From 964c4231d905d20cf468d78dab53e54c1b414ca9 Mon Sep 17 00:00:00 2001 From: Elena.Budnik Date: Thu, 22 Aug 2019 10:26:32 +0200 Subject: [PATCH] MESS spec param def --- NumericalData/AMDA/MESSENGER/EPS/mess-eps-spec.xml | 15 +++++++++------ 1 file changed, 9 insertions(+), 6 deletions(-) diff --git a/NumericalData/AMDA/MESSENGER/EPS/mess-eps-spec.xml b/NumericalData/AMDA/MESSENGER/EPS/mess-eps-spec.xml index 319a49e..cd2b901 100644 --- a/NumericalData/AMDA/MESSENGER/EPS/mess-eps-spec.xml +++ b/NumericalData/AMDA/MESSENGER/EPS/mess-eps-spec.xml @@ -32,12 +32,7 @@ PDS MESS-E_V_H_SW-EPPS-3-EPS-DDR-V1.0/EPS_PA_DAILY_SPECTROGRAM spase://CDPP/Instrument/AMDA/MESSENGER/EPS - EnergeticParticles - EPS PDS data products are derivate from the “Shaped” channel on EPS which is an integrated (hardware) channel. - The hardware channel responded to all particles (ion and electron) that are above the threshold (~30 keV). - Our experience at Mercury’s magnetosphere is that the primary particles are mostly energetic electrons. - Please note that the D03 detector on the EPS has a very high background and is not useable for any of these science data products. - + EnergeticParticles 2008-08-20T16:03:35Z @@ -46,12 +41,20 @@ PT120S Mercury + EPS PDS data products are derivate from the “Shaped” channel on EPS which is an integrated (hardware) channel. + The hardware channel responded to all particles (ion and electron) that are above the threshold (~30 keV). + Our experience at Mercury’s magnetosphere is that the primary particles are mostly energetic electrons. + Please note that the D03 detector on the EPS has a very high background and is not useable for any of these science data products. + countrate mes_eps_pad cnts/s + + Spectrogram + 16 -- libgit2 0.21.2