PROCEDURE: swe_maxbol PURPOSE: Maxwell-Boltzmann distribution for fitting SWEA electron energy spectra. The reference frame is at the instrument aperture, after the electrons have been accelerated by the spacecraft potential. Correction for spacecraft potential, but no correction for bulk flow. Units are energy flux [eV/cm2-sec-ster-eV]. USAGE: eflux = swe_maxbol(E, par=p) INPUTS: E: Measured energy [eV]. KEYWORDS: PARAM: Parameter structure. p = {n : 1.0d , $ ; core density [cm-3] T : 10.0d , $ ; core temperature [eV] k_n : 0.0d , $ ; halo density [cm-3] k_vh : 4000.0d , $ k_k : 5.0d , $ pot : 0.0d } ; spacecraft potential [V] $LastChangedBy: dmitchell $ $LastChangedDate: 2014-09-22 09:25:06 -0700 (Mon, 22 Sep 2014) $ $LastChangedRevision: 15831 $ $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/projects/maven/swea/swe_maxbol.pro $ CREATED BY: David L. Mitchell 03-29-13 FILE: swe_maxbol.pro