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

The Parker Solar Probe (PSP) and Solar Orbiter missions are designed to make groundbreaking observations of the Sun and interplanetary space within this decade. We show that a particularly interesting in situ observation of an interplanetary coronal mass ejection (ICME) by PSP may arise during close...

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Bibliographic Details
Published in:The Astrophysical journal 2020-11, Vol.903 (2), p.92
Main Authors: Möstl, Christian, Weiss, Andreas J., Bailey, Rachel L., Reiss, Martin A., Amerstorfer, Tanja, Hinterreiter, Jürgen, Bauer, Maike, McIntosh, Scott W., Lugaz, Noé, Stansby, David
Format: Article
Language:English
Subjects:
Astrophysics
Corona
Coronal mass ejection
Ejecta
Equator
Fluctuations
Flyby missions
Interplanetary magnetic fields
Interplanetary space
Magnetic fields
Magnetic flux
Mathematical models
Solar corona
Solar coronal mass ejections
Solar cycle
Solar magnetic fields
Solar Orbiter (ESA)
Solar orbits
Solar physics
Solar probes
Solar storm
Solar system
Solar wind
Space missions
Space weather
Sunspot numbers
Sunspots
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Summary:The Parker Solar Probe (PSP) and Solar Orbiter missions are designed to make groundbreaking observations of the Sun and interplanetary space within this decade. We show that a particularly interesting in situ observation of an interplanetary coronal mass ejection (ICME) by PSP may arise during close solar flybys (
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/abb9a1