Cosmic ray solar semidiurnal anisotropy 1. Treatment of experimental data

Physics – Plasma Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

15

Interplanetary Physics: Cosmic Rays, Interplanetary Physics: Interplanetary Magnetic Fields, Interplanetary Physics: Instruments And Techniques, Space Plasma Physics: Charged Particle Motion And Acceleration

Scientific paper

We have analyzed data obtained with 39 globally distributed detectors, with median primary rigidity of response (Rm) in the range: 10 GV<=Rm<=330 GV, for the period 1953 to 1992. The time interval covers several epochs of solar activity maxima, minima, and polar field reversals. Data are sparse for earlier period but adequate after 1970. We have investigated long-term changes in the parameters applicable to the annual mean solar semidiurnal variation. We show that its dependence on the median asymptotic latitude of viewing (λm) is given by cos2λm. The data are consistent with a double power law fit in rigidity for the entire period of our study. The power law exponents are given by γ1=0.7+/-0.3 (if R<=Rp) and γ2=-0.4+/-0.2 (if R>Rp), where Rp is the peak primary rigidity. The values of Rp near maximum for even solar activity cycles (20,22) are quite large (~125 GV) compared to other periods. These large values lie close to the epochs of magnetic polarity reversals from negative (qA<0) to positive (qA>0) in the northern hemisphere of Sun. During these times, the exponent γ2 acquires large negative values. Near solar activity minima, the values Rp are among the lowest at about 40 GV. We have also computed the mean limiting primary rigidity (Rc) for each year. The values of Rc lie close to 50 GV for solar activity minima and near 100 GV for maxima. In other words, the values of Rc are very close to those of Rp. Moreover, the correspondence between them is good. Both exhibit solar as well as Hale cycle variations.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Cosmic ray solar semidiurnal anisotropy 1. Treatment of experimental data 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 Cosmic ray solar semidiurnal anisotropy 1. Treatment of experimental data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmic ray solar semidiurnal anisotropy 1. Treatment of experimental data will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1418654

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.