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International Letters of Chemistry, Physics and Astronomy
Volume 33

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Statistical Study of Nine Months Distribution of Solar Flares
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Statistical Study of Nine Months Distribution of Solar Flares

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Abstract:

Solar flare is one of the solar activities that take place in the outermost layer of the corona. Solar flares can heat the material to several million degrees in just a few minutes and at the same time they release the numerous amount of energy. It is believed that a change of magnetic field lines potentially creates the solar flares. The objectives of the study are to identify and compare the types of solar flares (in X-Ray) region and to improve understanding of solar flares. Data are taken from the NOAA website, from the United States Department of Commerce, NOAA, Space Weather Prediction Center (SPWC). Solar radio flux readings were merged together with the three classes and a total of nine graphs were plotted. In illustrating the relationship of solar radio flux and solar flares, it can be explained by studying the range values of flux corresponding to flares values. From this case study, it was found that the minimum value of solar radio flux in order for the flares to occur is equivalent 68 x 10-22Wm-2Hz-1. Thus, whenever the values of solar radio flux are high, there should be a higher number of flares produced by the sun. The overall range of solar radio flux recorded in this study ranging from 68 x 10-22 Wm-2Hz-1 to 96 x 10-22 Wm-2Hz-1. Observing and collecting data from the Sun and develop our very own new prediction methods will leads the accuracy of the prediction of the behavior of the Sun more precisely.

Info:

Periodical:
International Letters of Chemistry, Physics and Astronomy (Volume 33)
Pages:
1-11
DOI:
https://doi.org/10.18052/www.scipress.com/ILCPA.33.1
Citation:
Z. S. Hamidi et al., "Statistical Study of Nine Months Distribution of Solar Flares", International Letters of Chemistry, Physics and Astronomy, Vol. 33, pp. 1-11, 2014
Online since:
May 2014
Authors:
Zety Sharizat Hamidi, N.N.M. Shariff, C. Monstein
Keywords:
Burst, e-CALLISTO, Solar Eclipse, Solar Radio, Sun, Type III
Export:
RIS, BibTeX, Text
Distribution:
Open Access

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This work is licensed under a
Creative Commons Attribution 4.0 International License

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Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 4 (2014) 29-36.

Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 5 (2014) 32-42.

Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 5 (2014) 43-49.

Z. S. Hamidi, N. N. M. Shariff, International Letters of Chemistry, Physics and Astronomy 7 (2014) 21-29.

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Z. S. Hamidi, N. N. M. Shariff, C. Monstein, W. N. A. Wan Zulkifli, M. B. Ibrahim, N. S. Arifin, N. A. Amran, International Letters of Chemistry, Physics and Astronomy 8 (2014) 13-19.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, W. N. A. Wan Zulkifli, M. B. Ibrahim, N. S. Arifin, N. A. Amran, International Letters of Chemistry, Physics and Astronomy 9 (2014) 8-15.

Z. S. Hamidi, N. N. M. Shariff, M. F. Ali, C. Monstein, W. N. A. Wan Zulkifli, M. B. Ibrahim, N. S. Arifin, N. A. Amran, International Letters of Chemistry, Physics and Astronomy 9 (2014) 84-92.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 11(1) (2014) 51-58.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 11(2) (2014) 135-145.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 11(2) (2014) 167-176.

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Z. S. Hamidi, N. N. M. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 12 (2014) 84-102.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 13(2) (2014) 104-111.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 13(2) (2014) 135-143.

Z. S. Hamidi, N. N. M. Shariff, C. Monstein, International Letters of Chemistry, Physics and Astronomy 13(2) (2014) 144-154 ( Received 17 April 2014; accepted 25 April 2014 ).

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