Automated detection and statistical study of solar radio spikes
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://link.springer.com/content/pdf/10.1007/s10509-023-04172-8.pdf
Reference24 articles.
1. Abduallah, Y., Jordanova, V.K., Liu, H., Li, Q., Wang, J.T.L., Wang, H.: Predicting solar energetic particles using SDO/HMI vector magnetic data products and a bidirectional LSTM network. Astrophys. J. Suppl. Ser. 260(1), 16 (2022). https://doi.org/10.3847/1538-4365/ac5f56
2. Antonov, A.V., Melnik, V.N., Konovalenko, A.A., Dorovskyy, V.V., Koval, A.A.: Decameter type IV bursts, fiber-bursts and type III bursts associated with group of solar active regions. Radio Phys. Radio Astron. 19(4), 295–306 (2014). https://doi.org/10.15407/rpra19.04.295
3. Benz, A., Simnett, G.: Solar radio signatures suggestive of proton beams. Nature 320, 508–509 (1986). https://doi.org/10.1038/320508a0
4. Bouratzis, C., Hillaris, A., Alissandrakis, C.E., et al.: High resolution observations with Artemis-IV and the NRH-I. Type IV associated narrow-band bursts. Astron. Astrophys. 586, A29 (2016). https://doi.org/10.1051/0004-6361/201527229
5. Chernov, G.P., Poquerusse, M., Bougeret, J.-L., Zlobec, P.: Comparison of the properties of long-lasting and impulsive type IV solar radio bursts with fine structures. Radio Sci. 36(6), 1745–1755 (2001). https://doi.org/10.1029/2000RS002451
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