Three-station observations of interplanetary scintillation at 327 MHz-II - Evolution of two-dimensional solar wind speed structure during 1983 to 1985

Details Three-station observations of interplanetary scintillation at 327 MHz-II - Evolution of two-dimensional solar wind speed structure during 1983 to 1985 Three-station observations of interplanetary scintillation at 327 MHz-II - Evolution of two-dimensional solar wind speed structure during 1983 to 1985

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nuria..33....1k&link_type=abstract

Nagoya University, Research Institute of Atmospherics, Proceedings (ISSN 0077-264X), vol. 33, March 1986, p. 1-18.

Astronomy and Astrophysics

Astronomy

2

Computer Aided Mapping, Interplanetary Medium, Radio Astronomy, Scintillation, Solar Wind Velocity, Color Coding, Interplanetary Magnetic Fields, Neutral Sheets, Solar Activity Effects, Solar Rotation

Scientific paper

Regular three-site observations of 327-MHz interplanetary scintillation obtained using the stations and apparatus described by Kojima et al. (1982) during 1983-1985 are reported and analyzed in terms of the two-dimensional structure of the solar wind. The data are presented in a series of color maps and characterized in detail. Features observed include concentration of low-speed regions around a wavy neutral sheet formed by the magnetic dipole and quadrupole fields, fuller development of high-speed regions in the Northern Hemisphere, large latitudional speed gradients, and two minimum-speed regions separated longitudinally by 180 deg and coincident with two giant bipolar magnetic regions.

Affiliated with

Also associated with

No associations

Rating

Three-station observations of interplanetary scintillation at 327 MHz-II - Evolution of two-dimensional solar wind speed structure during 1983 to 1985 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 Three-station observations of interplanetary scintillation at 327 MHz-II - Evolution of two-dimensional solar wind speed structure during 1983 to 1985, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Three-station observations of interplanetary scintillation at 327 MHz-II - Evolution of two-dimensional solar wind speed structure during 1983 to 1985 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1286070