Rotation Profiles of Coronal Bright Points Inside and Outside of Coronal Holes
Author:
Funder
Hrvatska Zaklada za Znanost
Horizon 2020 Framework Programme
Austrian-Croatian Bilateral Scientific Projects
Publisher
Springer Science and Business Media LLC
Link
https://link.springer.com/content/pdf/10.1007/s11207-024-02294-y.pdf
Reference71 articles.
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3. Bagashvili, S.R., Shergelashvili, B.M., Japaridze, D.R., Chargeishvili, B.B., Kosovichev, A.G., Kukhianidze, V., Ramishvili, G., Zaqarashvili, T.V., Poedts, S., Khodachenko, M.L., De Causmaecker, P.: 2017, Statistical properties of coronal hole rotation rates: are they linked to the solar interior? Astron. Astrophys. 603, A134. DOI. ADS.
4. Bohlin, J.D.: 1977, Extreme-ultraviolet observations of coronal holes. I: locations, sizes and evolution of coronal holes, June 1973 – January 1974. Solar Phys. 51, 377. DOI. ADS.
5. Brajša, R., Ruždjak, V., Vršnak, B., Wöhl, H., Pohjolainen, S., Urpo, S.: 1999, An estimate of microwave low-brightness-temperature regions’ heights obtained measuring their rotation velocity. Solar Phys. 184, 281. DOI. ADS.
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