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You searched for id:"oai:shodhganga.inflibnet.ac.in:10603/203717". One record found.

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1. [No author]. Time and frequency structure of broadband solar bursts in the 30 150 MHz band.

Degree: Physics, 2015, Bangalore University

newlineSolar radio physicists study the Sun as a star, the only star which one that can newlinebe observed in greater detail. Its atmosphere is a laboratory where unique newlineconditions of temperature, density and fluid motion exist which cannot be newlinereproduced in any terrestrial laboratory. The Sun can be studied in the optical newlineand radio band from ground based instruments. Galileo made the first optical newlinestudy of the Sun in 1609. Soon after Maxwell formulated the electromagnetic newlinetheory of light and subsequent demonstration of the existence of radio waves by newlineHertz. Later on there were many attempts made to detect radio emission from newlinethe Sun. Early attempts by Oliver Lodge and Thomson Edison were newlineunsuccessful because their apparatus was insensitive. Radio studies of the Sun newlinewere started with the serependitious discovery by J.S.Hey in the year 1942 newlineduring the World War II. The close association between the meter wave radio newlinebursts and solar flares was discovered by Hey. George Southworth detected newlinethe thermal radiation from the Sun in the same year at Bell Telephone labs. newlineRadio observations have the following advantages over other wavelength newlineregions: (i) Unique diagnosis for density, temperature and magnetic field (ii) newlineRadio emission can be observed from all layers of the Sun and (iii) newlineObservations can be made with high spatial, time and frequency resolution. newlineThe contributions by several solar radio astronomers in Australia, France and newlineCambridge led to the detection of three type basic components in the radio newlineemission of the Sun. They are (1). Quiet-Sun component, (2) Slowly varying newlinecomponent and (3) Radio bursts. The quiet-Sun radio emission is the radiation newlinethat remains constant for periods of months to years. This component is due to newlinethe thermal emission from the million degree corona. Advisors/Committee Members: Vijayakumar H Doddamani.

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

author], [. (2015). Time and frequency structure of broadband solar bursts in the 30 150 MHz band. (Thesis). Bangalore University. Retrieved from http://shodhganga.inflibnet.ac.in/handle/10603/203717

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

author], [No. “Time and frequency structure of broadband solar bursts in the 30 150 MHz band.” 2015. Thesis, Bangalore University. Accessed September 21, 2018. http://shodhganga.inflibnet.ac.in/handle/10603/203717.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

author], [No. “Time and frequency structure of broadband solar bursts in the 30 150 MHz band.” 2015. Web. 21 Sep 2018.

Vancouver:

author] [. Time and frequency structure of broadband solar bursts in the 30 150 MHz band. [Internet] [Thesis]. Bangalore University; 2015. [cited 2018 Sep 21]. Available from: http://shodhganga.inflibnet.ac.in/handle/10603/203717.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

author] [. Time and frequency structure of broadband solar bursts in the 30 150 MHz band. [Thesis]. Bangalore University; 2015. Available from: http://shodhganga.inflibnet.ac.in/handle/10603/203717

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

.