Abstract
We have analyzed type III-\(l\) radio bursts associated with SEP events (>10 MeV) during solar cycles 23 and 24 respectively. We have studied the properties of type III radio bursts and SEP events. We have also analyzed the correlation between the properties of type III-\(l\) bursts and SEPs. We found that the mean duration of type III-\(l\) bursts and their deviation for solar cycle 24 is higher. The log peak intensity of SEP and its deviation is higher for solar cycle 23, which suggests that the SEP events for solar cycle 23 are faster and long-duration events. From the correlations, we conclude that the type III-\(l\) radio burst properties for solar cycle 23 contribute more towards the SEP events as compared to solar cycle 24.
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Acknowledgement
We are thankful to the Culgoora and Learmooth radio observatories for their open data policy. We have used GOES-NOAA data for SEP events which are generated by the National Ocean and Atmospheric Administration, U.S. Department of Commerce, and also we used Wind/WAVES data for radio bursts which is maintained by the National Aeronautics and Space Administration, Goddard Space flight center, NASA.
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Deepak Pandey: Prepare the main body of the paper. Bimal Pande: Design the tables of paper and conclude the paper content. Seema Pande: Checked the grammar and spelling of the paper and set the format of the paper.
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Pandey, D., Pande, B. & Pande, S. Comparative analysis of type III solar radio bursts associated with solar particle events and its impact on space weather for solar cycle 23 & 24. Astrophys Space Sci 367, 91 (2022). https://doi.org/10.1007/s10509-022-04129-3
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DOI: https://doi.org/10.1007/s10509-022-04129-3