From cc8f921e8a1ef8adcfbd1491d3584675aab2da02 Mon Sep 17 00:00:00 2001 From: Quentin Brzustowski <quentin.brzustowski@irap.omp.eu> Date: Wed, 12 Feb 2020 17:03:05 +0100 Subject: [PATCH] Created instruments PSP/ISOIS/epiHi and epiLow and dataset HET --- Instrument/CDPP-AMDA/PSP/epiHi.xml | 45 +++++++++++++++++++++++++++++++++++++++++++++ Instrument/CDPP-AMDA/PSP/epiLo.xml | 52 ++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min.xml | 132 ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ 3 files changed, 229 insertions(+), 0 deletions(-) create mode 100644 Instrument/CDPP-AMDA/PSP/epiHi.xml create mode 100644 Instrument/CDPP-AMDA/PSP/epiLo.xml create mode 100644 NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min.xml diff --git a/Instrument/CDPP-AMDA/PSP/epiHi.xml b/Instrument/CDPP-AMDA/PSP/epiHi.xml new file mode 100644 index 0000000..42d4e4b --- /dev/null +++ b/Instrument/CDPP-AMDA/PSP/epiHi.xml @@ -0,0 +1,45 @@ +<?xml version="1.0" encoding="UTF-8"?> +<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"> + <Version>2.2.6</Version> + <Instrument> + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/PSP/epiHi</ResourceID> + <ResourceHeader> + <ResourceName>ISoIS EPI-Hi</ResourceName> + <AlternateName>Energetic Particle Instrument Hi-Energy</AlternateName> + <ReleaseDate>2019-11-12T16:00:05Z</ReleaseDate> + <Description>The science objective of the Integrated Science Investigation of the Sun, ISOIS, + experiment is to explore the physical mechanisms that produce, accelerate, and transport energetic + particles in the inner heliosphere. This will be achieved by observing energetic electrons, protons, + and heavy ions in the Sun's atmosphere and inner heliosphere to learn about the origin and seed population + of solar energetic particles, how these and other particles are accelerated, and what mechanisms are + responsible for transporting the different particle populations into the heliosphere. It will also + contribute to tracing the flow of energy that heats and accelerates the solar corona and solar wind, + and determining the structure and dynamics of the plasma and magnetic fields at the sources of the solar wind. + The Integrated Science Investigation of the Sun consists of two instruments, EPI-Lo and EPI-Hi, mounted on + the side of the spacecraft near the back ram-facing side, protected by the heat shield. + The EPI-Hi instrument system is based on ion-implanted solid-state detectors. It comprises three detector stacks + (particle telescopes). One is designated a High Energy Telescope (HET) and two are designated Low-Energy Telescopes (LET1 and LET2). + </Description> + <Acknowledgement>Please Acknowledge the National Aeronautics and Space Administration, NASA</Acknowledgement> + <Contact> + <PersonID>spase://SMWG/Person/David.J.McComas</PersonID> + <Role>PrincipalInvestigator</Role> + </Contact> + <Contact> + <PersonID>spase://SMWG/Person/Eric.R.Christian</PersonID> + <Role>DeputyPI</Role> + </Contact> + <InformationURL> + <Name>Parker Solar Probe Mission Instrument web page, JPL</Name> + <URL>http://parkersolarprobe.jhuapl.edu/Spacecraft/index.php#Instruments</URL> + </InformationURL> + <InformationURL> + <Name>Parker Solar Probe Mission Instrument web page, NASA</Name> + <URL>https://www.nasa.gov/content/goddard/parker-solar-probe-instruments/</URL> + </InformationURL> + </ResourceHeader> + <InstrumentType>SolidStateDetector</InstrumentType> + <InvestigationName>Parker Solar Probe ISOIS Investigation</InvestigationName> + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/PSP</ObservatoryID> + </Instrument> +</Spase> diff --git a/Instrument/CDPP-AMDA/PSP/epiLo.xml b/Instrument/CDPP-AMDA/PSP/epiLo.xml new file mode 100644 index 0000000..8822af3 --- /dev/null +++ b/Instrument/CDPP-AMDA/PSP/epiLo.xml @@ -0,0 +1,52 @@ +<?xml version="1.0" encoding="UTF-8"?