Issue
J. Space Weather Space Clim.
Volume 7, 2017
Flares, coronal mass ejections and solar energetic particles and their space weather impacts
Article Number A37
Number of page(s) 15
DOI https://doi.org/10.1051/swsc/2017035
Published online 25 December 2017
  • Cane HV, Erickson WC, Prestage NP. 2002. Solar flares, type III radio bursts, coronal mass ejections, and energetic particles. J Geophys Res: Space Phys 107: 1315. DOI:10.1029/2001JA000320. [NASA ADS] [CrossRef]
  • Cane HV, Richardson IG, von Rosenvinge TT. 2010. A study of solar energetic particle events of 1997–2006: their composition and associations. J Geophys Res: Space Phys 115: A08101. DOI:10.1029/2009JA014848.
  • Chertok IM. 1990. On the correlation between the solar gamma-ray line emission, radio bursts and proton fluxes in the interplanetary space. Astron Nachr 311: 379–381. [CrossRef]
  • Cliver EW, Kahler SW, Reames DV. 2004. Coronal shocks and solar energetic proton events. Astrophys J 605: 902–910. DOI:10.1086/382651. [NASA ADS] [CrossRef]
  • Cliver EW, Ling AG. 2007. Electrons and protons in solar energetic particle events. Astrophys J 658: 1349–1356. DOI:10.1086/511737. [CrossRef]
  • Crosby N, Heynderickx D, Jiggens P, Aran A, Sanahuja B, et al. 2015. SEPEM: a tool for statistical modeling the solar energetic particle environment. Space Weather 13: 406–426. DOI:10.1002/2013SW001008. [CrossRef]
  • Desai M, Giacalone J. 2016. Large gradual solar energetic particle events. Living Rev Sol Phys 13: 3. DOI:10.1007/s41116-016-0002-5. [CrossRef]
  • Dierckxsens M, Tziotziou K, Dalla S, Patsou I, Marsh MS, Crosby NB, Malandraki O, Tsiropoula G. 2015. Relationship between solar energetic particles and properties of flares and CMEs: statistical analysis of solar cycle 23 events. Sol Phys 290: 841–874. DOI:10.1007/s11207-014-0641-4. [CrossRef]
  • Gopalswamy N. 2003. Solar and geospace connections of energetic particle events. Geophys Res Lett 30: 8013. DOI:10.1029/2003GL017277.
  • Gopalswamy N, Yashiro S, Akiyama S, Mäkelä P, Xie H, Kaiser ML, Howard RA, Bougeret JL. 2008. Coronal mass ejections, type II radio bursts, and solar energetic particle events in the SOHO era. Ann Geophys 26: 3033–3047. DOI:10.5194/angeo-26-3033-2008. [NASA ADS] [CrossRef]
  • Kahler SW. 1982a. Radio burst characteristics of solar proton flares. Astrophys J 261: 710–719. DOI:10.1086/160381. [NASA ADS] [CrossRef]
  • Kahler SW. 1982b. The role of the big flare syndrome in correlations of solar energetic proton fluxes and associated microwave burst parameters. J Geophys Res 87: 3439–3448. DOI:10.1029/JA087iA05p03439. [NASA ADS] [CrossRef]
  • Laurenza M, Cliver EW, Hewitt J, Storini M, Ling AG, Balch CC, Kaiser ML. 2009. A technique for short-term warning of solar energetic particle events based on flare location, flare size, and evidence of particle escape. Space Weather 7: S04008. DOI:10.1029/2007SW000379. [NASA ADS] [CrossRef]
  • MacDowall RJ, Lara A, Manoharan PK, Nitta NV, Rosas AM, Bougeret JL. 2003. Long-duration hectometric type III radio bursts and their association with solar energetic particle (SEP) events. Geophys Res Lett 30: 8018. DOI:10.1029/2002GL016624. [CrossRef]
  • Melrose DB. 1985. Plasma emission mechanisms. In McLean DJ, Labrum NR, eds, pp. 177–210.
  • Miteva R, Klein K-L, Malandraki O, Dorrian G. 2013a. Solar energetic particle events in the 23rd solar cycle: interplanetary magnetic field configuration and statistical relationship with flares and CMEs. Sol Phys 282: 579–613. DOI:10.1007/s11207-012-0195-2. [CrossRef]
  • Miteva R, Klein K-L, Samwel SW, Nindos A, Kouloumvakos A, Reid H. 2013b. Radio signatures of solar energetic particles during the 23rd solar cycle. Cent Eur Astrophys Bull 37: 541–553.
  • Miteva R, Samwel SW, Costa-Duarte MV. 2017a. Solar energetic particle catalogs: assumptions, uncertainties and validity of reports. J Atmos Sol Terr Phys DOI:10.1016/j.jastp.2017.05.003, http://www.sciencedirect.com/science/article/pii/S1364682617302924.
  • Miteva R, Samwel SW, Costa-Duarte MV, Malandraki OE. 2017b. Solar cycle dependence of Wind/EPACT protons, solar flares and coronal mass ejections. Sun Geosph 12: 11–19.
