The Spectral Correlation Function Home Page


This page contains the details and the results from the Spectral Correlation Function (SCF) and its analysis of position-position-velocity data cubes. The SCF is a diagnostic tool which scans these data cubes quantifying the similarities and differences between neighboring spectra in the cubes. We intend to use this information to probe the structure of molecular clouds in the interstellar medium (ISM).

On this page, there are two types of data cubes analyzed. First, observed cubes have been made of several physical objects through radio observations. In addition, theoretical work in MHD simulations has resulted in simulations of the ISM. These simulations can also be used to produce data cubes. Both of these types of data cubes have been analyzed using the SCF algorithm. Maps of the correlation are generated as well as histograms of the values of the SCF results. We present both of these types of data here for your exploration and analysis.

The SCF algorithm is written for IDL 4.0.1 and is compatible with IDL 5.0.x, (though not optimized). The source is available in tar format as well as text documents.


SCF Web Resources


Summary of SCF Results

Several data cubes have been analyzed using the SCF routines and the current results are available here.


If you have questions or comments about the SCF project or would like to submit data for analysis by the SCF algorithm, please contact agoodman@cfa.harvard.edu or erosolowsky@cfa.harvard.edu.