> +<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"> + <Version>2.2.6</Version> + <Instrument> + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/PSP/epiLo</ResourceID> + <ResourceHeader> + <ResourceName>ISoIS EPI-Lo</ResourceName> + <AlternateName>Energetic Particle Instrument Low-Energy</AlternateName> + <ReleaseDate>2019-11-12T16:00:05Z</ReleaseDate> + <Description>The science objective of the Integrated Science Investigation of the Sun, ISOIS, + experiment is to explore the physical mechanisms that produce, accelerate, and transport energetic + particles in the inner heliosphere. This will be achieved by observing energetic electrons, protons, + and heavy ions in the Sun's atmosphere and inner heliosphere to learn about the origin and seed population + of solar energetic particles, how these and other particles are accelerated, and what mechanisms are + responsible for transporting the different particle populations into the heliosphere. It will also + contribute to tracing the flow of energy that heats and accelerates the solar corona and solar wind, + and determining the structure and dynamics of the plasma and magnetic fields at the sources of the solar wind. + The Integrated Science Investigation of the Sun consists of two instruments, EPI-Lo and EPI-Hi, mounted on + the side of the spacecraft near the back ram-facing side, protected by the heat shield. + The EPI-Lo instrument is disc-shaped and divided into 8 sections, or wedge assemblies, each section holding 10 + foil-covered apertures. Each aperture faces a slightly different direction, together they provide coverage of + nearly a full hemisphere. The apertures allow particles to enter the wedge interior, which contains a time-of-flight + mass spectrometer. Ions pass through the thin foils in the apertures and then hit a stop foil backed by a + solid-state detector. Electrons are detected by independent solid-state detectors covered by ~2 micron thick + aluminum flashing. Epi-Lo measures energetic ions from 0.02 MeV/n to 15 MeV total energy, protons from + about 0.04 MeV to 7 MeV, and energetic electrons from approximately 25 keV to 1000 keV. + It measures the ion composition and pitch-angle distributions from 30 keV/n up to 0.3 MeV/n or 1.0 MeV/n + every 5 or 30 seconds. It can return data for up to 64 energy bins and 80 angular ranges (one for each aperture). + </Description> + <Acknowledgement>Please Acknowledge the National Aeronautics and Space Administration, NASA</Acknowledgement> + <Contact> + <PersonID>spase://SMWG/Person/David.J.McComas</PersonID> + <Role>PrincipalInvestigator</Role> + </Contact> + <Contact> + <PersonID>spase://SMWG/Person/Eric.R.Christian</PersonID> + <Role>DeputyPI</Role> + </Contact> + <InformationURL> + <Name>Parker Solar Probe Mission Instrument web page, JPL</Name> + <URL>http://parkersolarprobe.jhuapl.edu/Spacecraft/index.php#Instruments</URL> + </InformationURL> + <InformationURL> + <Name>Parker Solar Probe Mission Instrument web page, NASA</Name> + <URL>https://www.nasa.gov/content/goddard/parker-solar-probe-instruments/</URL> + </InformationURL> + </ResourceHeader> + <InstrumentType>MassSpectrometer</InstrumentType> + <InvestigationName>Parker Solar Probe ISOIS Investigation</InvestigationName> + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/PSP</ObservatoryID> + </Instrument> +</Spase> diff --git a/NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min.xml b/NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min.xml new file mode 100644 index 0000000..70161da --- /dev/null +++ b/NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min.xml @@ -0,0 +1,132 @@ +<?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_3_0.xsd"> + <Version>2.3.0</Version> + <NumericalData> + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/PSP/epiHi/psp-het-1min</ResourceID> + <ResourceHeader> + <ResourceName>HET 1min</ResourceName> + <AlternateName>High Energy Telescope 1 min rate</AlternateName> + <ReleaseDate>2019-11-12T10:48:29Z</ReleaseDate> + <Description> + The HET is a cylinder containing a central stack of detector disks and two single detector disks, + one at each end. The individual detectors in the central stack have thicknesses of 1000 microns. + Three of the detectors in the central stack comprise two 1000-micron disks connected to act as single + 2000 micron detectors. The end detector