Long term variation of XBP, their properties, and environments
- Submitted by: Steven Saar, Harvard- Smithsonian Center for Astrophysics
- Authors: S. Saar and J. Schmelz
- Session: Monday afternoon posters.
We use an automated solar region detecting alogrithm to identify X-ray bright points (XBP) and their environments in XRT images. Filter ratios are used to determine approximate average temperatures. We explore how XBP numbers, locations, properties, and environments vary on long timescales.
public/hinode9/schedule/session-02p/v0100.txt · Last modified: 2015/07/30 00:48 (external edit)