Open Access
Issue
J. Space Weather Space Clim.
Volume 7, 2017
Article Number A13
Number of page(s) 15
DOI https://doi.org/10.1051/swsc/2017011
Published online 02 June 2017
  • Aran, A., B.Sanahuja, and D.Lario. SOLPEN CO: a solar particle engineering code. Adv. Space Res., 37, 1240–1246, 2006, DOI: 10.1016/j.asr.2005.09.019. [NASA ADS] [CrossRef]
  • Aran, A., B.Sanahuja, and D.Lario. Comparing proton fluxes of central meridian SEP events with those predicted by SOLPENCO. Adv. Space Res., 42, 1492–1499, 2008, DOI: 10.1016/j.asr.2007.08.003. [CrossRef]
  • Balch, C.C. Updated verification of the space weather prediction center’s solar energetic particle prediction model. Space Weather, 6, S01001, 2008, DOI: 10.1029/2007SW000337. [CrossRef]
  • Belov, A. Properties of solar X-ray flares and proton event forecasting. Adv. Space Res., 43 (4), 467–473, 2009, DOI: 10.1016/j.asr.2008.08.011. [CrossRef]
  • Davis, J., and M.Goadrich, The relationship between precision-recall and ROC curves. In: W., Cohen, and A.Moore, Editors, Proceedings Of The Twenty-Third International Conference On Machine Learning (Icml 06), Vol. 148 Of Acm International Conference Proceeding Series, Association for Computing Machinery, New York, NY, USA, 233–240, 2006, DOI: 10.1145/1143844.1143874.
  • Dennis, B.R., and D.M.Zarro. The Neupert effect − what can it tell us about the impulsive and gradual phases of solar flares? Sol. Phys., 146, 177–190, 1993, DOI: 10.1007/BF00662178. [NASA ADS] [CrossRef]
  • Dierckxsens, M., K.Tziotziou, S.Dalla, I.Patsou, M.S.Marsh, N.B.Crosby, O.Malandraki, and G.Tsiropoula. Relationship between solar energetic particles and properties of flares and CMEs: statistical analysis of solar cycle 23 events. Sol. Phys., 290, 841–874, 2015, DOI: 10.1007/s11207-014-0641-4. [CrossRef]
  • Dresing, N., R.Gómez-Herrero, B.Heber, A.Klassen, O.Malandraki, W.Dröge, and Y.Kartavykh. Statistical survey of widely spread out solar electron events observed with STEREO and ACE with special attention to anisotropies. A&A, 567, A27, 2014, DOI: 10.1051/0004-6361/201423789. [NASA ADS] [CrossRef] [EDP Sciences]
  • Garcia, H.A. Forecasting methods for occurrence and magnitude of proton storms with solar soft X-rays. Space Weather, 2, S02002, 2004, DOI: 10.1029/2003SW000001.
  • García-Rigo, A., M.Núñez, R.Qahwaji, O.Ashamari, P.Jiggens, G.Pérez, M.Hernández-Pajares, and A.Hilgers. Prediction and warning system of SEP events and solar flares for risk estimation in space launch operations. J. Space Weather Space Clim., 6 (27), A28, 2016, DOI: 10.1051/swsc/2016021. [CrossRef] [EDP Sciences]
  • Holman, G.D., M.J.Aschwanden, H.Aurass, M.Battaglia, P.C.Grigis, E.P.Kontar, W.Liu, P.Saint-Hilaire, and V.V.Zharkova. Implications of X-ray observations for electron acceleration and propagation in solar flares. Space Sci. Rev., 159, 107–166, 2011, DOI: 10.1007/s11214-010-9680-9. [NASA ADS] [CrossRef]
  • Kahler, S.W., E.W.Cliver, and A.G.Ling. Validating the proton prediction system (PPS). J. Atmos. Solar-Terr. Phys., 69, 43–49, 2007, DOI: 10.1016/j.jastp.2006.06.009. [CrossRef]
  • Kane, S.R., P.Evenson, and P.Meyer. Acceleration of interplanetary solar electrons in the 1982 August 14 flare. Astrophys. J., 299, L107–L110, 1985, DOI: 10.1086/184590. [CrossRef]
  • Klein, K.-L., S.Krucker, G.Lointier, and A.Kerdraon. Open magnetic flux tubes in the corona and the transport of solar energetic particles. A&A, 486, 589–596, 2008, DOI: 10.1051/0004-6361:20079228. [NASA ADS] [CrossRef] [EDP Sciences]
  • Kuznetsov, S.N., V.G.Kurt, B.Y.Yushkov, K.Kudela, and V.I.Galkin. Gamma-ray and high-energy-neutron measurements on CORONAS-F during the solar flare of 28 October 2003. Sol. Phys., 268, 175–193, 2011, DOI: 10.1007/s11207-010-9669-2. [CrossRef]
  • Laitinen, T., and S.Dalla. Energetic particle transport across the mean magnetic field: before diffusion. Astrophys. J., 834, 127, 2017, DOI: 10.3847/1538-4357/834/2/127. [CrossRef]
  • Laurenza, M., E.W.Cliver J.Hewitt, M.Storini, A.G.Ling, C.C.Balch, and M.L.Kaiser. 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, 2009, DOI: 10.1029/2007SW000379. [NASA ADS] [CrossRef]
  • Lee, M.A., R.A.Mewaldt, and J.Giacalone. Shock acceleration of ions in the heliosphere. Space Sci. Rev., 173, 247–281, 2012, DOI: 10.1007/s11214-012-9932-y. [NASA ADS] [CrossRef]
  • Mann, G., F.Jansen, R.J.MacDowall, M.L.Kaiser, and R.G.Stone. A heliospheric density model and type III radio bursts. A&A, 348, 614–620, 1999.
