Open Access
Issue |
J. Space Weather Space Clim.
Volume 9, 2019
Developing New Space Weather Tools: Transitioning fundamental science to operational prediction systems
|
|
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Article Number | A6 | |
Number of page(s) | 12 | |
DOI | https://doi.org/10.1051/swsc/2019002 | |
Published online | 01 February 2019 |
- Al-Ghraibah A, Boucheron LE, McAteer RTJ. 2015. An automated classification approach to ranking photospheric proxies of magnetic energy build-up. A&A 579: A64. DOI: 10.1051/0004-6361/201525978. [CrossRef] [EDP Sciences] [Google Scholar]
- Baranyi T, Győri L, Ludmány A. 2016. On-line tools for solar data compiled at the Debrecen observatory and their extensions with the Greenwich sunspot data. Sol Phys 291: 3081–3102. DOI: 10.1007/s11207-016-0930-1. [CrossRef] [Google Scholar]
- Barnes G, Leka KD, Schrijver CJ, Colak T, Qahwaji R, et al. 2016. A comparison of flare forecasting methods. I. Results from the All-Clear Workshop. Astrophys J 829: 89. DOI: 10.3847/0004-637X/829/2/89. [Google Scholar]
- Benz AO. 2017. Flare observations. Living Rev Sol Phys 14: 2. DOI: 10.1007/s41116-016-0004-3. [CrossRef] [Google Scholar]
- Georgoulis MK. 2012. On our ability to predict major solar flares. Astrophys Space Sci Proc 30: 93. DOI: 10.1007/978-3-642-29417-4-9. [CrossRef] [Google Scholar]
- Georgoulis MK. 2013. Toward an efficient prediction of solar flares: Which parameters, and how? Entropy 15: 5022–5052. DOI: 10.3390/e15115022. [CrossRef] [Google Scholar]
- Győri L., Baranyi T., Ludmány A.. 2011. Photospheric data programs at the Debrecen Observatory. In: Prasad Choudhary D. Strassmeier K.G. (Editors), Physics of sun and star spots, vol. 273 of IAU Symposium, Cambridge University Press, Cambridge, pp. 403–407. DOI: 10.1017/S174392131101564X. [Google Scholar]
- Korsós MB, Baranyi T, Ludmány A. 2014. Pre-flare dynamics of sunspot groups. Astrophys J 789: 107. DOI: 10.1088/0004-637X/789/2/107. [CrossRef] [Google Scholar]
- Korsós MB, Ludmány A, Erdélyi R, Baranyi T. 2015. On flare predictability based on sunspot group evolution. Astrophys J 802: L21. DOI: 10.1088/2041-8205/802/2/L21. [CrossRef] [Google Scholar]
- Korsós M.B., Ruderman M.S.. 2016. On flare and CME predictability based on sunspot group evolution. In: Dorotovic, I., Fischer, C.E. Temmer, M. (Editors), Coimbra solar physics meeting: Ground-based solar observations in the space instrumentation era, vol. 504 of Astronomical Society of the Pacific Conference Series, University of Coimbra, Coimbra, 43 p. [Google Scholar]
- Louis RE, Kliem B, Ravindra B, Chintzoglou G. 2015. Triggering an eruptive flare by emerging flux in a solar active-region complex. Sol Phys 290: 3641–3662. DOI: 10.1007/s11207-015-0726-8. [NASA ADS] [CrossRef] [Google Scholar]
- Schrijver CJ. 2007. A characteristic magnetic field pattern associated with all major solar flares and its use in flare forecasting. Astrophys J Lett 655: L117–L120. DOI: 10.1086/511857. [CrossRef] [Google Scholar]
- Yamada M. 1999. Review of controlled laboratory experiments on physics of magnetic reconnection. J Geophys Res 104: 14529–14542. DOI: 10.1029/1998JA900169. [CrossRef] [Google Scholar]
- Yamada M, Kulsrud R, Ji H. 2010. Magnetic reconnection. Rev Modern Phys 82: 603–664. DOI: 10.1103/RevModPhys.82.603. [Google Scholar]
- Yang S, Zhang J, Xiang Y. 2015. Magnetic reconnection between small-scale loops observed with the new vacuum solar telescope. Astrophys J Lett 798: L11. DOI: 10.1088/2041-8205/798/1/L11. [Google Scholar]
- Ye Y, Korsós MB, Erdélyi R. 2018. Detailed analysis of dynamic evolution of three Active Regions at the photospheric level before flare and CME occurrence. Adv Space Res 61: 673–682. DOI: 10.1016/j.asr.2017.09.038. [CrossRef] [Google Scholar]
- Zheng R, Korsós MB, Erdélyi R. 2015. Semicircular-like secondary flare ribbons associated with a failed eruption. Astrophys J 809: 45. DOI: 10.1088/0004-637X/809/1/45. [CrossRef] [Google Scholar]
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