Commit fb015f802e4d455e7dd547075e7df7d8635c16b1
1 parent
1e9b966c
Exists in
master
and in
11 other branches
added PSP SPE
Showing
3 changed files
with
135 additions
and
1 deletions
Show diff stats
| ... | ... | @@ -0,0 +1,34 @@ |
| 1 | +<?xml version="1.0" encoding="UTF-8"?> | |
| 2 | +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd"> | |
| 3 | + <Version>2.2.6</Version> | |
| 4 | + <Instrument> | |
| 5 | + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/PSP/SPE</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>SWEAP SPANe</ResourceName> | |
| 8 | + <AlternateName>Solar Probe Analyser (SPAN) electrons</AlternateName> | |
| 9 | + <ReleaseDate>2019-11-12T16:00:05Z</ReleaseDate> | |
| 10 | + <Description>The SPAN-A module has two ESAs to measure ions and electrons from the ram direction and nadir. SPAN-B consists of a single ESA to measure electrons from the anti-ram direction. SPAN-A is located on the ram direction side of PSP and SPAN-B is on the anti-ram side. Significant savings in mass are realized by combining the electron and ion ESAs, which was a lesson learned from FAST and THEMIS. Electrostatic deflectors extend the narrow planar intrinsic angular field of view, FOV, of each ESA to 240°?120°. Together the SPAN electron sensors provide a nearly 4? sr FOV for electrons only excluding the region of the sky blocked by the heat shield. | |
| 11 | + The SPAN sensors utilize the classic top-hat hemispherical ESA design developed by UCB (Carlson et al. 1983) that affords a uniform response over a planar 360° FOV. Particles entering the analyzer are selected for energy per charge, E/q, by a voltage applied to the inner hemisphere. This voltage is swept from near zero to several kV to measure ion and electron energies as low as a few eV/q to as high as 30 keV/q thus providing excellent energy coverage and resolution. Angular resolution is provided in one plane by discrete segmented anodes and out of that plane by electrostatic deflectors, resulting in a broad instrumental FOV appropriate for a non-spinning spacecraft like PSP. | |
| 12 | + Both ion and electron sensors use microchannel plate, MCP, detectors for particle detection, and discrete anodes for MCP charge collection. The electron sensor uses chevron-pair detectors.Pulse-counting electronics for the electron sensors utilize a multi-channel preamplifier ASIC developed by researchers at the Laboratoire de Physique du Plasmas, LPP, for the Solar Orbiter mission. | |
| 13 | + SPAN-B measures electrons only and is a near duplicate of the SPAN-A e-analyzer as only the anode patterns are different. SPAN-B is mounted in an orthogonal orientation to SPAN-A and it is on the opposite side of the spacecraft. The ability of SWEAP to use the same design for both SPAN-A and SPAN-B electron sensors provides significant savings in design time and analysis. | |
| 14 | + </Description> | |
| 15 | + <Acknowledgement>Acknowledgement to the NASA Parker Solar Probe Mission and the SWEAP team led by J.Kasper for use of data</Acknowledgement> | |
| 16 | + <Contact> | |
| 17 | + <PersonID>spase://SMWG/Person/Justin.C.Kasper</PersonID> | |
| 18 | + <Role>PrincipalInvestigator</Role> | |
| 19 | + </Contact> | |
| 20 | + <Contact> | |
| 21 | + <PersonID>spase://SMWG/Person/Nicola.J.Fox</PersonID> | |
| 22 | + <Role>ProjectScientist</Role> | |
| 23 | + </Contact> | |
| 24 | + <InformationURL> | |
| 25 | + <Name>SWEAP Instruments webpage</Name> | |
| 26 | + <URL>http://sweap.cfa.harvard.edu/SWEAP.html</URL> | |
| 27 | + <Description>SWEAP Instrument Web Page</Description> | |
| 28 | + </InformationURL> | |
| 29 | + </ResourceHeader> | |
| 30 | + <InstrumentType>ElectrostaticAnalyser</InstrumentType> | |
| 31 | + <InvestigationName>Parker Solar Probe SWEAP Investigation</InvestigationName> | |
| 32 | + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/PSP</ObservatoryID> | |
| 33 | + </Instrument> | |
| 34 | +</Spase> | |
| ... | ... |
Instrument/CDPP-AMDA/PSP/SPI.xml
| ... | ... | @@ -7,7 +7,7 @@ |
| 7 | 7 | <ResourceName>SWEAP SPANi</ResourceName> |
| 8 | 8 | <AlternateName>Solar Probe Analyser (SPAN) ion</AlternateName> |
| 9 | 9 | <ReleaseDate>2019-11-12T16:00:05Z</ReleaseDate> |
| 10 | - <Description>The SPAN-Ai instrument uses curved plates to create electrostatic optics that sort incoming ions based on their energy-per-charge and utilizes segmented anodes and leectrostatic deflectors to select particles based on their azimuthal and elevation angles. | |
| 10 | + <Description>The SPAN-Ai instrument uses curved plates to create electrostatic optics that sort incoming ions based on their energy-per-charge and utilizes segmented anodes and electrostatic deflectors to select particles based on their azimuthal and elevation angles. | |
