Dependence of the height of the E-layer on solar activity

Details Dependence of the height of the E-layer on solar activity Dependence of the height of the E-layer on solar activity

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ge%26ae..32..138a&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 32, no. 4, p. 138-141.

Computer Science

Sound

E Region, Earth Ionosphere, Incoherent Scattering, Rocket Sounding, Solar Activity Effects, Geomagnetism, Ion Recombination, Molecular Ions, Solar Cycles, Space Plasmas

Scientific paper

Variations of hmE, the height of the E-layer maximum, with solar activity were investigated on the basis of rocket sounding data. Data from the Kharkov incoherent scattering station indicate that periods of low and high solar activity are characterized by a small monotonic decrease in hmE, while a more abrupt decrease in hmE occurs in the case of intermediate activity, F = 140-180.

Affiliated with

Also associated with

No associations

Rating

Dependence of the height of the E-layer on solar activity 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 Dependence of the height of the E-layer on solar activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dependence of the height of the E-layer on solar activity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1166758