Commit 695c129a68dd8fe638ced6189767e7c96dd7ff10
1 parent
71185d00
Exists in
master
and in
12 other branches
new instr
Showing
1 changed file
with
50 additions
and
0 deletions
Show diff stats
| @@ -0,0 +1,50 @@ | @@ -0,0 +1,50 @@ | ||
| 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://www.spase-group.org/data/schema/spase-2_2_6.xsd"> | ||
| 3 | + <Version>2.2.6</Version> | ||
| 4 | + <Instrument> | ||
| 5 | + <ResourceID>spase://CDPP/Instrument/AMDA/MAVEN/SEP</ResourceID> | ||
| 6 | + <ResourceHeader> | ||
| 7 | + <ResourceName>SEP</ResourceName> | ||
| 8 | + <AlternateName>Solar Energetic Particle</AlternateName> | ||
| 9 | + <ReleaseDate>2016-08-01T22:37:00Z</ReleaseDate> | ||
| 10 | + <Description>The Solar Energetic Particle (SEP) instrument is part of the Particles and Fields | ||
| 11 | + Package and determines the impact of SEPs on the upper atmosphere. | ||
| 12 | + | ||
| 13 | +Goals: | ||
| 14 | + * Determine SEP input into the atmosphere as a function of altitude | ||
| 15 | + * Determine SEP heating, ionization, and sputtering of upper atmosphere | ||
| 16 | + * Detect the highest energy pickup ions (>30 to 100s of keV) | ||
| 17 | + | ||
| 18 | +Observations: | ||
| 19 | + * Characterize solar particles in an energy range that affects upper atmosphere and ionospheric processes (~120 – 200 km) | ||
| 20 | + * Time resolution adequate to capture major SEP events ( less 1 hour) | ||
| 21 | + | ||
| 22 | + Technical details and heritage: | ||
| 23 | + * Two dual double-ended telescopes | ||
| 24 | + * Four look directions per species, optimized for parallel and perpendicular Parker Spiral viewing | ||
| 25 | + * Protons and heavier ions from ~25 keV to 12 MeV | ||
| 26 | + * Electrons from ~25 keV to 1 MeV | ||
| 27 | + * Energy fluxes 10 to 106 eV/cm2-sec-ster-eV | ||
| 28 | + * Better than 50% energy resolution | ||
| 29 | + * Heritage from (nearly identical to) SST on THEMIS | ||
| 30 | + </Description> | ||
| 31 | + <Contact> | ||
| 32 | + <PersonID>spase://SMWG/Person/Davin.Larson</PersonID> | ||
| 33 | + <Role>PrincipalInvestigator</Role> | ||
| 34 | + </Contact> | ||
| 35 | + <InformationURL> | ||
| 36 | + <Name>SEP web page, Summary sheet </Name> | ||
| 37 | + <URL>http://lasp.colorado.edu/home/maven/science/instrument-package/sep/</URL> | ||
| 38 | + </InformationURL> | ||
| 39 | + </ResourceHeader> | ||
| 40 | + <InstrumentType>ParticleDetector</InstrumentType> | ||
| 41 | + <InvestigationName></InvestigationName> | ||
| 42 | + <OperatingSpan> | ||
| 43 | + <StartDate>2013-11-18T13:28:00</StartDate> | ||
| 44 | + <!--StopDate>2014-12-16T00:00:00</StopDate--> | ||
| 45 | + <!-- Note : Mission phases : multiple tags possible --> | ||
| 46 | + <Note>Mars arrival : 2014-09-28T19:24:00</Note> | ||
| 47 | + </OperatingSpan> | ||
| 48 | + <ObservatoryID>spase://CDPP/Observatory/AMDA/MAVEN</ObservatoryID> | ||
| 49 | + </Instrument> | ||
| 50 | +</Spase> |