Short and long-term variations in the cosmic ray intensity and their connection with the 5303 Å coronal line intensity in solar cycle No. 20

Author:

Iucci N.,Parisi M.,Villoresi G.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference24 articles.

1. Bachelet, F., Iucci, N., Parisi, M., and Villoresi, G.: 1971, ‘Revised Daily Data 1957–1965 for 65 Cosmic Ray Neutron Monitors, LPS-71–7’, Laboratorio Plasma nello Spazio del C.N.R., Roma.

2. Bachelet, F., Iucci, N., Villoresi, G., and Sporre, B.: 1972a, Nuovo Cimento 7B, 17.

3. Bachelet, F., Iucci, N., and Villoresi, G.: 1972b, Nuovo Cimento 7B, 45.

4. Burger, J. J. and Swanenburg, B. N.: 1972, ‘Energy Dependent Time Lag in the Long-Term Modulation of Cosmic Rays’, preprint.

5. Carmichael, H. and Katzman, J.: 1971, Proc. Inter. Conf. Cosmic Rays, Hobart 7, 2675.

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