Implementation of Frequency Drift for Identification of Solar Radio Burst Type II
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| internalnotes | [1] M. Durante and F. Cucinotta, "Physical basis of radiation protection in space travel," Reviews of Modern Physic, vol. 83, pp. 1245-1281, Nov. 2011. [2] Z. S. Hamidi, N. N. M. Shariff and C. Monstein, "Characterization of selected solar radio bursts based on solar activity detected by eCALLISTO (Malaysia)," International Letters of Chemistry Physics and Astronomy, vol. 13, pp. 144-154, Jul. 2014. [3] X. Wang and Y. Yan, "Analysis of the CME-driven shock from the SEP event that occurred on 2006 December 14," Research in Astronomy and Astrophysics, vol. 12, pp. 1535-1548, Nov. 2012. [4] A. G. Emslie, R. B. Dennis, A. Y. Shih, P. C. Chamberlin, R. A. Mewaldt, C. S. Moore, G. H. Share, A. Vourlidas and B. T. Welsch, “Global energetics of thirty-eight large solar eruptive events,” The Astrophysical Journal, vol. 759, pp. 71-117, Oct. 2012. [5] Z. S. Hamidi, N. N. M. Shariff and C. Monstein, “Occurrences rate of type II and III solar radio bursts at low frequency radio region 45- 870 MHz,” International Letters of Chemistry Physics and Astronomy, vol. 37, pp.103-112, Sep. 2013. [6] Z. Z. Abidin, N. M. Anim, Z. S. Hamidi, C. Monstein, Z. A. Ibrahim, and R. Umar, N. N. M. Shariff, N. Ramli, N. A. I. Aziz and I. Sukma, “Radio frequency interference in solar monitoring using CALLISTO,” New Astronomy Reviews, vol. 67, pp. 18-33, Aug. 2015. [7] H. A. S. Reid and H. Ratcliffe, “A review of solar type III radio bursts,” Research in Astronomy and Astrophysics, vol. 14, pp. 773- 803, Jul. 2014. [8] N. Gopalswamy, A. Lara, R. P. Lepping, M. L. Kaiser, D. Berdichevsky and O. C. St Cyr, “Interplanetary acceleration of coronal mass ejections,” Geophysical Research Letters, vol. 27, pp. 145-148 , Jan. 2000. [9] M. R. Kundu, Solar Radio Astronomy, New York, USA: Inderscience Publication, 1965. [10] P. Zucca, E. P. Carley, J. McCauley, P.T. Gallagher, C. Monstein, and R. T. J. McAteer, “Observations of low frequency solar radio bursts from the Rosse solar-terrestrial observatory," Solar Physics, vol. 280, pp. 591-602, Oct. 2012. [11] N. Gopalswamy, “Coronal mass ejections and solar radio emissions,” in Proc. PRE VII’11, 2011, p. 325-342. [12] M. Wang, G. Gao, R. Xie and C. Tan, “Possible radio precursors/signatures of the CMEs onset: Radio type III bursts and fine structures in the centimeter-metric wavelength region,” Research in Astronomy and Astrophysics, vol. 11, pp. 607-616, Dec. 2011. [13] N. Ramli, Z. S. Hamidi, Z. Z. Abidin and S. N. Shahar, “The relation between solar radio burst types II, III and IV due to solar activities,” in Proc. IconSpace’15, 2015, p. 123-127. [14] D. G. Wentzel, “Solar radio emission very near the plasma frequency,” The Astrophysical Journal, vol. 270, pp. 250-255, Jul. 1983. [15] N. H. Sabri, A. W. Azlan, R. Umar, S. S. Sulan, Z. A. Ibrahim and W. Z. A. W. Mokhtar, “The effect of solar radiation on radio signal for radio astronomy purposes,” Malaysian Journal of Analytical Sciences, vol. 19, pp. 1374-1381, Jul. 2015. [16] R. Umar, N. H. Sabri, Z. Z. Abidin, Z. A. Ibrahim, A. Azid, H. Juahir, M. E. Toriman and M. K. A. Kamarudin, “Preliminary study of radio astronomical lines effect of rain below 2.9 GHz,” Jurnal Teknologi, vol. 75, pp. 7-11, Jun. 2015. [17] A. Benz, C. Monstein and H. Meyer, “CALLISTO-A new concept for solar radio spectrometers,” Solar Physics, vol. 226, pp. 143-151, Jan. 2005. [18] V. V. Lobzin, I. H. Cairns, P. A. Robinson, G. Steward and G. Patterson, “Automatic recognition of type III solar radio bursts: Automated radio burst identification system method and first observations,” Space Weather, vol. 7, pp. 1-12, Apr. 2009. [19] V. V. Lobzin, I. H. Cairns, P. A. Robinson, G. Steward and P. Patterson, “Automatic recognition of coronal type II radio bursts: The automated radio burst identification system method and first observations,” The Astrophysical Journal Letters, vol. 710, pp. 58-62, Jan. 2010. [20] L. Ma, Z. Chen, L. Xu and Y. Yan, “Multimodal deep learning for solar radio burst classification,” Pattern Recognition, vol. 61, pp. 573-582, Jan. 2017. |
