diff --git a/NumericalData/AMDA/Cassini/RPWS/cass-rpws-neproxy.xml b/NumericalData/AMDA/Cassini/RPWS/cass-rpws-neproxy.xml
index afe279c..c7785bb 100644
--- a/NumericalData/AMDA/Cassini/RPWS/cass-rpws-neproxy.xml
+++ b/NumericalData/AMDA/Cassini/RPWS/cass-rpws-neproxy.xml
@@ -5,20 +5,26 @@
spase://CDPP/NumericalData/AMDA/Cassini/RPWS/cass-rpws-neproxy
electron proxy
- 2015-10-19T17:01:00
- Cassini RPWS Neproxy data are taken Planetary Data System
- (NASA).
- Cassini RPWS Neproxy data contains all available RPWS Langmuir probe (LP) floating potentials and secondary products, electron number densities and spacecraft potentials.
- Parameter plotting arguments:
- FLOATING_POTENTIAL : measured electric potential at the probe in volts
- SPACECRAFT_POTENTIAL : electric potential at the spacecraft surface derived from the probe floating potential
- ELECTRON_NUMBER_DENSITY : derived proxy electron number density
+ Langmuir Probe : electron density proxy
+ 2017-10-19T17:01:00
+ Cassini RPWS Neproxy data contains all available RPWS Langmuir probe (LP) floating potentials and secondary products.
+
+ Cassini RPWS Langmuir Probe proxy electron density data are derived
+ using an empirical relation between the floating potential and CAPS
+ measured densities, for the entire mission. Spacecraft potential data
+ are also derived from LP floating potential.
+
- spase://SMWG/Person/Elena.budnik
- TechnicalContact
+ spase://SMWG/Person/William.S.Kurth
+ PrincipalInvestigator
+
+
+ spase://CDPP/Person/J.Wahlund
+ DataProducer
- http://www.lesia.obspm.fr/
+ PDS home page
+ https://pds-ppi.igpp.ucla.edu/data/CO-SS_S-RPWS-5-NEPROXY-V1.0/CATALOG/NEPROXYDS.CAT
@@ -32,8 +38,9 @@
NetCDF
PDS
+ CO-SS_S-RPWS-5-NEPROXY-V1.0
spase://CDPP/Instrument/AMDA/Cassini/RPWS
- Ephemeris
+ ThermalPlasma
2004-08-27T00:03:27Z
@@ -42,8 +49,18 @@
PT640S
Saturn
+ Occasional RPWS Langmuir probe voltage sweeps have interference in
+ individual sweep samples. These samples have been filtered away before
+ analysis and should not pose a problem for the delivered output
+ parameters. The Ufloat proxy method for this data set is applicable only
+ for densities below 5 cm^-3. To avoid uncertainty of the transition
+ region, data are limited to radial distance beyond 7 Rs from Saturn and
+ absolute magnetic latitude above 15 degrees. Also the data inside 10 Rt
+ from Titan are not included for the same reason. The proxy method uses
+ the photoelectron condition directly measured by the instrument and
+ therefore not available when LP is totally in shadow.
- floating pot
+ floating potential
cass_neproxy_fpot
phys.potential;phys.elecField;instr.obsty
V
@@ -55,7 +72,7 @@
- s/c pot
+ s/c potential
cass_neproxy_scpot
phys.potential;phys.elecField;instr.obsty
V
diff --git a/Person/J.Wahlund.xml b/Person/J.Wahlund.xml
new file mode 100644
index 0000000..a140309
--- /dev/null
+++ b/Person/J.Wahlund.xml
@@ -0,0 +1,10 @@
+
+
+ 2.2.0
+
+ spase://CDPP/Person/J.Wahlund
+ Dr. Jan-Erik Wahlund
+ Uppsala university
+ Jan-Erik.Wahlund@rymdfysik.uu.se
+
+
--
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