Super-Active Regions and Production of Major Solar Flares,
Abstract
The success of imaging detectors with small fields of view such as HXIS or the Pinhole/Occulter Facility (P/OF) depends strongly on the ability to point the right place at the right time. During solar maximum years many active regions coexist on the solar disk. Therefore, in order the imaging detector to the right plane, it is important to know which active region is most likely to produce major flares. This knowledge is also important for flare prediction.
Document Details
- Document Type
- Technical Report
- Publication Date
- Oct 01, 1985
- Accession Number
- ADA163104
Entities
People
- Taeil Bai
Organizations
- Stanford University