Origin of Solar Rotational Periodicity and Harmonics Identified in the Interplanetary Magnetic Field B z $B_{z}$ Component Near the Earth During Solar Cycles 23 and 24-Reference-Cited by-同舟云学术

Origin of Solar Rotational Periodicity and Harmonics Identified in the Interplanetary Magnetic Field B z $B_{z}$ Component Near the Earth During Solar Cycles 23 and 24

Published:2019-04 Issue:4 Volume:294 Page:
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Choi Kyung-Eun,Lee Dae-Young^ORCID

Funder

National Research Foundation of Korea

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s11207-019-1433-7.pdf

Reference42 articles.

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3. Chowdhury, P., Choudhary, D.P., Gosain, S., Moon, Y.-J.: 2014, Short-term periodicities in interplanetary, geomagnetic and solar phenomena during Solar Cycle 24. Astrophys. Space Sci. 356, 7. DOI .

4. Crooker, N.U., Lazarus, A.J., Phillips, J.L., Steinberg, J.T., Szabo, A., Lepping, R.P., Smith, E.J.: 1997, Coronal streamer belt asymmetries and seasonal solar wind variations deduced from Wind and Ulysses data. J. Geophys. Res. 102, 4673. DOI .

5. Echer, E., Svalgaard, L.: 2004, Asymmetry in the Rosenberg–Coleman effect around solar minimum revealed by wavelet analysis of the interplanetary magnetic field polarity data (1927 – 2002). Geophys. Res. Lett. 31, 12. DOI .

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