Nonlinear effects on torsional Alfven waves S. Vasheghani Farahani, V.M. Nakariakov, T. Van Doorsselaere, E. Verwichte.
1 Searching for Alfvén Waves John Yoritomo The Catholic University of America Mentor: Dr. Adriaan van Ballegooijen The Smithsonian Astrophysical Observatory.
I. INTRODUCTION Gas Pressure Magnetic Tension Coronal loops are thin and bright structure of hot plasma emitting intense radiation in X-ray and EUV. (1)
Journal Club Paper Reviewing By Tung-Shin Hsu UCLA, October 27, 2010
MAGNETIC TWIST OF EUV CORONAL LOOPS OBSERVED BY TRACE RyunYoung Kwon, Jongchul Chae Astronomy Program, School of Earth and Environmental Science Seoul.
