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Characteristics of Decametric Emission of Jupiter | ||
| Al-Mustansiriyah Journal of Science | ||
| Article 1, Volume 25, Issue 1, 2014, Pages 95-102 | ||
| Author | ||
| Rasha H. Ibrahim | ||
| Abstract | ||
| A statistical study was made to know the characteristics of Decametric (DAM) emission emitted from Jupiter's planet. These characteristics are the sporadic nature, time, type and the frequency. Period of 11 years was taken to study the first and year 2004 was taken to study the others. Data were provided from Radio Jove project, which gave information about the observer's location, date, time, type and the frequency. The results indicated that the DAM emission was sporadic, the time was between (00:01-05:31) hour, it was found that (Io-B) is the largest number, as compared with others, a large number emission occurred at frequency range (20-21) MHz. The results were compared with results of Radio Jove software, which indicated that the DAM emission is sporadic, the time is between (00:01-05:00) and the frequency is 21MHz. | ||
| Keywords | ||
| DAM Emission; Acceleration of Particles; Radio Signals | ||
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