Parameters of Coronal Dimmings and Their Variations during Solar Cycle 24

Author:

Vakhrusheva A. A.,Shugai Yu. S.,Kaportseva K. B.,Eremeev V. E.,Kalegaev V. V.

Publisher

Pleiades Publishing Ltd

Reference41 articles.

1. Chertok, I.M. and Grechnev, V.V., Large-scale dimmings produced by solar coronal mass ejections according to SOHO/EIT data in four EUV lines, Astron. Rep., 2003a, vol. 47, no. 11, pp. 934–945.

2. Chertok, I.M. and Grechnev, V.V., Manifestations of CME-associated dimmings at four EUV wavelengths of SOHO/EIT, in International Solar Cycle Studies Symposium “Solar Variability as an Input to the Earth’s Environment”, ESA SP-535, Tatranská Lomnica, Slovakia, 2003, Wilson, A., Ed., 2003b.

3. Chertok, I.M. and Grechnev, V.V., Some manifestations of large-scale activity on the solar disk in relation to coronal mass emissions, Soln.-Zemnaya Fiz., 2004, vol. 6, pp. 101–103.

4. Chertok, I.M. and Grechnev, V.V., Large-scale activity in the Bastille Day 2000 solar event, Sol. Phys., 2005, vol. 229, pp. 95–114.

5. Chikunova, G., Dissauer, K., Podladchikova, T., and Veronig, A.M., Coronal dimmings associated with coronal mass ejections on the solar limb, Astrophys. J., 2020, vol. 896, pp. 17–33. https://doi.org/10.3847/1538-4357/ab9105

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