The structure of the daytime equatorial ionosphere

Details The structure of the daytime equatorial ionosphere The structure of the daytime equatorial ionosphere

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22...28d&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 22, Jan.-Feb. 1982, p. 28-32. In Russian.

Other

Equatorial Atmosphere, Ionospheric Electron Density, Ionospheric Ion Density, Space Plasmas, Vertical Distribution, Charged Particles, Daytime, Particle Energy, Solar Activity Effects

Scientific paper

An analytic solution of the ionospheric-plasma equations is used to obtain the vertical distribution of charged-particle density and temperature above the magnetic equator at heights of 100-2000 km at midday hours for quiet geomagnetic conditions and various levels of solar activity. It is shown that the calculated vertical electron-temperature profiles have a maximum at 250 km, while the isothermal region (T sub e = T sub n) is situated in the 380-500 km region at low solar activity and in the 380-650 km region at high solar activity. The nonisothermicity of the medium does not produce changes in hmF2 and NmF2 but produces an increase in O(+) concentration above the isothermal region and a decrease in H(+) concentration in a wide range of heights.

Affiliated with

Also associated with

No associations

Rating

The structure of the daytime equatorial ionosphere 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 The structure of the daytime equatorial ionosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The structure of the daytime equatorial ionosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1647383