Observing and studying 20.1 MHz solar radio signals
Other Title(s)
رصد و دراسة الإشارات الراديوية الشمسية بتردد 20.1 ميكاهرتز
Dissertant
Thesis advisor
al-Nuaymi, Muhammad Salih Ahmad
al-Sabti, Abd al-Azim Ward Shjar
Comitee Members
al-Tawil, Radi Sh.
Abbud, Kamal Muhammad
Abd al-Wahhab, Hassan N.
Salih, Muhammad A. B.
University
University of Baghdad
Faculty
College of Science
Department
Astronomy and Space Department
University Country
Iraq
Degree
Ph.D.
Degree Date
2008
English Abstract
Solar radiations can be regarded as a useful source of information for studying and examining the Sun as a natural reactor.
Observing and analyzing solar emission using radio telescope are widely adopted by astronomers as radio telescopes are functioning adequately under various weather conditions that optical telescopes do not.
The objective of the present work is to observe and analyze solar radio bursts at 20.1 MHz frequency.
To make this study possible, a radio telescope capable of observing 20.1 MHz emission has been employed.
This telescope consists mainly of an antenna and a receiver.
The antenna is designed and assembled to collect the desired data.
A computer program is used to convert analog data into digital data and saved them in assigned files.
Solar storms type III were observed and recorded during the period 1-1-2006 to 30-6-2006 (coincides with the present minimum solar cycle).
The collected data which contains noise and solar bursts are carefully examined and analyzed.
Observations show that solar bursts reached the terrestrial collector at different durations (around 60 seconds) and different intensities.
Furthermore, it is noticed that solar storms generally rise to a peak of emission faster than they drop off afterward.
This is thought to be due to very dynamic and changeable magnetic fields of Sun
Main Subjects
No. of Pages
70
Table of Contents
Table of contents.
Abstract.
Abstract in Arabic.
Chapter One : Introduction.
Chapter Two : Theory of solar flare and solar radio bursts.
Chapter Three : Description of the radio telescope system.
Chapter Four : Results and discussion.
Chapter Five : Conclusions and future work.
References.
American Psychological Association (APA)
Tuma, Ziyad Abd al-Ahad. (2008). Observing and studying 20.1 MHz solar radio signals. (Doctoral dissertations Theses and Dissertations Master). University of Baghdad, Iraq
https://search.emarefa.net/detail/BIM-604525
Modern Language Association (MLA)
Tuma, Ziyad Abd al-Ahad. Observing and studying 20.1 MHz solar radio signals. (Doctoral dissertations Theses and Dissertations Master). University of Baghdad. (2008).
https://search.emarefa.net/detail/BIM-604525
American Medical Association (AMA)
Tuma, Ziyad Abd al-Ahad. (2008). Observing and studying 20.1 MHz solar radio signals. (Doctoral dissertations Theses and Dissertations Master). University of Baghdad, Iraq
https://search.emarefa.net/detail/BIM-604525
Language
English
Data Type
Arab Theses
Record ID
BIM-604525
