Search for the Exit: Voyager 1 at Heliosphere’s Border with the Galaxy.
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Relating the Sub-Parker Spiral Structure of the Heliospheric Magnetic Field to the Dynamic Sources of Solar Wind N. A. Schwadron Southwest Research Institute.
The Solar Orbiter Mission
CSI 769 Fall 2010 Jie Zhang
2.7.2010GONG 2010 – SoHO 24 Aix-en-Provence The Solar Orbiter Mission Max-Planck-Institut für Sonnensystemforschung Achim Gandorfer.
Solar Cycle Variation of the Heliospheric Magnetic Flux, Solar Wind Flux and Galactic Cosmic Rays Charles W. Smith, Nathan A. Schwadron Ken G. McCracken,
1 Abramenko V.I., 1 Yurchyshyn, V., 2 Linker, J., 2 Mikic, Z.
S. T. Wu 1,2 , A. H. Wang 1 , Yang Liu 3 , and Todd Hoeksema 3
An overview of the cycle variations in the solar corona
1. Background2. Flux variation3. Polarity reversal4. Electron evolution5. Conclusions The role of coronal mass ejections in the solar cycle evolution of.
Solar Astronomy: Science in Service to Education Kelly Beck (Haas Center for Public Service, Stanford), Deborah Scherrer (Stanford Solar Center, Stanford),