CDPP / CNES

Commit 1a6c8f9b2f6f0390b135296f554dc06fa021aa65

Authored by Elena.Budnik
1 parent dd7fd46c
Exists in master and in 11 other branches amdadev, aschulz, autocommit, bepi_master, bepi_update, cleanup_registry, cleanup_registry_master, cleanup_registry_merged, juice_jdc, juno_jade, soar

ULYSSES SWICS Instrument

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Instrument/CDPP-AMDA/Ulysses/SWICS.xml 0 → 100644
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  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>2.3.1</Version>
  4 + <Instrument>
  5 + <ResourceID>spase://CNES/Instrument/CDPP-AMDA/Ulysses/SWICS</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>SWICS</ResourceName>
  8 + <AlternateName>Solar Wind Ion Composition Spectrometer</AlternateName>
  9 + <AlternateName>GLG</AlternateName>
  10 + <ReleaseDate>2019-05-05T12:34:56Z</ReleaseDate>
  11 + <Description>The Solar Wind Ion Composition Spectrometer (SWICS) on Ulysses is designed to determine uniquely the elemental and
  12 + ionic-charge composition, and the temperatures and mean speeds of all major solar-wind ions, from H through Fe, at solar wind
  13 + speeds ranging from 175 km/s (protons) to 1280 km/s (Fe8+). The instrument, which covers an energy per charge range from 0.16
  14 + to 59.6 keV/e in ~13 min, combines an electrostatic analyzer with post-acceleration, followed by a time-of-flight and energy measurement.
  15 + The measurements made by SWICS will have an impact on many areas of solar and heliospheric physics, in particular providing essential
  16 + and unique information on: (i) conditions and processes in the region of the corona where the solar wind is accelerated; (ii) the
  17 + location of the source regions of the solar wind in the corona; (iii) coronal heating processes; (iv) the extent and causes of
  18 + variations in the composition of the solar atmosphere; (v) plasma processes in the solar wind; (vi) the acceleration of energetic
  19 + particles in the solar wind; (vii) the thermalization and acceleration of interstellar ions in the solar wind, and their composition;
  20 + and (viii) the composition, charge states and behavior of the plasma in various regions of the Jovian magnetosphere.</Description>
  21 + <Contact>
  22 + <PersonID>spase://SMWG/Person/George.Gloeckler</PersonID>
  23 + <Role>PrincipalInvestigator</Role>
  24 + </Contact>
  25 + <InformationURL>
  26 + <Name>Instrument description at ESA's cosmos portal</Name>
  27 + <URL>https://www.cosmos.esa.int/web/ulysses/swics-instrument</URL>
  28 + </InformationURL>
  29 + </ResourceHeader>
  30 + <InstrumentType>EnergeticParticleInstrument</InstrumentType>
  31 + <InvestigationName>Solar Wind Ion Composition Spectrometer (GLG/SWICS) on Ulysses</InvestigationName>
  32 + <ObservatoryID>spase://CNES/Observatory/CDPP-AMDA/Ulysses</ObservatoryID>
  33 + </Instrument>
  34 +</Spase>
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