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Introduction of the ASGARD CodeASGARD stands for 'Automated Selection and Grouping of events in AIA Regional Data'. The code is a refinement of the event detection method in Ugarte-Urra & Warren (2014). It is intended to automatically detect and group brightenings ('events') in the AIA EUV channels, to record event parameters, and to find related events over multiple channels. Ultimately, the goal is to automatically determine heating and cooling timescales in the corona and to significantly increase statistics in this respect. The code is written in IDL and requires the SolarSoft library. It is parallelized and can run with multiple CPUs. Input files are regions of interest (ROIs) in time series of AIA images from the JSOC cutout service (http://jsoc.stanford.edu/ajax/exportdata.html). The ROIs need to be tracked, co-registered, and limited in time (typically 12 hours).
Document ID
20170008503
Acquisition Source
Marshall Space Flight Center
Document Type
Presentation
Authors
Bethge, Christian
(Universities Space Research Association Huntsville, AL, United States)
Winebarger, Amy
(NASA Marshall Space Flight Center Huntsville, AL United States)
Tiwari, Sanjiv
(Bay Area Environmental Research Inst. Huntsville, AL, United States)
Fayock, Brian
(Raytheon Co. Huntsville, AL, United States)
Date Acquired
September 5, 2017
Publication Date
August 21, 2017
Subject Category
Solar Physics
Computer Programming And Software
Report/Patent Number
MSFC-E-DAA-TN45899
Meeting Information
Meeting: Meeting Solar Physics Division
Location: Portland, OR
Country: United States
Start Date: August 21, 2017
End Date: August 25, 2017
Sponsors: American Astronomical Society
Funding Number(s)
CONTRACT_GRANT: NNM13AA43C
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
Code development
Corona
Solar
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