Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1972
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..17..409s&link_type=abstract
Astrophysics and Space Science, Volume 17, Issue 2, pp.409-425
Astronomy and Astrophysics
Astrophysics
7
Scientific paper
The electron production rates in the night-time D-region arising from the transit of strong celestial X-ray sources Sco X-1, Tau X-1 and Galactic Center are estimated and compared with the ambient electron production rates resulting from other known stable agencies. Using the experimentally measured values of the night-time electron densities, the number of additional electrons/cc expected from the passage of these sources is computed. For the 164 kHz transmission from Tashkent, received at Ahmedabad, the associated enhancement in the attenuation is calculated using the full wave admittance technique of Barron and Budden. Reasonable agreement is shown to exist between the calculated values of the attenuation and those of direct observations.
Chakravarty S. C.
Jain Arun K.
Kasturirangan K.
Ramanathan K. R.
Rao U. R.
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