From 122d1c49b55036b125440de4f00abc8245e9b4b2 Mon Sep 17 00:00:00 2001 From: Elena.Budnik Date: Tue, 15 Mar 2016 16:48:39 +0100 Subject: [PATCH] work --- Instrument/AMDA/STEREO-A/IMPACT/SWEA.xml | 4 ++-- Instrument/AMDA/STEREO-B/IMPACT/SWEA.xml | 4 ++-- NumericalData/AMDA/STEREO-A/SWEA/sta-swea-mom.xml | 26 +++++++++++++------------- NumericalData/AMDA/STEREO-B/SWEA/stb-swea-mom.xml | 26 +++++++++++++------------- 4 files changed, 30 insertions(+), 30 deletions(-) diff --git a/Instrument/AMDA/STEREO-A/IMPACT/SWEA.xml b/Instrument/AMDA/STEREO-A/IMPACT/SWEA.xml index 09560f4..7fc8f6b 100644 --- a/Instrument/AMDA/STEREO-A/IMPACT/SWEA.xml +++ b/Instrument/AMDA/STEREO-A/IMPACT/SWEA.xml @@ -4,8 +4,8 @@ spase://CDPP/Instrument/AMDA/STEREO-A/IMPACT/SWEA - STEREO-A IMPACT/SWEA - STEREO-A IMPACT Solar Wind Plasma Electron Analyzer + SWEA + Solar Wind Plasma Electron Analyzer 2011-12-23T20:14:31Z SWEA is designed to measure the distribution function of the solar wind core and halo electrons from below an eV to several keV, with high spectral and angular resolution over practically the full spherical range. This capability allows the distinction between these components in detail during both undisturbed periods and the passage of CME generated disturbances, when the interplanetary field rotates far out of the ecliptic plane. SWEA consists of a hemispherical top-hat electrostatic analyzer (ESA) that provides a 360 deg. field of view in a plane, combined with electrostatic deflectors to provide nearly 4 pi coverage when SWEA is mounted at the end of the STEREO boom. The inner plate radius is 3.75 cm and the plate separation is 0.28 cm. The resulting energy resolution dE/E is 18%, and the geometric factor is 0.01 cm2 ster E (eV). SWEA compensates for the effects of spacecraft potential on the lowest energy particles by having an outer hemisphere that can be biased according to the plasma density measured by the PLASTIC solar wind ion instrument. Detailed descriptions of the IMPACT SWEA can be found in Space Science Reviews 136, 227-239 (2008). diff --git a/Instrument/AMDA/STEREO-B/IMPACT/SWEA.xml b/Instrument/AMDA/STEREO-B/IMPACT/SWEA.xml index a2909ef..2b8e81d 100644 --- a/Instrument/AMDA/STEREO-B/IMPACT/SWEA.xml +++ b/Instrument/AMDA/STEREO-B/IMPACT/SWEA.xml @@ -4,8 +4,8 @@ spase://CDPP/Instrument/AMDA/STEREO-B/IMPACT/SWEA - STEREO-B IMPACT/SWEA - STEREO-B IMPACT Solar Wind Plasma Electron Analyzer + SWEA + Solar Wind Plasma Electron Analyzer 2011-12-21T00:00:00Z SWEA is designed to measure the distribution function of the solar wind core and halo electrons from below an eV to several keV, with high spectral and angular resolution over practically the full spherical range. This capability allows the distinction between these components in detail during both undisturbed periods and the passage of CME generated disturbances, when the interplanetary field rotates far out of the ecliptic plane. SWEA