disks are 500 microns thick. The front end detector and the + outermost detectors at each end of the central stack are each divided into five active elements, + a central bulls-eye and four quadrants, each of equal area. Which active area hit on different disks + gives directional information on the particle. An outer annular segment of each detector acts as an + anti-coincidence shield to detect particles that exit the cylinder before passing through all the detectors. + The HET covers electrons up to approximately 6 MeV and protons and heavy ions to at least 100 MeV/n. + The lower range overlaps the high end of the Low Energy Telescopes. + The measurements are divided into two different sides of the instrument, A and B + </Description> + <Acknowledgement> + Please acknowledge the National Aeronautics and Space Administration, NASA + </Acknowledgement> + <Contact> + <PersonID>spase://SMWG/Person/David.J.McComas</PersonID> + <Role>PrincipalInvestigator</Role> + </Contact> + <Contact> + <PersonID>spase://SMWG/Person/Eric.R.Christan</PersonID> + <Role>DeputyPI</Role> + </Contact> + <InformationURL> + <Name>PSP/ISoIS Energetic Particle Data - User Guide</Name> + <URL>https://spdf.sci.gsfc.nasa.gov/pub/data/psp/isois/ISOIS_Data_Glossary.pdf</URL> + </InformationURL> + <InformationURL> + <Name>Parker Solar Probe Mission Instrument web page, JPL</Name> + <URL>http://parkersolarprobe.jhuapl.edu/Spacecraft/index.php#Instruments</URL> + </InformationURL> + </ResourceHeader> + <AccessInformation> + <RepositoryID>spase://SMWG/Repository/CNES/CDPP-AMDA</RepositoryID> + <Availability>Online</Availability> + <AccessRights>Open</AccessRights> + <AccessURL> + <Name>AMDA at CDPP</Name> + <URL> + http://amda.cdpp.eu + </URL> + </AccessURL> + <Format>Text</Format> + <Acknowledgement> + AMDA is a science analysis system provided by the Centre de Donnees de la + Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and + Universite Paul Sabatier, Toulouse + </Acknowledgement> + </AccessInformation> + <ProviderName>SPDF</ProviderName> + <ProviderResourceName>psp/fields/l2/mag_rtn_1min/</ProviderResourceName> + <ProviderAcknowlegment> + Please acknowledge the CDAWeb team at GSFC/SPDF.</ProviderAcknowlegment> + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/PSP/MAG</InstrumentID> + <MeasurementType>EnergeticParticles</MeasurementType> + <TemporalDescription> + <TimeSpan> + <StartDate>2018-09-02T00:00:12Z</StartDate> + <StopDate>2025-08-12T23:59:55Z</StopDate> + </TimeSpan> + <Cadence>PT60S</Cadence> + </TemporalDescription> + <ObservedRegion>Heliosphere.Inner</ObservedRegion> + <ObservedRegion>Sun.Corona</ObservedRegion> + <Parameter> + <Name>H flux side A</Name> + <ParameterKey>psp_het_1min_AHf</ParameterKey> + <Description> + Proton flux side A + </Description> + <Units>1/cm²/sr/s/(MeV/nuc)</Units> + <RenderingHints> + <DisplayType>Spectrogram</DisplayType> + </RenderingHints> + <Particle> + <ParticleQuantity>EnergyFlux</ParticleQuantity> + </Particle> + </Parameter> + <Parameter> + <Name>H flux side B</Name> + <ParameterKey>psp_het_1min_BHf</ParameterKey> + <Description> + Proton flux side B + </Description> + <Units>1/cm²/sr/s/(MeV/nuc)</Units> + <RenderingHints> + <DisplayType>Spectrogram</DisplayType> + </RenderingHints> + <Particle> + <ParticleQuantity>EnergyFlux</ParticleQuantity> + </Particle> + </Parameter> + <Parameter> + <Name>He flux side A</Name> + <ParameterKey>psp_het_1min_AHef</ParameterKey> + <Description> + Helium flux side A + </Description> + <Units>1/cm²/sr/s/(MeV/nuc)</Units> + <RenderingHints> + <DisplayType>Spectrogram</DisplayType> + </RenderingHints> + <Particle> + <ParticleQuantity>EnergyFlux</ParticleQuantity> + </Particle> + </Parameter> + <Parameter> + <Name>He flux side B</Name> + <ParameterKey>psp_het_1min_BHef</ParameterKey> + <Description> + Helium flux side B + </Description> + <Units>1/cm²/sr/s/(MeV/nuc)</Units> + <RenderingHints> + <DisplayType>Spectrogram</DisplayType> + </RenderingHints> + <Particle> + <ParticleQuantity>EnergyFlux</ParticleQuantity> + </Particle> + </Parameter> +</NumericalData> +</Spase> -- libgit2 0.21.2