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| spelling | 14747 https://intelek.unisza.edu.my/intelek/pages/view.php?ref=14747 https://intelek.unisza.edu.my/intelek/pages/search.php?search=!collection407072 Restricted Document Article Journal application/pdf 7 Adobe Acrobat Pro DC 20 Paper Capture Plug-in with ClearScan 1.6 Acer acer ACER 2024-08-28 21:59:49 7593-01-FH02-ESERI-16-06916.pdf UniSZA Private Access Implementation of Frequency Drift for Identification of Solar Radio Burst Type II International Journal on Advance Science Engineering Information Technology Sun is constantly produced mass and radiation during its natural activities, which will interact with ionosphere and affect the earth weather. In radio astronomer community, CALLISTO is used to capture the radio signal comes from solar activities such as solar burst. Solar flares and Coronal Mass Ejections (CMEs) were closely associated with the production of solar radio burst Type II and III. However, the determination of solar burst existence is done manually using spectrograph which appears for every 15 minutes. In order to assist the solar radio researcher to speed up the process of solar burst identification and detection, this work presents a new algorithm to auto classify solar radio burst Type II and III. The value of frequency drift was used as the main idea in this auto classify algorithm because it can easily implemented using MATLAB. There are three main steps involved named as pre-processing, identification and classification. Auto calculation of frequency drift burst on spectra was obtained from two parts which are frequency axis (df) and time axis (dt). The results of the frequency drift implementation in classification algorithm show that the algorithm developed gave almost similar determination as in manual detection. However, there are always have rooms for improvement for better detection system in future which may include specific characterization of bursts and improved noise elimination. 6 5 775-780 [1] M. Durante and F. Cucinotta, "Physical basis of radiation protection in space travel," Reviews of Modern Physic, vol. 83, pp. 1245-1281, Nov. 2011. [2] Z. S. Hamidi, N. N. M. Shariff and C. Monstein, "Characterization of selected solar radio bursts based on solar activity detected by eCALLISTO (Malaysia)," International Letters of Chemistry Physics and Astronomy, vol. 13, pp. 144-154, Jul. 2014. [3] X. Wang and Y. Yan, "Analysis of the CME-driven shock from the SEP event that occurred on 2006 December 14," Research in Astronomy and Astrophysics, vol. 12, pp. 1535-1548, Nov. 2012. [4] A. G. Emslie, R. B. Dennis, A. Y. Shih, P. C. Chamberlin, R. A. Mewaldt, C. S. Moore, G. H. Share, A. Vourlidas and B. T. Welsch, “Global energetics of thirty-eight large solar eruptive events,” The Astrophysical Journal, vol. 759, pp. 71-117, Oct. 2012. [5] Z. S. Hamidi, N. N. M. Shariff and C. Monstein, “Occurrences rate of type II and III solar radio bursts at low frequency radio region 45- 870 MHz,” International Letters of Chemistry Physics and Astronomy, vol. 37, pp.103-112, Sep. 2013. [6] Z. Z. Abidin, N. M. Anim, Z. S. Hamidi, C. Monstein, Z. A. Ibrahim, and R. Umar, N. N. M. Shariff, N. Ramli, N. A. I. Aziz and I. Sukma, “Radio frequency interference in solar monitoring using CALLISTO,” New Astronomy Reviews, vol. 67, pp. 18-33, Aug. 2015. [7] H. A. S. Reid and H. Ratcliffe, “A review of solar type III radio bursts,” Research in Astronomy and Astrophysics, vol. 14, pp. 773- 803, Jul. 2014. [8] N. Gopalswamy, A. Lara, R. P. Lepping, M. L. Kaiser, D. Berdichevsky and O. C. St Cyr, “Interplanetary acceleration of coronal mass ejections,” Geophysical Research Letters, vol. 27, pp. 145-148 , Jan. 2000. [9] M. R. Kundu, Solar Radio Astronomy, New York, USA: Inderscience Publication, 1965. [10] P. Zucca, E. P. Carley, J. McCauley, P.T. Gallagher, C. Monstein, and R. T. J. McAteer, “Observations of low frequency solar radio bursts from the Rosse solar-terrestrial observatory," Solar Physics, vol. 280, pp. 591-602, Oct. 2012. [11] N. Gopalswamy, “Coronal