consists of a hemispherical top-hat electrostatic analyzer (ESA) that provides a 360 deg. field of view in a plane, combined with electrostatic deflectors to provide nearly 4 pi coverage when SWEA is mounted at the end of the STEREO boom. The inner plate radius is 3.75 cm and the plate separation is 0.28 cm. The resulting energy resolution dE/E is 18%, and the geometric factor is 0.01 cm2 ster E (eV). SWEA compensates for the effects of spacecraft potential on the lowest energy particles by having an outer hemisphere that can be biased according to the plasma density measured by the PLASTIC solar wind ion instrument. Detailed descriptions of the IMPACT SWEA can be found in Space Science Reviews 136, 227-239 (2008). diff --git a/NumericalData/AMDA/STEREO-A/SWEA/sta-swea-mom.xml b/NumericalData/AMDA/STEREO-A/SWEA/sta-swea-mom.xml index 48cd041..494e358 100644 --- a/NumericalData/AMDA/STEREO-A/SWEA/sta-swea-mom.xml +++ b/NumericalData/AMDA/STEREO-A/SWEA/sta-swea-mom.xml @@ -4,7 +4,7 @@ spase://CDPP/NumericalData/AMDA/STEREO-A/IMPACT/SWEA/sta-swea-mom - swea-moments E:45-2000eV + electron moments E:45-2000eV 2015-10-14T11:48:00Z @@ -33,7 +33,7 @@ Heliosphere.Remote1AU - Ne + density ne_part_sta phys.density;phys.electron cm-3 @@ -46,7 +46,7 @@ - Te_b + t_b te_part_sta phys.temperature;phys.electron eV @@ -56,17 +56,17 @@ 3 - Te_par + t_para 0 te_part_sta(0) - Te_perp1 + t_perp1 1 te_part_sta(1) - Te_perp2 + t_perp2 2 te_part_sta(2) @@ -77,7 +77,7 @@ - Qe_rtn + Q_rtn qe_part_sta phys.heatflux;phys.electron erg/sec/cm2 @@ -91,17 +91,17 @@ 3 - Qe_R + q_r 0 qe_part_sta(0) - Qe_T + q_t 1 qe_part_sta(1) - Qe_N + q_n 2 qe_part_sta(2) @@ -112,7 +112,7 @@ - Qe_b + Q_b qe_b_sta phys.heatflux;phys.electron erg/sec/cm2 @@ -126,12 +126,12 @@ 2 - Qe_par + q_para 0 qe_b_sta(0) - Qe_perp + q_perp 1 qe_b_sta(1) diff --git a/NumericalData/AMDA/STEREO-B/SWEA/stb-swea-mom.xml b/NumericalData/AMDA/STEREO-B/SWEA/stb-swea-mom.xml index c6913cb..101705e 100644 --- a/NumericalData/AMDA/STEREO-B/SWEA/stb-swea-mom.xml +++ b/NumericalData/AMDA/STEREO-B/SWEA/stb-swea-mom.xml @@ -4,7 +4,7 @@ spase://CDPP/NumericalData/AMDA/STEREO-B/IMPACT/SWEA/stb-swea-mom - swea-moments E:45-2000eV + electron moments E:45-2000eV 2015-10-14T14:42:00Z @@ -33,7 +33,7 @@ Heliosphere.Remote1AU - Ne + density ne_part_stb phys.density;phys.electron cm-3 @@ -46,7 +46,7 @@ - Te_b + t_b te_part_stb phys.temperature;phys.electron eV @@ -56,17 +56,17 @@ 3 - Te_par + t_para 0 te_part_stb(0) - Te_perp1 + t_perp1 1 te_part_stb(1) - Te_perp2 + t_perp2 2 te_part_stb(2) @@ -77,7 +77,7 @@ - Qe_rtn + Q_rtn qe_part_stb phys.heatflux;phys.electron erg/sec/cm2 @@ -91,17 +91,17 @@ 3 - Qe_R + q_r 0 qe_part_stb(0) - Qe_T + q_t 1 qe_part_stb(1) - Qe_N + q_n 2 qe_part_stb(2) @@ -112,7 +112,7 @@ - Qe_b + Q_b qe_b_stb phys.heatflux;phys.electron erg/sec/cm2 @@ -126,12 +126,12 @@ 2 - Qe_par + q_para 0 qe_b_stb(0) - Qe_perp + q_perp 1 qe_b_stb(1) -- libgit2 0.21.2