Tutorials for UVCS/SOHO Data Analysis
UVCS/SOHO data is processed in three major steps:
Spectral Data Files
are read by the UVCS Display and Analysis Software
package, and can be calibrated in wavelength and intensity,
in addition to being
corrected for image distortion, detector flat-field, and dark counts.
Click here for DAS Tutorial
Processed Spectral Data Files
are then corrected to separate instrumental from astronomical sources.
In intensity, disk-scattered stray light and interplanetary emission
In wavelength, instrumental broadening, point spread functions, and
intrinsic quantization errors are removed.
Click here for Profile Curve-fit Tutorial (Updated)
Science Data Files are then analyzed by comparing with results
of theoretical radiative-transfer codes.
This ``empirical modeling'' provides densities, abundances, and
velocity distribution parameters.
Click here for Model Code Tutorial
Created by Raid
Suleiman & Steven Cranmer
Last Modified on 10/17/13