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projects/maven/swia/

mvn_swia_protonalphamoms_mag.pro


PROCEDURE: MVN_SWIA_PROTONALPHAMOMS_MAG PURPOSE: Routine to compute approximately the proton and alpha moments from fine distributions. Does not work if distribution is too hot and they overlap. Modified from 'mvn_swia_protonalphamoms' to compute in magnetic field coords. AUTHOR: Jasper Halekas CALLING SEQUENCE: MVN_SWIA_PROTONALPHAMOMS_MAG, TRANGE = TRANGE INPUTS: KEYWORDS: TRANGE: Time Range to Compute Moments ARCHIVE: Use Archive data instead of Survey (default) $LastChangedBy: jhalekas $ $LastChangedDate: 2014-11-04 06:30:10 -0800 (Tue, 04 Nov 2014) $ $LastChangedRevision: 16131 $ $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/projects/maven/swia/mvn_swia_protonalphamoms_mag.pro $

Routines

Routines from mvn_swia_protonalphamoms_mag.pro

mvn_swia_protonalphamom_mag, n1, t1, v1, n2, t2, v2, dat=dat, plot=plot, archive=archive
mvn_swia_protonalphamoms_mag, archive=archive, trange=trange

Routine details

top source mvn_swia_protonalphamom_mag

mvn_swia_protonalphamom_mag, n1, t1, v1, n2, t2, v2, dat=dat, plot=plot, archive=archive

Parameters

n1
t1
v1
n2
t2
v2

Keywords

dat
plot
archive

top source mvn_swia_protonalphamoms_mag

mvn_swia_protonalphamoms_mag, archive=archive, trange=trange

Keywords

archive
trange

File attributes

Modification date: Fri Nov 21 06:43:13 2014
Lines: 74
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