Comprehensive Analysis of the Formation of a Shock Wave Associated with a Coronal Mass Ejection
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/871/i=2/a=212/pdf
Reference56 articles.
1. Automated Temperature and Emission Measure Analysis of Coronal Loops and Active Regions Observed with the Atmospheric Imaging Assembly on the Solar Dynamics Observatory (SDO/AIA)
2. PLASMA PHYSICAL PARAMETERS ALONG CME-DRIVEN SHOCKS. II. OBSERVATION–SIMULATION COMPARISON
3. FIRST COMPLETE DETERMINATION OF PLASMA PHYSICAL PARAMETERS ACROSS A CORONAL MASS EJECTION-DRIVEN SHOCK
4. IDENTIFICATION OF SUPER- AND SUBCRITICAL REGIONS IN SHOCKS DRIVEN BY CORONAL MASS EJECTIONS
5. Super- and sub-critical regions in shocks driven by radio-loud and radio-quiet CMEs
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