Lags and Hysteresis Loops of Cosmic Ray Intensity Versus Sunspot Numbers: Quantitative Estimates for Cycles 19 – 23 and a Preliminary Indication for Cycle 24-Reference-Cited by-同舟云学术

Lags and Hysteresis Loops of Cosmic Ray Intensity Versus Sunspot Numbers: Quantitative Estimates for Cycles 19 – 23 and a Preliminary Indication for Cycle 24

Published:2014-01-16 Issue:7 Volume:289 Page:2727-2732
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Kane R. P.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s11207-014-0479-9.pdf

Reference21 articles.

1. Belov, A.: 2000, Space Sci. Rev. 93, 79.

2. Burlaga, L.F., McDonald, F.B., Ness, N.F.: 1993, J. Geophys. Res. 98, 1.

3. Burlaga, L.F., McDonald, F.B., Goldstein, M.N., Lazarus, A.J.: 1985, J. Geophys. Res. 90, 12027.

4. Cane, H.V., Wibberenz, G., Richardson, I.G., von Rosenvinge, T.T.: 1999, Geophys. Res. Lett. 26, 565.

5. Dorman, L.I.: 1959, Proc. 6th Int. Cosmic Ray Conf. 4, 328.

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