Microsoft PowerPoint - Flares - Solar flare - Document - PDFSEARCH.IO

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Date: 2010-12-14 17:05:32 Astrophysics Light sources Sun Astronomy Corona Solar flare Magnetic reconnection Photosphere Convection zone Plasma physics Space plasmas Physics		Microsoft PowerPoint - Flares&CMEs.ppt Add to Reading List Source URL: www.heliophysics.ucar.edu Download Document from Source Website File Size: 1,70 MB Share Document on Facebook

	Sunspots Overhead – Worksheet to follow the viewing of the demonstration movie at http://astro.unl.edu/video/demonstrationvideos Background -647702927350The continuous (blackbody) spectra produced by the photosphere o DocID: 1u7Pf - View Document
	[Voice of Troy Cline] The core of our sun has a temerapture 15.7 million degrees Kelvin. However, the solar surface of the p photosphere is only 5,770 degrees Kelvin. But then something very interesting happens. The temp DocID: 1o50R - View Document
	Title: Horizontal plasma motion in the solar photosphere Author: Michal Švanda Department: Astronomical Institute of Charles University Supervisor: Ing. Miroslav Klvaňa, CSc., Astronomical institute AS CR Ondřejov Sup DocID: 1nGEG - View Document
	DYNAMICS OF MOTIONS IN THE QUIET PHOTOSPHERE M. Švanda(1), M. Klvaňa(2), M. Sobotka(2), V. Bumba(2), (1) Faculty of Mathematics and Physics, Charles University in Prague, Czech Republic, (2) DocID: 1nbIf - View Document
	Vector Spectromagnetograph 1. Introduction The Vector Spectromagnetograph (VSM) is responsible for taking high-quality magnetic field observations in the photosphere and the chromosphere by recording the Zeeman-induced p DocID: 1n8zc - View Document