'Open flux' presentation slideshows

Reconstruction of solar magnetic field since 1700 onwards

????? 2 ?. Reconstruction of solar magnetic field since 1700 onwards. ? ?. In collaboration with Robert Cameron, Dieter Schmitt and Manfred Schuessler. Free parameter. Complements of Talk 1. Initial condition. e-folding time of approximately 4000 years. Decay time:.

559 views • 41 slides

Mike Lockwood (Space Science and Technology Department, STFC Rutherford Appleton Laboratory

The Space Environment in the Inner Heliosphere. Mike Lockwood (Space Science and Technology Department, STFC Rutherford Appleton Laboratory & Southampton University) 4 th European Space Weather Week, 9 th November 2007. ROUGH GUIDES. THE ROUGH GUIDE to. The Moon & Mars.

487 views • 25 slides

194 views • 19 slides

The Rise of Solar Cycle 24: Magnetic Fields from the Dynamo through the Photosphere and Corona and Connecting to the Heliosphere Part 2: Corona & Heliophere.

176 views • 17 slides

Comments on Reconnection at the Sun

Comments on Reconnection at the Sun. L. A. Fisk University of Michigan. Footpoint Motions on the Solar Surface. Three-Dimensional Perspective. Questions Asked. What kind of values are expected for the spatial scales of reconnection events and the time scales for the reconnection?

213 views • 13 slides

The Rise of Solar Cycle 24: Magnetic Fields from the

The Rise of Solar Cycle 24: Magnetic Fields from the Dynamo to through the Photosphere and Corona and Connecting to the Heliosphere Wed-Thur Jul 13-14 Conveners: Joan Burkepile, Giuliana de Toma, Juan Fontenla, and Chuck Smith

63 views • 6 slides