  • Marsh, M.S., S.Dalla, M.Dierckxsens, T.Laitinen, and N.B.Crosby. SPARX: a modeling system for solar energetic particle radiation space weather forecasting. Space Weather, 13, 386–394, 2015, DOI: 10.1002/2014SW001120. [CrossRef]
  • Masson, S., P.Démoulin, S.Dasso, and K.-L.Klein. The interplanetary magnetic structure that guides solar relativistic particles. A&A, 538, A32, 2012, DOI: 10.1051/0004-6361/201118145. [NASA ADS] [CrossRef] [EDP Sciences]
  • Nakajima, H., H.Sekiguchi, M.Sawa, K.Kai, and S.Kawashima. The radiometer and polarimeters at 80, 35, and 17 GHz for solar observations at Nobeyama. Publ. Astron. Soc. Jpn., 37, 163–170, 1985.
  • Neupert, W.M. Comparison of solar X-ray line emission with microwave emission during flares. Astrophys. J., 153, L59–L64, 1968, DOI: 10.1086/180220. [NASA ADS] [CrossRef]
  • Núñez, M. Predicting solar energetic proton events (E > 10 MeV). Space Weather, 9, 07003, 2011, DOI: 10.1029/2010SW000640.
  • Núñez, M. Real-time prediction of the occurrence and intensity of the first hours of > 100 MeV solar energetic proton events. Space Weather, 13, 807–819, 2015, DOI: 10.1002/2015SW001256. [CrossRef]
  • Posner, A. Up to 1-hour forecasting of radiation hazards from solar energetic ion events with relativistic electrons. Space Weather, 5, S05001, 2007, DOI: 10.1029/2006SW000268. [CrossRef]
  • Richardson, I.G., and H.V.Cane. Particle flows observed in ejecta during solar event onsets and their implication for the magnetic field topology. J. Geophys. Res., 101, 27521–27532, 1996, DOI: 10.1029/96JA02643. [NASA ADS] [CrossRef]
  • Richardson, I.G., T.T.von Rosenvinge, H.V.Cane, E.R.Christian, C.M.S.Cohen, A.W.Labrador, R.A.Leske, R.A.Mewaldt, M.E.Wiedenbeck, and E.C.Stone. > 25 MeV proton events observed by the High Energy Telescopes on the STEREO A and B spacecraft and/or at Earth during the first seven years of the STEREO mission. Sol. Phys., 289, 3059–3107, 2014, DOI: 10.1007/s11207-014-0524-8. [NASA ADS] [CrossRef]
  • Smart, D.F., and M.A.Shea. Modeling the time-intensity profile of solar flare generated particle fluxes in the inner heliosphere. Adv. Space Res., 12, 303–312, 1992, DOI: 10.1016/0273-1177(92)90120-M. [CrossRef]
  • Souvatzoglou, G., A.Papaioannou, H.Mavromichalaki, J.Dimitroulakos, and C.Sarlanis. Optimizing the real-time ground level enhancement alert system based on neutron monitor measurements: introducing GLE alert plus. Space Weather, 12, 633–649, 2014, DOI: 10.1002/2014SW001102. [CrossRef]
  • Torii, C., Y.Tsukiji, S.Kobayashi, N.Yoshimi, H.Tanaka, and S.Enome. Full-automatic radiopolarimeters for solar patrol at microwave frequencies. Proc. Res. Inst. Atmos., Nagoya Univ., 26, 129–132, 1979.

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