Computer Science
Scientific paper
Mar 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sosyr..39..157v&link_type=abstract
Solar System Research, Volume 39, Issue 2, pp.157-162
Computer Science
Scientific paper
Long-term data on the evolution of the parameters of motion of 15 artificial satellites of the Earth in orbits with minimal heights of 400 1100 km were used to study the density variations in the upper atmosphere at minimums of four cycles of solar activity. It was found that the density at these heights considered increased by about 7% at the minimum of solar cycle 20 as compared to solar cycle 19. Later, the density fell rather linearly at the minimums of cycles 21 and 22. The statistical processing of the data for solar cycles 20 22 demonstrated that the density decreased by 4.6% over ten years and by 9.9% over 20 years. Analyzing the density variations during the four cycles of solar activity, we found that the long-term decrease in density observed at the minimums of cycles 20 22 is caused mainly by specific variations of the solar activity parameters (namely, the solar radio flux and the level of geomagnetic disturbance).
Suevalov V. V.
Volkov I. I.
No associations
LandOfFree
Estimation of long-term density variations in the upper atmosphere of the earth at minimums of solar activity from evolution of the orbital parameters of the earth's artificial satellites 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 Estimation of long-term density variations in the upper atmosphere of the earth at minimums of solar activity from evolution of the orbital parameters of the earth's artificial satellites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Estimation of long-term density variations in the upper atmosphere of the earth at minimums of solar activity from evolution of the orbital parameters of the earth's artificial satellites will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1568522