UCL DEPARTMENT OF SPACE & CLIMATE PHYSICS SPACE PLASMA PHYSICS GROUP A Potential Mission Concept for the M3 2022 Launch: Investigation of MagnetoPause.
The Photosphere & CME Initiation “We would like us to give us your views on the application of vector field and photospheric flows data to the CME initiation.
The Independency of Stellar Mass-Loss Rates on Stellar X-ray Luminosity and Activity
An Introduction to the NIMROD Fusion Magnetohydrodynamics Simulation Project Prof. Carl Sovinec Department of Engineering Physics University of Wisconsin-Madison.
195 Å image – behind 195 Å image – Sun- Earth line – SOHO/ EIT image 195 Å image – Sun- Earth line – SOHO/ EIT image 195 Å image – ahead SECCHI Extreme.
195 Å image – behind
The Rise of Solar Cycle 24: Magnetic Fields from the Dynamo through the Photosphere and Corona and Connecting to the Heliosphere Part 1: Interior and Photosphere.
1 Heliospheric Magnetic Field 1835-2010 Leif Svalgaard Stanford University, CA [email protected] .
New STEREO/SECCHI Processing for Heliospheric Transients
