Observations of the brightness temperature distribution of the quiet solar corona at decametric wavelengths

Details Observations of the brightness temperature distribution of the quiet solar corona at decametric wavelengths Observations of the brightness temperature distribution of the quiet solar corona at decametric wavelengths

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sici.symp...23s&link_type=abstract

In Alabama Univ., Huntsville. STIP Symposium on Physical Interpretation of Solar/Interplanetary and Cometary Intervals p 23 (SEE

Physics

Brightness Distribution, Brightness Temperature, Decimeter Waves, Interplanetary Medium, Intervals, Solar Corona, Arrays, Interferometers, Radio Telescopes

Scientific paper

The brightness temperature distribution of the quiet solar corona at a wavelength of 8.9 meters is measured by two types of radio telescope: (1) a 'T' type array with a resolution of 26'X38', and (2) a fan beam interferometer with an E-W resolution of 3'. It is found that the persistent bright regions do not have any angular structure on scales of 6' or less. The daily variations of the brightness temperature of different regions are studied and the possible interpretation discussed.

Affiliated with

Also associated with

No associations

Rating

Observations of the brightness temperature distribution of the quiet solar corona at decametric wavelengths 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 Observations of the brightness temperature distribution of the quiet solar corona at decametric wavelengths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of the brightness temperature distribution of the quiet solar corona at decametric wavelengths will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1761422