Abstract
There are two types of high-speed solar wind streams classified in two categories:coronal-hole and solar-flare-generated streams. These two types are classified in two categories considering the bulk speed, proton density, temperature and magnetic field in the interplanetary medium. Their effects on cosmic ray intensity have been studied on a short-term basis during 1980–1986. Daily means of one middle and one low-latitude set of neutron monitor data have been taken for analysis using the Chree method of superposed epochs. The investigation indicates that the solar-flare-generated high-speed solar wind streams are more effective in producing cosmic ray decreases than are the coronal-hole generated streams.
Similar content being viewed by others
References
Hundhausen, A. J.: 1979,Rev. Geophys. Space Phys. 17, 2032.
Iucci, N., Parisi, M., Storini, M., and Villoresi, G.: 1979,Nuovo Cimento 2c, 421.
King, J.: 1983,Interplanetary Medium Data Book - Supplement 2, 1978–1982, NSSCD/WDC-A, Goddard Space Flight Centre, Greenbelt, MA.
King, J.: 1986a,Interplanetary Medium Data Book - Supplement 3, NSSD/WDC-A, Goddard Space Flight Centre, Greenbelt, MA.
King, J.: 1986b,Interplanetary Medium Data Book - Supplement 3A, 1977–1985, NSSCD/WDC-A, Goddard Space Flight Centre Greenbelt, MA.
King, J.: 1989,Interplanetary Medium Data Book - Supplement 4, 1985–1988, NSSCD/WDC-A, Goddard Space Flight Centre, Greenbelt, MA.
Lockwood, J. A. and Webber, W. R.: 1984,J. Geophys. Res. 89, 17.
Lockwood, J. A., Webber, W. R., and Debrunner, H.: 1991,J. Geophys. Res. 96, 11587.
Mavromichalaki, H., Vassilaki, A., and Marmatsouri, E.: 1988,Solar Phys. 115, 345.
Munakata, Y., Mori. S., Ryu, J. Y., Agrawal S. P., and Venkatesan, D.: 1987,Proc. 20th Int. Cosmic Ray Conf. 4, 39.
Mishra, B. L., Shrivastava, P. K., and Agrawal, S. P.: 1990,Proc. 21st Int. Cosmic Ray Conf. 6, 299.
Sreenivasan, S. R. and Johnson, R. H.: 1968,Can. J. Phys. 46, S954.
Shrivastava, P. K.: 1990,Proc. 21st Int. Cosmic Ray Conf. 6, 65.
Shrivastava, P. K. and Agrawal, S. P.: 1990,Proc. Basic Plasma Processes on the Sun, Kluwer Academy Press, Holland, p. 259.
Shrivastava, P. K. and Shukla, R. P.: 1993,Proc. 23rd Int. Cosmic Ray Conf. 3, 489.
Venkatesan, D., Shukla, A. K., and Agrawal, S. P.: 1982,Solar Phys. 120, 145.
Zirker, J. B.: 1977,Rev. Geophys. Space Phys. 15, 247.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Shrivastava, P.K., Shukla, R.P. High-speed solar wind streams of two different origins and cosmic-ray variations during 1980–1986. Sol Phys 154, 177–185 (1994). https://doi.org/10.1007/BF00676782
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00676782