From 695c129a68dd8fe638ced6189767e7c96dd7ff10 Mon Sep 17 00:00:00 2001
From: Elena.Budnik <ebudnik@irap.omp.eu>
Date: Mon, 26 Sep 2016 10:22:27 +0200
Subject: [PATCH] new instr

---
 Instrument/AMDA/MAVEN/SEP.xml | 50 ++++++++++++++++++++++++++++++++++++++++++++++++++
 1 file changed, 50 insertions(+), 0 deletions(-)
 create mode 100644 Instrument/AMDA/MAVEN/SEP.xml

diff --git a/Instrument/AMDA/MAVEN/SEP.xml b/Instrument/AMDA/MAVEN/SEP.xml
new file mode 100644
index 0000000..5b55da1
--- /dev/null
+++ b/Instrument/AMDA/MAVEN/SEP.xml
@@ -0,0 +1,50 @@
+<?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://www.spase-group.org/data/schema/spase-2_2_6.xsd">
+  <Version>2.2.6</Version>
+  <Instrument>
+    <ResourceID>spase://CDPP/Instrument/AMDA/MAVEN/SEP</ResourceID>
+    <ResourceHeader>
+      <ResourceName>SEP</ResourceName>
+      <AlternateName>Solar Energetic Particle</AlternateName>
+      <ReleaseDate>2016-08-01T22:37:00Z</ReleaseDate>
+      <Description>The Solar Energetic Particle (SEP) instrument is part of the Particles and Fields 
+        Package and determines the impact of SEPs on the upper atmosphere.
+
+Goals:
+    * Determine SEP input into the atmosphere as a function of altitude
+    * Determine SEP heating, ionization, and sputtering of upper atmosphere
+    * Detect the highest energy pickup ions (>30 to 100s of keV)
+
+Observations:
+    * Characterize solar particles in an energy range that affects upper atmosphere and ionospheric processes (~120 – 200 km)
+    * Time resolution adequate to capture major SEP events ( less 1 hour)
+    
+ Technical details and heritage:
+    * Two dual double-ended telescopes
+    * Four look directions per species, optimized for parallel and perpendicular Parker Spiral viewing
+    * Protons and heavier ions from ~25 keV to 12 MeV
+    * Electrons from ~25 keV to 1 MeV
+    * Energy fluxes 10 to 106 eV/cm2-sec-ster-eV
+    * Better than 50% energy resolution
+    * Heritage from (nearly identical to) SST on THEMIS
+      </Description>
+      <Contact>       
+        <PersonID>spase://SMWG/Person/Davin.Larson</PersonID>
+        <Role>PrincipalInvestigator</Role>
+      </Contact>
+      <InformationURL>
+        <Name>SEP web page, Summary sheet </Name>
+        <URL>http://lasp.colorado.edu/home/maven/science/instrument-package/sep/</URL>
+      </InformationURL>      
+    </ResourceHeader>
+   <InstrumentType>ParticleDetector</InstrumentType>
+    <InvestigationName></InvestigationName>
+    <OperatingSpan>
+      <StartDate>2013-11-18T13:28:00</StartDate>
+      <!--StopDate>2014-12-16T00:00:00</StopDate-->
+      <!-- Note :  Mission phases : multiple tags possible -->
+      <Note>Mars arrival : 2014-09-28T19:24:00</Note>
+    </OperatingSpan>
+    <ObservatoryID>spase://CDPP/Observatory/AMDA/MAVEN</ObservatoryID>
+  </Instrument>
+</Spase>
--
libgit2 0.21.2