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 + + -- libgit2 0.21.2