From fb015f802e4d455e7dd547075e7df7d8635c16b1 Mon Sep 17 00:00:00 2001
From: Quentin Brzustowski <quentin.brzustowski@irap.omp.eu>
Date: Mon, 4 May 2020 13:27:27 +0200
Subject: [PATCH] added PSP SPE
---
Instrument/CDPP-AMDA/PSP/SPE.xml | 34 ++++++++++++++++++++++++++++++++++
Instrument/CDPP-AMDA/PSP/SPI.xml | 2 +-
NumericalData/CDPP-AMDA/PSP/SPE/psp-spe-pad.xml | 100 ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
3 files changed, 135 insertions(+), 1 deletion(-)
create mode 100644 Instrument/CDPP-AMDA/PSP/SPE.xml
create mode 100644 NumericalData/CDPP-AMDA/PSP/SPE/psp-spe-pad.xml
diff --git a/Instrument/CDPP-AMDA/PSP/SPE.xml b/Instrument/CDPP-AMDA/PSP/SPE.xml
new file mode 100644
index 0000000..91be28e
--- /dev/null
+++ b/Instrument/CDPP-AMDA/PSP/SPE.xml
@@ -0,0 +1,34 @@
+<?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/SPE</ResourceID>
+ <ResourceHeader>
+ <ResourceName>SWEAP SPANe</ResourceName>
+ <AlternateName>Solar Probe Analyser (SPAN) electrons</AlternateName>
+ <ReleaseDate>2019-11-12T16:00:05Z</ReleaseDate>
+ <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.
+ 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.
+ 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.
+ 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.
+ </Description>
+ <Acknowledgement>Acknowledgement to the NASA Parker Solar Probe Mission and the SWEAP team led by J.Kasper for use of data</Acknowledgement>
+ <Contact>
+ <PersonID>spase://SMWG/Person/Justin.C.Kasper</PersonID>
+ <Role>PrincipalInvestigator</Role>
+ </Contact>
+ <Contact>
+ <PersonID>spase://SMWG/Person/Nicola.J.Fox</PersonID>
+ <Role>ProjectScientist</Role>
+ </Contact>
+ <InformationURL>
+ <Name>SWEAP Instruments webpage</Name>
+ <URL>http://sweap.cfa.harvard.edu/SWEAP.html</URL>
+ <Description>SWEAP Instrument Web Page</Description>
+ </InformationURL>
+ </ResourceHeader>
+ <InstrumentType>ElectrostaticAnalyser</InstrumentType>
+ <InvestigationName>Parker Solar Probe SWEAP Investigation</InvestigationName>
+ <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/PSP</ObservatoryID>
+ </Instrument>
+</Spase>
diff --git a/Instrument/CDPP-AMDA/PSP/SPI.xml b/Instrument/CDPP-AMDA/PSP/SPI.xml
index 0e9bf10..81e1a67 100644
--- a/Instrument/CDPP-AMDA/PSP/SPI.xml
+++ b/Instrument/CDPP-AMDA/PSP/SPI.xml
@@ -7,7 +7,7 @@
<ResourceName>SWEAP SPANi</ResourceName>
<AlternateName>Solar Probe Analyser (SPAN) ion</AlternateName>
<ReleaseDate>2019-11-12T16:00:05Z</ReleaseDate>
- <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.
+ <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.
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.
* Sensor Type: Electrostatic Analyzer with Time-of-Flight
* Particles Measured: Positively charged ions
diff --git a/NumericalData/CDPP-AMDA/PSP/SPE/psp-spe-pad.xml b/NumericalData/CDPP-AMDA/PSP/SPE/psp-spe-pad.xml
new file mode 100644
index 0000000..9acd178
--- /dev/null
+++ b/NumericalData/CDPP-AMDA/PSP/SPE/psp-spe-pad.xml
@@ -0,0 +1,100 @@
+<?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://amda.irap.omp.eu/public/schemas/spase-2_3_1.xsd">
+ <Version>2.3.1</Version>
+ <NumericalData>
+ <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/PSP/SPE/psp-spe-pad</ResourceID>
+ <ResourceHeader>
+ <ResourceName>PAD</ResourceName>
+ <AlternateName>SWEAP SPANe Level 3 spectrogramms</AlternateName>
+ <ReleaseDate>2020-04-12T10:48:29Z</ReleaseDate>
+ <Description>
+ This data set provides spectra of the energy flux versus Energy and pitchangle
+ </Description>
+ <Acknowledgement>
+ Please acknowledge the NASA Parker Solar Probe Mission and SWEAP team led by Justin Kasper for use of data.
+ </Acknowledgement>
+ <Contact>
+ <PersonID>spase://SMWG/Person/Justin.C.Kasper</PersonID>
+ <Role>PrincipalInvestigator</Role>
+ </Contact>
+ <Contact>
+ <PersonID>spase://SMWG/Person/Davin.Larson</PersonID>
+ <Role>ProjectScientist</Role>
+ </Contact>
+ <InformationURL>
+ <Name>Investigation Publication</Name>
+ <URL>https://link.springer.com/article/10.1007%2Fs11214-015-0206-3</URL>
+ <Description>
+ Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus
+ </Description>
+ </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/sweap/spe/l3/spe_sf0_pad/</ProviderResourceName>
+ <ProviderAcknowlegment>
+ Please acknowledge the CDAWeb team at GSFC/SPDF.</ProviderAcknowlegment>
+ <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/PSP/SPE</InstrumentID>
+ <MeasurementType>ThermalPlasma</MeasurementType>
+ <TemporalDescription>
+ <TimeSpan>
+ <StartDate>2018-09-02T00:00:12Z</StartDate>
+ <StopDate>2025-08-12T23:59:55Z</StopDate>
+ </TimeSpan>
+ <CadenceMin>PT20S</CadenceMin>
+ <CadenceMax>PT40S</CadenceMax>
+ </TemporalDescription>
+ <ObservedRegion>Heliosphere.Inner</ObservedRegion>
+ <ObservedRegion>Sun.Corona</ObservedRegion>
+ <Parameter>
+ <Name>eflux/ener</Name>
+ <ParameterKey>psp_spe_EvsE</ParameterKey>
+ <Description>
+ Differential Energy Flux vs Energy
+ </Description>
+ <Units>eV/cm**2-s-ster-eV</Units>
+ <RenderingHints>
+ <DisplayType>Spectrogram</DisplayType>
+ </RenderingHints>
+ </Parameter>
+ <Parameter>
+ <Name>eflux/pa</Name>
+ <ParameterKey>psp_spe_Evspa</ParameterKey>
+ <Description>
+ Differential Energy Flux vs Pitch Angle
+ </Description>
+ <Units>eV/cm**2-s-ster-eV</Units>
+ <RenderingHints>
+ <DisplayType>Spectrogram</DisplayType>
+ </RenderingHints>
+ </Parameter>
+ <Parameter>
+ <Name>eflux/ener/pa : 2D</Name>
+ <ParameterKey>psp_spe_EvsEvspa</ParameterKey>
+ <Description>
+ Differential Energy Flux vs Energy and Pitch Angle
+ </Description>
+ <Units>eV/cm**2-s-ster-eV</Units>
+ <RenderingHints>
+ <DisplayType>Spectrogram</DisplayType>
+ </RenderingHints>
+ </Parameter>
+
+</NumericalData>
+</Spase>
--
libgit2 0.21.2