Hostname: page-component-848d4c4894-75dct Total loading time: 0 Render date: 2024-04-30T14:49:00.604Z Has data issue: false hasContentIssue false

The solar physics FORWARD codes: Now with widgets!

Published online by Cambridge University Press:  06 January 2014

Blake Forland
Affiliation:
High Altitude Observatory/National Center for Atmospheric Research3080 Center Green Dr. Boulder, CO, 80027, USA email: lyon.bcf@gmail.com, sgibson@ucar.edu Dept of Physics & Metro State College DenverNC 3123 Campus Box 69 1201 5th Street, Denver, CO, 80204-2005, USA email: dove@msudenver.edu
Sarah Gibson
Affiliation:
High Altitude Observatory/National Center for Atmospheric Research3080 Center Green Dr. Boulder, CO, 80027, USA email: lyon.bcf@gmail.com, sgibson@ucar.edu
James Dove
Affiliation:
Dept of Physics & Metro State College DenverNC 3123 Campus Box 69 1201 5th Street, Denver, CO, 80204-2005, USA email: dove@msudenver.edu
Therese Kucera
Affiliation:
NASA Goddard Space Flight Center & Greenbelt, MD20771, USA email: therese.a.kucera@nasa.gov
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have developed a suite of forward-modeling IDL codes (FORWARD) to convert analytic models or simulation data cubes into coronal observables, allowing a direct comparison with observations. Observables such as extreme ultraviolet, soft X-ray, white light, and polarization images from the Coronal Multichannel Polarimeter (CoMP) can be reproduced. The observer's viewpoint is also incorporated in the FORWARD analysis and the codes can output the results in a variety of forms in order to easily create movies, Carrington maps, or simply observable information at a particular point in the plane of the sky. We present a newly developed front end to the FORWARD codes which utilizes IDL widgets to facilitate ease of use by the solar physics community. Our ultimate goal is to provide as useful a tool as possible for a broad range of scientific applications.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013 

References

Bak-Stȩślicka, U., Gibson, S. E., Fan, Y., Bethge, C., Forland, B., & Rachmeler, L. A. 2013, Astrophys. J. in press; Arxiv 1304.7388Google Scholar
Dove, J., Gibson, S., Rachmeler, L. A., Tomczyk, S., & Judge, P. 2011, Astrophys. J., 731, 1CrossRefGoogle Scholar
Gibson, S. E., Kucera, T. A., et al. 2010, Astrophys. J., 723, 1133CrossRefGoogle Scholar
Kucera, T. A., Gibson, S. E., Schmit, D. J., Landi, E., & Tripathi, D. 2012, Astrophys. J., 757, 73Google Scholar
Rachmeler, L. A., Gibson, S. E., Dove, J. B., DeVore, C. R., & Fan, Y. 2013, Solar Phys. in press, Arxiv 1304.7594Google Scholar
Schmit, D. J. & Gibson, S. E. 2011, Astrophys. J., 733, 1CrossRefGoogle Scholar