Flux of low-energy electrons below 30 KM

Details Flux of low-energy electrons below 30 KM Flux of low-energy electrons below 30 KM

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..129a&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Jan.-Feb. 1985, p. 129-131. In Russian.

Computer Science

Sound

Atmospheric Radiation, Balloon Sounding, Electron Flux Density, Galactic Cosmic Rays, Secondary Emission, Electron Energy, Radiosondes, Secondary Cosmic Rays

Scientific paper

Fluxes of electrons with energies above 20 keV but below 1 MeV were measured at altitudes below 30 km in the atmosphere using balloon radiosondes over Rylsk, USSR in August 1976. The energy of secondary particles (electrons) with an energy of 20-40 keV at heights of 20-30 km was determined to be 5 x 10 to the 9th eV/sq cm s, which exceeds by more than a factor of 2 the energy of the galactic-cosmic-ray flux arriving at the boundary of the atmosphere.

Affiliated with

Also associated with

No associations

Rating

Flux of low-energy electrons below 30 KM 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 Flux of low-energy electrons below 30 KM, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Flux of low-energy electrons below 30 KM will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1591681