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NASA NTRS · 20170008503

Introduction of the ASGARD Code

Abstract

ASGARD 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).

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BibTeXRIS

Bethge, Christian, Winebarger, Amy, Tiwari, Sanjiv, Fayock, Brian. 2017-08-21. Introduction of the ASGARD Code. https://ntrs.nasa.gov/citations/20170008503

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