REVISION LECTURE I SOLAR PHYSICS PHAS M314/SPCEG012 April 23, 2012 1.
Basic principle of medical dermatology: "If it's dry, wet it ...
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HMI OBSERVATIONS OF TRANSIENT PHENOMENA Juan Carlos Martínez Oliveros Space Sciences Laboratory, UC Berkeley Charles Lindsey, Hugh Hudson, S. Couvidat,
Cosmic Ray Intensity Variation and Its Connection with the Total and Spectral Solar Irradiance Gigolashvili Marina, Kapanadze Natela Georgian National.
1 Nuclear reactions in the Sun A first look at the SunA first look at the Sun A deeper look: helioseismologyA deeper look: helioseismology Neutrino: the.
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Turbulent Origins of the Sun’s Corona & Solar WindS. R. Cranmer, September 22, 2011, B.U. CSP Turbulent Origins of the Sun’s Hot Corona and the Solar Wind.
Exploring the Solar Wind with Ultraviolet Light Steven R. Cranmer and the UVCS/SOHO Team Harvard-Smithsonian Center for Astrophysics.
Active Region Flux Dispersal (SH13A-1518) B.T. Welsch & Y.Li Space Sciences Lab, UC-Berkeley The ultimate fate of the magnetic flux introduced into the.
1.B – Solar Dynamo 1.C – Global Circulation 1.D – Irradiance Sources 1.H – Far-side Imaging 1.F – Solar Subsurface Weather 1.E – Coronal Magnetic Field.
Understanding the Connection Between Magnetic Fields in the Solar Interior and Magnetic Activity in the Corona W.P. Abbett and G.H. Fisher, B.T. Welsch,