Radial Distributions of Coronal Electron Temperatures: Specificities of the DYN Model
Author:
Funder
Belgian Federal Science Policy Office
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://link.springer.com/content/pdf/10.1007/s11207-021-01814-4.pdf
Reference17 articles.
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2. Antonucci, E., Romoli, M., Andretta, V., Fineschi, S., Heinzel, P., Daniel Moses, , J., et al.: 2019, Metis: the solar orbiter visible light and ultraviolet coronal imager. Astron. Astrophys. DOI.
3. Baumbach, S.: 1937, Strahlung, Ergiebigkeit and Electronendichte der Sonnenkorona. Astron. Nachr. 263, 121.
4. Ebert, R.W., McComas, D.J., Elliott, H.A., Forsyth, R.J., Gosling, J.T.: 2009, Bulk properties of the slow and fast solar wind and interplanetary coronal mass ejections measured by Ulysses: three polar orbits of observations. J. Geophys. Res. 114(A1), A01109. DOI. ADS.
5. Echim, M.M., Lemaire, J., Lie-Svendsen, Ø.: 2011, A review on solar wind modeling: kinetic and fluid aspects. Surv. Geophys. 32(1), 1. DOI. ADS.
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