MHD Modeling Support for HMI Jon A. Linker Predictive Science, Inc. (PSI[removed]Mesa Rim Rd, Suite 170 San Diego, CA 92121, USA

First Page		Document Content
Date: 2009-09-30 14:38:59 Astrophysics Physics Astronomy Light sources Corona Space telescopes Solar wind STEREO Coronal loop Space plasmas Plasma physics Sun		MHD Modeling Support for HMI Jon A. Linker Predictive Science, Inc. (PSI[removed]Mesa Rim Rd, Suite 170 San Diego, CA 92121, USA Add to Reading List Source URL: hmi.stanford.edu Download Document from Source Website File Size: 2,60 MB Share Document on Facebook

	Astronomy & Astrophysics manuscript no. lp˙ref1˙v2 (DOI: will be inserted by hand later) April 29, 2005 Electron density along a coronal loop observed with CDS/SOHO DocID: 1o79B - View Document
	Modeling a coronal loop heated by MHD-turbulence nanoflares F. Reale1 , G. Nigro2 , F. Malara2 , G. Peres1 , P. Veltri2 ABSTRACT We model the hydrodynamic evolution of the plasma confined in a coronal loop, 30000 km long DocID: 1mNb8 - View Document
	Solar Physics DOI: /•••••-•••-•••-••••-• A Rapid, Manual Method to Map Coronal-Loop Structures of an Active Region Using Cubic B´ ezier DocID: 1mDpz - View Document
	Matthew Brookhart – Coaxial Current Injection Vθ Coronal Loop, Anchored in Turbulent Photosphere Jz DocID: 1jAuI - View Document
	The Astrophysical Journal, 685:1262Y 1269, 2008 October 1 # 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A. PLASMA FLOWS GUIDED BY STRONG MAGNETIC FIELDS IN THE SOLAR CORONA Eckart Marsch DocID: 196VA - View Document