PROCEDURE: thm_part_energy_interpolate PURPOSE: Interpolate particle data by energy between sst & esa distributions using a weighted curve fitting routine. INPUTS: dist_sst: SST particle distribution structure in flux dist_esa: ESA particle distribution structure in flux energies: The set of target energies to interpolated the SST to. OUTPUTS: Replaces dist_sst with the interpolated data set KEYWORDS: error: Set to 1 on error, zero otherwise NOTES: #1 The number of time samples and the times of those samples must be the same for dist_sst & dist_esa (use thm_part_time_interpolate.pro) #2 The number of angles and the angles of each sample must be the same for dist_sst & dist_esa (use thm_part_sphere_interp.pro) SEE ALSO: thm_part_dist_array thm_part_smooth thm_part_subtract, thm_part_omni_convert thm_part_time_interpolate.pro thm_part_sphere_interp.pro $LastChangedBy: pcruce $ $LastChangedDate: 2013-09-26 16:32:05 -0700 (Thu, 26 Sep 2013) $ $LastChangedRevision: 13156 $ $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/thmsoc/trunk/idl/themis/spacecraft/particles/thm_part_energy_interpolate.pro $