Solar energetic particles in the inner heliosphere: status and open questions

被引:48
作者
Anastasiadis, Anastasios [1 ]
Lario, David [2 ]
Papaioannou, Athanasios [1 ]
Kouloumvakos, Athanasios [3 ]
Vourlidas, Angelos [1 ,4 ]
机构
[1] Natl Observ Athens, IAASARS, I Metaxa & Vas Pavlou St, Penteli 15236, Greece
[2] NASA, Heliophys Sci Div, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Univ Toulouse III Paul Sabatier, CNES, CNRS, IRAP, Toulouse, France
[4] Johns Hopkins Univ, Appl Phys Lab, 11100 Johns Hopkins Rd, Laurel, MD 20723 USA
来源
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES | 2019年 / 377卷 / 2148期
关键词
solar energetic particles; solar flares; coronal mass ejections; GROUND-LEVEL ENHANCEMENT; CORONAL MASS EJECTIONS; PROTON EVENTS; INTERPLANETARY SHOCKS; FORECASTING METHODS; SPACE WEATHER; RELEASE TIMES; SEP EVENTS; CYCLE; 24; ACCELERATION;
D O I
10.1098/rsta.2018.0100
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Solar energetic particle (SEP) events are related to both solar flares and coronal mass ejections (CMEs) and they present energy spectra that span from a few keV up to several GeV. A wealth of observations from widely distributed spacecraft have revealed that SEPs fill very broad regions of the heliosphere, often all around the Sun. Highenergy SEPs can sometimes be energetic enough to penetrate all the way down to the surface of the Earth and thus be recorded on the ground as ground level enhancements (GLEs). The conditions of the radiation environment are currently unpredictable due to an as-yet incomplete understanding of solar eruptions and their corresponding relation to SEP events. This is because the complex nature and the interplay of the injection, acceleration and transport processes undergone by the SEPs in the solar corona and the interplanetary space prevent us from establishing an accurate understanding (based on observations and modelling). In this work, we review the current status of knowledge on SEPs, focusing on GLEs and multi-spacecraft events. We extensively discuss the forecasting and nowcasting efforts of SEPs, dividing these into three categories. Finally, we report on the current open questions and the possible direction of future research efforts. This article is part of the theme issue 'Solar eruptions and their space weather impact'.
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页数:19
相关论文
共 149 条
[1]   Modelling of proton acceleration in application to a ground level enhancement [J].
Afanasiev, A. ;
Vainio, R. ;
Rouillard, A. P. ;
Battarbee, M. ;
Aran, A. ;
Zucca, P. .
ASTRONOMY & ASTROPHYSICS, 2018, 614
[2]   Solar Activity from 2006 to 2014 and Short-term Forecasts of Solar Proton Events Using the ESPERTA Model [J].
Alberti, T. ;
Laurenza, M. ;
Cliver, E. W. ;
Storini, M. ;
Consolini, G. ;
Lepreti, F. .
ASTROPHYSICAL JOURNAL, 2017, 838 (01)
[3]   Predicting Flares and Solar Energetic Particle Events: The FORSPEF Tool [J].
Anastasiadis, A. ;
Papaioannou, A. ;
Sandberg, I. ;
Georgoulis, M. ;
Tziotziou, K. ;
Kouloumvakos, A. ;
Jiggens, P. .
SOLAR PHYSICS, 2017, 292 (09)
[4]   Comparing proton fluxes of central meridian SEP events with those predicted by SOLPENCO [J].
Aran, A. ;
Sanahuja, B. ;
Lario, D. .
ADVANCES IN SPACE RESEARCH, 2008, 42 (09) :1492-1499
[5]   SOLPENCO: A solar particle engineering code [J].
Aran, A. ;
Sanahuja, B. ;
Lario, D. .
SPACE WEATHER PREDICTION: APPLICATIONS AND VALIDATION, 2006, 37 (06) :1240-1246
[6]   Fluxes and fluences of SEP events derived from SOLPENCO [J].
Aran, A ;
Sanahuja, B ;
Lario, D .
ANNALES GEOPHYSICAE, 2005, 23 (09) :3047-3053
[7]   GeV Particle Acceleration in Solar Flares and Ground Level Enhancement (GLE) Events [J].
Aschwanden, Markus J. .
SPACE SCIENCE REVIEWS, 2012, 171 (1-4) :3-21
[8]   SEC proton prediction model: verification and analysis [J].
Balch, CC .
RADIATION MEASUREMENTS, 1999, 30 (03) :231-250
[9]   Updated verification of the Space Weather Prediction Center's solar energetic particle prediction model [J].
Balch, Christopher C. .
SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS, 2008, 6 (01)
[10]   Solar energetic particle events in 2006-2012 in the PAMELA experiment data [J].
Bazilevskaya, G. A. ;
Mayorov, A. G. ;
Malakhov, V. V. ;
Mikhailov, V. V. ;
Adriani ;
Barbarino, G. C. ;
Bellotti, R. ;
Boezio, M. ;
Bogomolov, E. A. ;
Bonechi, L. ;
Bongi, M. ;
Bonvicini, V. ;
Bottai, S. ;
Bruno, A. ;
Cafagna, F. ;
Campana, D. ;
Carbone, R. ;
Carlson, P. ;
Casolino, M. ;
Castellini, G. ;
Consiglio, L. ;
De Pascale, M. P. ;
De Santis, C. ;
De Simone, N. ;
Di Felice, V. ;
Galper, A. M. ;
Gillard, W. ;
Jerse, G. ;
Karelin, A. V. ;
Koldashov, S. V. ;
Krutkov, S. Y. ;
Kvashnin, A. N. ;
Leonov, A. ;
Marcelli, L. ;
Menn, W. ;
Mocchiutti, E. ;
Monaco, A. ;
Mori, N. ;
Osteria, G. ;
Palma, F. ;
Papini, P. ;
Pearce, M. ;
Picozza, P. ;
Pizzolotto, C. ;
Ricci, M. ;
Ricciarini, S. B. ;
Sarkar, R. ;
Rossetto, L. ;
Simon, M. ;
Sparvoli, R. .
23RD EUROPEAN COSMIC RAY SYMPOSIUM (AND 32ND RUSSIAN COSMIC RAY CONFERENCE), 2013, 409