Transition region of the solar wind according to observations of scintillations of a water-vapor-line maser source

Details Transition region of the solar wind according to observations of scintillations of a water-vapor-line maser source Transition region of the solar wind according to observations of scintillations of a water-vapor-line maser source

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..537b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, July-Aug. 1984, p. 537-540. In Russian.

Astronomy and Astrophysics

Astronomy

1

Interstellar Masers, Scintillation, Solar Wind, Water Masers, Astronomical Models, Distance, Transonic Flow

Scientific paper

The dependence of the scintillation index on radial distance in the near-solar medium m(R) for R = 10-20 solar radii is calculated on the basis of scintillation observations of S252A in June 1983. The results are compared with previous results on m(R) variations, and it is found that the data obtained refer to the region of the subsonic-to-supersonic transition of the solar wind. The resulting form of m(R) can be explained by a model which takes into account the radial features of electron-density fluctuations as well as heliolatitude variations arising at the decline phase of the 11-year solar cycle.

Affiliated with

Also associated with

No associations

Rating

Transition region of the solar wind according to observations of scintillations of a water-vapor-line maser source 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 Transition region of the solar wind according to observations of scintillations of a water-vapor-line maser source, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Transition region of the solar wind according to observations of scintillations of a water-vapor-line maser source will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1675730