Interplanetary rendezvous at a solar wind stream
Author:
Affiliation:
1. CNR–Institute for Plasma Science and Technology, National Research Council, Bari, Italy.
2. KTH Royal Institute of Technology, Stockholm, Sweden.
3. University of Calabria, Rende, Italy.
Abstract
Publisher
American Association for the Advancement of Science (AAAS)
Link
https://www.science.org/doi/pdf/10.1126/science.adr5854
Reference15 articles.
1. Nine Outstanding Questions of Solar Wind Physics
2. In situ observations of large-amplitude Alfvén waves heating and accelerating the solar wind
3. P. Hellinger, L. Matteini, Š. Štverák, P. M. Trávníček, E. Marsch, JGR Space Phys. 116, A09105 (2011).
4. Chromospheric Alfvénic Waves Strong Enough to Power the Solar Wind
5. Interchange reconnection as the source of the fast solar wind within coronal holes
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