diff --git a/Instrument/AMDA/Geotail/EPIC.xml b/Instrument/AMDA/Geotail/EPIC.xml
index 159e0cf..7dcfc25 100644
--- a/Instrument/AMDA/Geotail/EPIC.xml
+++ b/Instrument/AMDA/Geotail/EPIC.xml
@@ -7,9 +7,9 @@
EPIC
Energetic Particles and Ion Composition instrument
2017-02-04T12:34:56.789
- The Energetic Particles and Ion Composition (EPIC) instrument (block diagram) is actually composed of two separate sensor and processing assemblies.
- * The STICS assembly (Supra-Thermal Ion Composition Spectrometer) uses a quadrispherical electrostatic analyzer followed by a foil/solid state detector time-of-flight (TOF) telecope to measure charge state, mass and energy of ions with energies of 30 - 230 keV/charge. It uses an electrostatic analyzer with a geometry factor of 0.05 cm**2 sr, time of flight and energy analysis.
- * The ICS assembly (Ion Composition Subsystem) measures mass and energy properties of energetic ions with energies of less than 50 keV to 3 MeV. It uses a pair of collimators with sweeping magnets to reject electrons, followed by TOF and energy analysis, with a geometry factor of 0.2 cm**2 sr. A thin foil/solid state detector electron telescope measures electrons higher than 30 keV.
+ The Energetic Particles and Ion Composition (EPIC) instrument is actually composed of two separate sensor and processing assemblies.
+ * The STICS assembly (Supra-Thermal Ion Composition Spectrometer) uses a quadrispherical electrostatic analyzer followed by a foil/solid state detector time-of-flight (TOF) telecope to measure charge state, mass and energy of ions with energies of 30 - 230 keV/charge. It uses an electrostatic analyzer with a geometry factor of 0.05 cm^2 sr, time of flight and energy analysis.
+ * The ICS assembly (Ion Composition Subsystem) measures mass and energy properties of energetic ions with energies of less than 50 keV to 3 MeV. It uses a pair of collimators with sweeping magnets to reject electrons, followed by TOF and energy analysis, with a geometry factor of 0.2 cm^2 sr. A thin foil/solid state detector electron telescope measures electrons higher than 30 keV.
spase://SMWG/Person/Donald.J.Williams
diff --git a/Instrument/AMDA/Geotail/LEP.xml b/Instrument/AMDA/Geotail/LEP.xml
index a0a4bb5..628ba01 100644
--- a/Instrument/AMDA/Geotail/LEP.xml
+++ b/Instrument/AMDA/Geotail/LEP.xml
@@ -20,10 +20,6 @@
spase://SMWG/Person/Donald.H.Fairfield
Scientist
-
- spase://SMWG/Person/Jan.Merka
- MetadataContact
-
The Geotail Low Energy Particle Experiment (LEP)
http://www.darts.isas.ac.jp/stp/geotail/jgg_lep.pdf
diff --git a/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-ed.xml b/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-ed.xml
index 19c956a..34770ef 100644
--- a/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-ed.xml
+++ b/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-ed.xml
@@ -4,21 +4,24 @@
spase://CDPP/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-ed
- ED : electron flux
- Electron Detector :
+ ED : electron flux : E > 34 keV
+ Electron Detector : electron integral flux : E > 34 keV
2017-02-12T10:48:29Z
- *'directionward' (tailward, etc) : the correspondinf sector is taken
+ *'directionward' (tailward, etc) : the corresponding sector is taken
* Sectors (degrees) : 0., 45., 90., 135., 180., 225., 270., 315.;
-
-
-
+
+ spase://CDPP/Person/Stuart.Nyland
+ DataProducer
+
+
+ spase://CDPP/Person/Elena.Budnik
+ TechnicalContact
+
-
-
-
-
+
+
@@ -32,7 +35,7 @@
CDF
-
+ JHU/APL
spase://CDPP/Instrument/AMDA/Geotail/EPIC
EnergeticParticles
@@ -42,19 +45,18 @@
PT3S
- Comet
-
-
+ Earth.Magnetosphere
+
- integral flux : E > 34 keV
+ e- flux
gtl_edhigh_av
-
-
-
-
-
+ 1/(cm**2-s-sr-kev)
+
+ Electron
+ NumberFlux
+
-
+
diff --git a/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-phigh.xml b/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-phigh.xml
new file mode 100644
index 0000000..4c98fd4
--- /dev/null
+++ b/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-phigh.xml
@@ -0,0 +1,67 @@
+
+
+ 2.2.6
+
+ spase://CDPP/NumericalData/AMDA/GEOTAIL/EPIC/gtl-epic-phigh
+
+ P2 : proton flux
+ P2 : proton flux : 58 - 77 keV : averaged over two heads
+ 2017-02-12T10:48:29Z
+
+
+
+ spase://CDPP/Person/Stuart.Nyland
+ DataProducer
+
+
+ spase://CDPP/Person/Elena.Budnik
+ TechnicalContact
+
+
+
+
+
+
+
+ gtl-ics-high
+ PartOf
+ ICS : high resolution : profile
+
+
+
+ spase://SMWG/Repository/CDPP/AMDA
+ Online
+ Open
+
+ AMDA at CDPP
+ http://amda.cdpp.eu
+
+ CDF
+
+
+ JHU/APL
+ spase://CDPP/Instrument/AMDA/Geotail/EPIC
+ EnergeticParticles
+
+
+ 1992-10-18T00:01:17Z
+ 2010-12-31T23:57:50Z
+
+ PT6S
+
+ Earth.Magnetosphere
+
+
+
+ proton flux
+ gtl_phigh_av
+
+
+ 1/(cm**2-s-sr-kev)
+
+ Proton
+ NumberFlux
+
+
+
+
diff --git a/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-edb.xml b/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-edb.xml
index db5c8a0..eecd59e 100644
--- a/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-edb.xml
+++ b/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-edb.xml
@@ -22,14 +22,6 @@
spase://SMWG/Person/Donald.H.Fairfield
Scientist
-
- spase://SMWG/Person/Jan.Merka
- MetadataContact
-
-
- spase://SMWG/Person/Elena.Budnik
- TechnicalContact
-
The Geotail Low Energy Particle Experiment (LEP)
http://www.darts.isas.ac.jp/stp/geotail/jgg_lep.pdf
diff --git a/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-k0.xml b/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-k0.xml
index 85fc644..c82e21e 100644
--- a/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-k0.xml
+++ b/NumericalData/AMDA/GEOTAIL/LEP/gtl-lep-k0.xml
@@ -17,14 +17,6 @@
spase://SMWG/Person/Donald.H.Fairfield
Scientist
-
- spase://SMWG/Person/Jan.Merka
- MetadataContact
-
-
- spase://SMWG/Person/Elena.Budnik
- TechnicalContact
-
The Geotail Low Energy Particle Experiment (LEP)
http://www.darts.isas.ac.jp/stp/geotail/jgg_lep.pdf
diff --git a/Person/Stuart.Nyland.xml b/Person/Stuart.Nyland.xml
new file mode 100644
index 0000000..0ffb5c6
--- /dev/null
+++ b/Person/Stuart.Nyland.xml
@@ -0,0 +1,10 @@
+
+
+ 2.2.0
+
+ spase://CDPP/Person/Stuart.Nyland
+ Dr. Stuart Nyland
+ Applied Physics Laboratory, Johns Hopkins University
+ Stu.Nylund@jhuapl.edu
+
+
--
libgit2 0.21.2