Possibility of measuring the parameters of large-scale inhomogeneities in the interplanetary plasma by radio astronomy

Details Possibility of measuring the parameters of large-scale inhomogeneities in the interplanetary plasma by radio astronomy Possibility of measuring the parameters of large-scale inhomogeneities in the interplanetary plasma by radio astronomy

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975azh....52..369s&link_type=abstract

Astronomicheskii Zhurnal, vol. 52, Mar.-Apr. 1975, p. 369-373. In Russian.

Astronomy and Astrophysics

Astronomy

2

Cosmic Plasma, Interplanetary Medium, Nonuniform Plasmas, Radio Astronomy, Radio Wave Refraction, Solar Wind, Cross Correlation, Electron Density Profiles, Plasma Density, Scintillation

Scientific paper

The possibility is considered of measuring refraction on large-scale inhomogeneities in the interplanetary plasma by terrestrial radio astronomical observations. The method is based on the measurement of the scintillation pattern shift at two frequencies that is caused by refraction. Values are estimated for the refraction shift on the mean electron density gradient and on inhomogeneities measuring 10 to the 9th power cm.

Affiliated with

Also associated with

No associations

Rating

Possibility of measuring the parameters of large-scale inhomogeneities in the interplanetary plasma by radio astronomy 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 Possibility of measuring the parameters of large-scale inhomogeneities in the interplanetary plasma by radio astronomy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Possibility of measuring the parameters of large-scale inhomogeneities in the interplanetary plasma by radio astronomy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-947764