Figures, animations and code for the paper Möstl et al. 2020 ApJ

Moestl, Christian; Weiss, Andreas; Bailey, Rachel; Reiss, Martin; Amerstorfer, Tanja; Hinterreiter, Jürgen; Bauer, Maike; Mcintosh, Scott W.; Lugaz, Noe; Stansby, David

doi:10.6084/m9.figshare.12563765.v6

1/1

21 files

Figures, animations and code for the paper Möstl et al. 2020 ApJ

Version 6 2020-09-17, 09:23

Version 5 2020-09-02, 09:05

Version 4 2020-08-28, 13:46

Version 3 2020-08-27, 11:12

Version 2 2020-07-28, 09:20

Version 1 2020-07-28, 09:18

journal contribution

posted on 2020-09-17, 09:23 authored by Christian MoestlChristian Moestl, Andreas Weiss, Rachel Bailey, Martin ReissMartin Reiss, Tanja AmerstorferTanja Amerstorfer, Jürgen HinterreiterJürgen Hinterreiter, Maike Bauer, Scott W. Mcintosh, Noe Lugaz, David StansbyDavid Stansby

Figures, animations and code for the paper Möstl et al. 2020 (ApJ): "Prediction of the in situ coronal mass ejection rate for solar cycle 25: Implications for Parker Solar Probe in situ observations"

https://arxiv.org/abs/2007.14743

The source code an also be found on github:

https://github.com/helioforecast/Papers/tree/master/Moestl2020_PSP_rate

Funding

Austrian Science Fund (FWF): P31521-N27

Austrian Science Fund (FWF): P31659-N27

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heliophysics magnetic flux ropes coronal mass ejections ICMEs CMEs parker solar probe Solar Orbiter Space Science Space and Solar Physics

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MIT

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Figures, animations and code for the paper Möstl et al. 2020 ApJ

Funding

Austrian Science Fund (FWF): P31521-N27

Austrian Science Fund (FWF): P31659-N27

History

Usage metrics

Categories

Keywords

Licence

Exports