Temporal and Periodic Variation of the MCMESI for the Last Two Solar Cycles; Comparison with the Number of Different Class X-ray Solar Flares
Author:
Funder
TÜBİTAK
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s11207-020-01711-2.pdf
Reference46 articles.
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3. Barlyaeva, T., Wojak, J., Lamy, P., Boclet, B., Toth, I.: 2018, Periodic behaviour of coronal mass ejections, eruptive events, and solar activity proxies during solar cycles 23 and 24. J. Atmos. Solar-Terr. Phys. 177, 12. DOI.
4. Byrne, J.P., Morgan, H., Habbal, S.R., Gallagher, P.T.: 2012, Automatic detection and tracking of Coronal Mass Ejections. II. Multiscale filtering of coronagraph images. Astrophys. J. 752(2), 145. DOI.
5. Chang, C., Glover, G.H.: 2010, Time–frequency dynamics of resting-state brain connectivity measured with fMRI. NeuroImage 50(1), 81. DOI.
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