| 11 | 11 | This allows each particle's velocity to be determined. SPAN-Ai alos has time-of-flight electrons that can measure the mass-to-charge ratio of the incoming ions. |
| 12 | 12 | * Sensor Type: Electrostatic Analyzer with Time-of-Flight |
| 13 | 13 | * Particles Measured: Positively charged ions |
| ... | ... |
| ... | ... | @@ -0,0 +1,100 @@ |
| 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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd"> | |
| 3 | + <Version>2.3.1</Version> | |
| 4 | + <NumericalData> | |
| 5 | + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/PSP/SPE/psp-spe-pad</ResourceID> | |
| 6 | + <ResourceHeader> | |
| 7 | + <ResourceName>PAD</ResourceName> | |
| 8 | + <AlternateName>SWEAP SPANe Level 3 spectrogramms</AlternateName> | |
| 9 | + <ReleaseDate>2020-04-12T10:48:29Z</ReleaseDate> | |
| 10 | + <Description> | |
| 11 | + This data set provides spectra of the energy flux versus Energy and pitchangle | |
| 12 | + </Description> | |
| 13 | + <Acknowledgement> | |
| 14 | + Please acknowledge the NASA Parker Solar Probe Mission and SWEAP team led by Justin Kasper for use of data. | |
| 15 | + </Acknowledgement> | |
| 16 | + <Contact> | |
| 17 | + <PersonID>spase://SMWG/Person/Justin.C.Kasper</PersonID> | |
| 18 | + <Role>PrincipalInvestigator</Role> | |
| 19 | + </Contact> | |
| 20 | + <Contact> | |
| 21 | + <PersonID>spase://SMWG/Person/Davin.Larson</PersonID> | |
| 22 | + <Role>ProjectScientist</Role> | |
| 23 | + </Contact> | |
| 24 | + <InformationURL> | |
| 25 | + <Name>Investigation Publication</Name> | |
| 26 | + <URL>https://link.springer.com/article/10.1007%2Fs11214-015-0206-3</URL> | |
| 27 | + <Description> | |
| 28 | + Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus | |
| 29 | + </Description> | |
| 30 | + </InformationURL> | |
| 31 | + </ResourceHeader> | |
| 32 | + <AccessInformation> | |
| 33 | + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> | |
| 34 | + <Availability>Online</Availability> | |
| 35 | + <AccessRights>Open</AccessRights> | |
| 36 | + <AccessURL> | |
| 37 | + <Name>AMDA at CDPP</Name> | |
| 38 | + <URL> | |
| 39 | + http://amda.cdpp.eu | |
| 40 | + </URL> | |
| 41 | + </AccessURL> | |
| 42 | + <Format>Text</Format> | |
| 43 | + <Acknowledgement> | |
| 44 | + AMDA is a science analysis system provided by the Centre de Donnees de la | |
| 45 | + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and | |
| 46 | + Universite Paul Sabatier, Toulouse | |
| 47 | + </Acknowledgement> | |
| 48 | + </AccessInformation> | |
| 49 | + <ProviderName>SPDF</ProviderName> | |
| 50 | + <ProviderResourceName>psp/sweap/spe/l3/spe_sf0_pad/</ProviderResourceName> | |
| 51 | + <ProviderAcknowlegment> | |
| 52 | + Please acknowledge the CDAWeb team at GSFC/SPDF.</ProviderAcknowlegment> | |
| 53 | + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/PSP/SPE</InstrumentID> | |
| 54 | + <MeasurementType>ThermalPlasma</MeasurementType> | |
| 55 | + <TemporalDescription> | |
| 56 | + <TimeSpan> | |
| 57 | + <StartDate>2018-09-02T00:00:12Z</StartDate> | |
| 58 | + <StopDate>2025-08-12T23:59:55Z</StopDate> | |
| 59 | + </TimeSpan> | |
| 60 | + <CadenceMin>PT20S</CadenceMin> | |
| 61 | + <CadenceMax>PT40S</CadenceMax> | |
| 62 | + </TemporalDescription> | |
| 63 | + <ObservedRegion>Heliosphere.Inner</ObservedRegion> | |
| 64 | + <ObservedRegion>Sun.Corona</ObservedRegion> | |
| 65 | + <Parameter> | |
| 66 | + <Name>eflux/ener</Name> | |
| 67 | + <ParameterKey>psp_spe_EvsE</ParameterKey> | |
| 68 | + <Description> | |
| 69 | + Differential Energy Flux vs Energy | |
| 70 | + </Description> | |
| 71 | + <Units>eV/cm**2-s-ster-eV</Units> | |
| 72 | + <RenderingHints> | |
| 73 | + <DisplayType>Spectrogram</DisplayType> | |
| 74 | + </RenderingHints> | |
| 75 | + </Parameter> | |
| 76 | + <Parameter> | |
| 77 | + <Name>eflux/pa</Name> | |
| 78 | + <ParameterKey>psp_spe_Evspa</ParameterKey> | |
| 79 | + <Description> | |
| 80 | + Differential Energy Flux vs Pitch Angle | |
| 81 | + </Description> | |
| 82 | + <Units>eV/cm**2-s-ster-eV</Units> | |
| 83 | + <RenderingHints> | |
| 84 | + <DisplayType>Spectrogram</DisplayType> | |
| 85 | + </RenderingHints> | |
| 86 | + </Parameter> | |
| 87 | + <Parameter> | |
| 88 | + <Name>eflux/ener/pa : 2D</Name> | |
| 89 | + <ParameterKey>psp_spe_EvsEvspa</ParameterKey> | |
| 90 | + <Description> | |
| 91 | + Differential Energy Flux vs Energy and Pitch Angle | |
| 92 | + </Description> | |
| 93 | + <Units>eV/cm**2-s-ster-eV</Units> | |
| 94 | + <RenderingHints> | |
| 95 | + <DisplayType>Spectrogram</DisplayType> | |
| 96 | + </RenderingHints> | |
| 97 | + </Parameter> | |
| 98 | + | |
| 99 | +</NumericalData> | |
| 100 | +</Spase> | |
| ... | ... |