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The Solar Wind Quasi-Invariant Observed by STEREO A and B at Solar Minimum 2007 and Comparison with Two Other Minima |
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| Authors: | Leitner M Farrugia C J Galvin A Simunac K D C Biernat H K Osherovich V A |
| Institution: | 1.Institute of Astro- and Particle Physics, University of Innsbruck, Technikerstrasse 25/8, 6020, Innsbruck, Austria ;2.Space Science Center and Department of Physics, University of New Hampshire, Durham, NH, USA ;3.Space Research Institute, Austrian Academy of Sciences, Graz, Austria ;4.NASA Goddard Space Flight Center, Greenbelt, MD, USA ; |
| Abstract: | Solar Physics - The solar wind quasi-invariant (QI) is defined as the ratio of the solar wind magnetic energy density to the plasma kinetic energy density (i.e., the inverse square of the... |
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