mass ejections and solar radio emissions,” in Proc. PRE VII’11, 2011, p. 325-342. [12] M. Wang, G. Gao, R. Xie and C. Tan, “Possible radio precursors/signatures of the CMEs onset: Radio type III bursts and fine structures in the centimeter-metric wavelength region,” Research in Astronomy and Astrophysics, vol. 11, pp. 607-616, Dec. 2011. [13] N. Ramli, Z. S. Hamidi, Z. Z. Abidin and S. N. Shahar, “The relation between solar radio burst types II, III and IV due to solar activities,” in Proc. IconSpace’15, 2015, p. 123-127. [14] D. G. Wentzel, “Solar radio emission very near the plasma frequency,” The Astrophysical Journal, vol. 270, pp. 250-255, Jul. 1983. [15] N. H. Sabri, A. W. Azlan, R. Umar, S. S. Sulan, Z. A. Ibrahim and W. Z. A. W. Mokhtar, “The effect of solar radiation on radio signal for radio astronomy purposes,” Malaysian Journal of Analytical Sciences, vol. 19, pp. 1374-1381, Jul. 2015. [16] R. Umar, N. H. Sabri, Z. Z. Abidin, Z. A. Ibrahim, A. Azid, H. Juahir, M. E. Toriman and M. K. A. Kamarudin, “Preliminary study of radio astronomical lines effect of rain below 2.9 GHz,” Jurnal Teknologi, vol. 75, pp. 7-11, Jun. 2015. [17] A. Benz, C. Monstein and H. Meyer, “CALLISTO-A new concept for solar radio spectrometers,” Solar Physics, vol. 226, pp. 143-151, Jan. 2005. [18] V. V. Lobzin, I. H. Cairns, P. A. Robinson, G. Steward and G. Patterson, “Automatic recognition of type III solar radio bursts: Automated radio burst identification system method and first observations,” Space Weather, vol. 7, pp. 1-12, Apr. 2009. [19] V. V. Lobzin, I. H. Cairns, P. A. Robinson, G. Steward and P. Patterson, “Automatic recognition of coronal type II radio bursts: The automated radio burst identification system method and first observations,” The Astrophysical Journal Letters, vol. 710, pp. 58-62, Jan. 2010. [20] L. Ma, Z. Chen, L. Xu and Y. Yan, “Multimodal deep learning for solar radio burst classification,” Pattern Recognition, vol. 61, pp. 573-582, Jan. 2017. |
| spellingShingle | Implementation of Frequency Drift for Identification of Solar Radio Burst Type II |
| summary | Sun is constantly produced mass and radiation during its natural activities, which will interact with ionosphere and affect the earth weather. In radio astronomer community, CALLISTO is used to capture the radio signal comes from solar activities such as solar burst. Solar flares and Coronal Mass Ejections (CMEs) were closely associated with the production of solar radio burst Type II and III. However, the determination of solar burst existence is done manually using spectrograph which appears for every 15 minutes. In order to assist the solar radio researcher to speed up the process of solar burst identification and detection, this work presents a new algorithm to auto classify solar radio burst Type II and III. The value of frequency drift was used as the main idea in this auto classify algorithm because it can easily implemented using MATLAB. There are three main steps involved named as pre-processing, identification and classification. Auto calculation of frequency drift burst on spectra was obtained from two parts which are frequency axis (df) and time axis (dt). The results of the frequency drift implementation in classification algorithm show that the algorithm developed gave almost similar determination as in manual detection. However, there are always have rooms for improvement for better detection system in future which may include specific characterization of bursts and improved noise elimination. |
| title | Implementation of Frequency Drift for Identification of Solar Radio Burst Type II |
| title_full | Implementation of Frequency Drift for Identification of Solar Radio Burst Type II |
| title_fullStr | Implementation of Frequency Drift for Identification of Solar Radio Burst Type II |
| title_full_unstemmed | Implementation of Frequency Drift for Identification of Solar Radio Burst Type II |
| title_short | Implementation of Frequency Drift for Identification of Solar Radio Burst Type II |
| title_sort | implementation of frequency drift for identification of solar radio burst type ii |