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
50 | + Universite Paul Sabatier, Toulouse | |
51 | + </Acknowledgement> | |
52 | + </AccessInformation> | |
53 | + <ProviderName>http://soar.esac.esa.int/soar</ProviderName> | |
54 | + <ProviderResourceName>EPD-EPT-SUN-RATES</ProviderResourceName> | |
55 | + <ProviderAcknowlegment></ProviderAcknowlegment> | |
56 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-HET</InstrumentID> | |
57 | + <MeasurementType>EnergeticParticles</MeasurementType> | |
58 | + <TemporalDescription> | |
59 | + <TimeSpan> | |
60 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
61 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
62 | + </TimeSpan> | |
63 | + <CadenceMin>PT5M</CadenceMin> | |
64 | + <CadenceMax>PT10M</CadenceMax> | |
65 | + </TemporalDescription> | |
66 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
67 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
68 | + <Parameter> | |
69 | + <Name>fe flux: total</Name> | |
70 | + <ParameterKey>solo_het_tot_feflux</ParameterKey> | |
71 | + <Description>Ferrum flux</Description> | |
72 | + <Ucd/> | |
73 | + <Units>1/(s cm^2 sr MeV/n)</Units> | |
74 | + <UnitsConversion/> | |
75 | + <RenderingHints> | |
76 | + <DisplayType>Spectrogram</DisplayType> | |
77 | + </RenderingHints> | |
78 | + <Structure> | |
79 | + <Size>16</Size> | |
80 | + </Structure> | |
81 | + </Parameter> | |
82 | +</NumericalData> | |
83 | +</Spase> | |
... | ... |