Prediction of the In Situ Coronal Mass Ejection Rate for Solar Cycle 25: Implications for Parker Solar Probe In Situ Observations

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ADS bibcode
2020AGUFMSH0490001M
year
2020
Listed Authors
Moestl, C.
Weiss, A.
Reiss, M.
Bailey, R.
Amerstorfer, U.
Amerstorfer, T.
Hinterreiter, J.
Bauer, M.
McIntosh, S. W.
Lugaz, N.
Stansby, D.
Listed Institutions
Austrian Academy of Sciences, Vienna, Austria
Institute of Geodesy, Graz University of Technology, Graz, Austria
Space Research Institute, Austrian Academy of Sciences, Vienna, Austria; Institute of Geodesy, Graz University of Technology, Graz, Austria
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Institute of Physics, University of Graz, Graz, Austria; Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Space Research Institute, Austrian Academy of Sciences, Graz, Austria; University of Graz, Institute of Physics, Graz, Austria
High Altitude Observatory, Boulder, CO, United States
University of New Hampshire, Durham, United States

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