The relationship between magnetic field strength and loop lengths in solar coronal active regions
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20053619/pdf
Reference21 articles.
1. Three‐dimensional Stereoscopic Analysis of Solar Active Region Loops. II.SOHO/EIT Observations at Temperatures of 1.5–2.5 MK
2. Modeling of Coronal EUV Loops Observed withTRACE. I. Hydrostatic Solutions with Nonuniform Heating
3. The Bragg Crystal Spectrometer for SOLAR-A
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