Characteristics of Forbush effects in recurrent high-velocity streams of the solar wind.

Details Characteristics of Forbush effects in recurrent high-velocity streams of the solar wind. Characteristics of Forbush effects in recurrent high-velocity streams of the solar wind.

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..753k&link_type=abstract

Geomagn. Aeron., Vol. 30, No. 6, p. 753 - 754

Physics

Forbush Effect: Cosmic Rays, Forbush Effect: Solar Wind

Scientific paper

The variation of the exponent of the rigidity spectrum of galactic cosmic rays inside high-velocity streams of the solar wind is discussed. It is shown that the exponent of the spectrum as the Earth is immersed in a high-velocity stream reaches its minimum at the time of maximum velocity, and then a smooth recovery of the value of the exponent γ to a value characteristic of undisturbed conditions occurs.

Affiliated with

Also associated with

No associations

Rating

Characteristics of Forbush effects in recurrent high-velocity streams of the solar wind. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Characteristics of Forbush effects in recurrent high-velocity streams of the solar wind., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Characteristics of Forbush effects in recurrent high-velocity streams of the solar wind. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-985487