  • Miteva R, Samwel SW, Krupar V. 2017c. Solar radio bursts from proton-producing flares and CMEs. In Ninth workshop ‘Solar in fluences on the magnetosphere, ionosphere and atmosphere’, Georgieva K, Kirov B, Danov D, eds. Proceedings of the Conference held 30 May–3 June, 2017 in Sunny Beach, Bulgaria, pp. 19–23. ISSN 2367-7570.
  • Nelson GJ, Melrose DB. 1985. Type II bursts. In McLean DJ, Labrum NR, eds, pp. 333–359.
  • Nindos A, Aurass H, Klein K-L, Trottet G. 2008. Radio emission of flares and coronal mass ejections. Invited review. Sol Phys 253: 3–41. DOI:10.1007/s11207-008-9258-9. [NASA ADS] [CrossRef]
  • Núñez M. 2011. Predicting solar energetic proton events (E greater than 10 MeV). Space Weather 9: 07003. DOI:10.1029/2010SW000640.
  • Núñez M. 2015. Real-time prediction of the occurrence and intensity of the first hours of greater than 100 MeV solar energetic proton events. Space Weather 13: 807–819. DOI:10.1002/2015SW001256. [CrossRef]
  • Papaioannou A, Sandberg I, Anastasiadis A, Kouloumvakos A, Georgoulis MK, Tziotziou K, Tsiropoula G, Jiggens P, Hilgers A. 2016. Solar flares, coronal mass ejections and solar energetic particle event characteristics. J Space Weather Space Clim 6: A42. DOI:10.1051/swsc/2016035. [CrossRef] [EDP Sciences]
  • Pick M. 1986. Observations of radio continua and terminology. Sol Phys 104: 19–32. DOI:10.1007/BF00159942. [NASA ADS] [CrossRef]
  • Pick M, Vilmer N. 2008. Sixty-five years of solar radioastronomy: flares, coronal mass ejections and Sun Earth connection. Astron Astrophys Rev 16: 1–153. DOI:10.1007/s00159-008-0013-x. [NASA ADS] [CrossRef] [MathSciNet]
  • Posner A. 2007. Up to 1-hour forecasting of radiation hazards from solar energetic ion events with relativistic electrons. Space Weather 5: S05001. DOI:10.1029/2006SW000268. [CrossRef]
  • Prakash O, Feng L, Michalek G, Gan W, Lu L, Shanmugaraju A, Umapathy S. 2017. Characteristics of events with metric-to-decahectometric type II radio bursts associated with CMEs and flares in relation to SEP events. Astrophys Space Sci 362: 56. DOI:10.1007/s10509-017-3034-y. [CrossRef]
  • Pulkkinen T. 2007. Space weather: terrestrial perspective. Living Rev Sol Phys 4: 1. DOI:10.12942/lrsp-2007-1. [CrossRef]
  • Schwenn R. 2006. Space weather: the solar perspective. Living Rev Sol Phys 3: 2. DOI:10.12942/lrsp-2006-2. [CrossRef]
  • Stewart RT. 1985. Moving type IV bursts. In McLean DJ, Labrum NR, eds, pp. 361–383.
  • Suzuki S, Dulk GA. 1985. Bursts of type III and type V. In McLean DJ, Labrum NR, eds, pp. 289–332.
  • Thejappa G, MacDowall RJ, Kaiser ML. 2007. Monte Carlo simulation of directivity of interplanetary radio bursts. Astrophys J 671: 894–906. DOI:10.1086/522664. [NASA ADS] [CrossRef]
  • Trottet G, Samwel S, Klein K-L, Dudok de Wit T , Miteva R. 2015. Statistical evidence for contributions of flares and coronal mass ejections to major solar energetic particle events. Sol Phys 290: 819–839. DOI:10.1007/s11207-014-0628-1. [CrossRef]
  • Vainio R, Valtonen E, Heber B, Malandraki OE, Papaioannou A, et al. 2013. The first SEPServer event catalogue ∼68-MeV solar proton events observed at 1 AU in 1996-2010. J Space Weather Space Clim 3: A12. DOI:10.1051/swsc/2013030. [CrossRef] [EDP Sciences]
  • Warmuth A, Mann G. 2004. The application of radio diagnostics to the study of the solar drivers of space weather. In Scherer K, Fichter H, Herber B, eds. Lecture Notes in Physics, Berlin Springer Verlag, vol. 656 of Lecture Notes in Physics, Springer Verlag, Berlin 49. DOI:10.1007/b100037.
  • Wild JP, Smerd SF, Weiss AA. 1963. Solar bursts. ARA&A 1: 291. DOI:10.1146/annurev.aa.01.090163.001451. [NASA ADS] [CrossRef]
  • Winter LM, Ledbetter K. 2015. Type II and type III radio bursts and their correlation with solar energetic proton events. Astrophys J 809: 105. DOI:10.1088/0004-637X/809/1/105. [CrossRef]

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