Spectroscopy -- Second Steps

 

                                   

Linhui Sui,  Astrid Veronig,  Brian Dennis,  Richard Schwartz


 

Topics*:

bullet Analyzing a Flare with Different Attenuator States.
bullet Selecting Multiple Analysis Intervals.
bullet Changing Fitting Models.
bullet Saving and Restoring the Fitting Parameters and Spectral Data.
bullet Plotting the Fitted Spectra Outside SPEX.
bullet Making a Movie of the Spectra.
bullet Choosing and Evaluating a Background Model.
bullet Creating and Customizing Postscript Plots within SPEX.
bullet Using RHESSI Data of a Different Orbit for Background Subtraction.



 

*: Throughout this tutorial, the X4.8 flare July 23 2002 and the M1.5 flare on June 1 2002 are used as examples to explain the topics. Words in fixed font represent SPEX commands.

 

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Responsible NASA Official:
 Brian Dennis
Web Design:
Merrick Berg
Solar Physics Laboratory, Goddard Space Flight Center
Space Science Laboratory, University of California Berkeley
  		Responsible Berkeley Official:
 Hugh Hudson
Systems Admin:
Jon Loran

This page last updated: June 27, 2011