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• W4380051310 endingPage "35" @default.
• W4380051310 startingPage "35" @default.
• W4380051310 abstract "In an effort to develop computational tools for predicting radiation hazards from solar energetic particles (SEPs), we have created a data-driven physics-based particle transport model to calculate the injection, acceleration and propagation of SEPs from coronal mass ejection (CME) shocks traversing through the solar corona and interplanetary magnetic fields. The model runs on an input of corona and heliospheric plasma and magnetic field configuration from an MHD model driven by solar photospheric magnetic field measurements superposed with observed CME shocks determined from coronagraph images. Using several advanced computation techniques involving stochastic simulation and integration, it rigorously solves the time-dependent 5-dimensional focus transport equation in the phase space that includes pitch-angle scattering, diffusion across magnetic field line, and particle acceleration by CME shocks. We apply the model to the 2011 November 3 CME event. The calculation results reproduce multi-spacecraft SEP observations reasonably well without normalization of particle flux. This circumsolar SEP event seen by spacecraft at Earth, STEREO-A and STEREO-B at widely separated longitudes can be explained by diffusive shock acceleration by a single CME shock with a moderate speed." @default.
• W4380051310 created "2023-06-10" @default.
• W4380051310 creator A5003575459 @default.
• W4380051310 creator A5010179711 @default.
• W4380051310 creator A5010299185 @default.
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• W4380051310 creator A5027629446 @default.
• W4380051310 creator A5030266079 @default.
• W4380051310 creator A5035201812 @default.
• W4380051310 creator A5048788887 @default.
• W4380051310 date "2023-06-01" @default.
• W4380051310 modified "2023-10-16" @default.
• W4380051310 title "A Data-driven, Physics-based Transport Model of Solar Energetic Particles Accelerated by Coronal Mass Ejection Shocks Propagating through the Solar Coronal and Heliospheric Magnetic Fields" @default.
• W4380051310 cites W1658899696 @default.
• W4380051310 cites W1873216632 @default.
• W4380051310 cites W1927992296 @default.
• W4380051310 cites W1963701191 @default.
• W4380051310 cites W1966109696 @default.
• W4380051310 cites W1966508007 @default.
• W4380051310 cites W1968400135 @default.
• W4380051310 cites W1975421256 @default.
• W4380051310 cites W1976316526 @default.
• W4380051310 cites W1977841716 @default.
• W4380051310 cites W1978090441 @default.
• W4380051310 cites W1978572776 @default.
• W4380051310 cites W1979831902 @default.
• W4380051310 cites W1983941642 @default.
• W4380051310 cites W1986463499 @default.
• W4380051310 cites W1989488695 @default.
• W4380051310 cites W1991626520 @default.
• W4380051310 cites W1992150388 @default.
• W4380051310 cites W2001008513 @default.
• W4380051310 cites W2001833979 @default.
• W4380051310 cites W2003110235 @default.
• W4380051310 cites W2006234711 @default.
• W4380051310 cites W2009842141 @default.
• W4380051310 cites W2010409066 @default.
• W4380051310 cites W2013994742 @default.
• W4380051310 cites W2014292057 @default.
• W4380051310 cites W2018632743 @default.
• W4380051310 cites W2018819045 @default.
• W4380051310 cites W2018827598 @default.
• W4380051310 cites W2029955914 @default.
• W4380051310 cites W2032882333 @default.
• W4380051310 cites W2041278067 @default.
• W4380051310 cites W2042192850 @default.
• W4380051310 cites W2049440614 @default.
• W4380051310 cites W2049957901 @default.
• W4380051310 cites W2054796185 @default.
• W4380051310 cites W2055711645 @default.
• W4380051310 cites W2057002746 @default.
• W4380051310 cites W2064221922 @default.
• W4380051310 cites W2067277085 @default.
• W4380051310 cites W2067499111 @default.
• W4380051310 cites W2068284534 @default.
• W4380051310 cites W2074798192 @default.
• W4380051310 cites W2085184639 @default.
• W4380051310 cites W2086329925 @default.
• W4380051310 cites W2086425040 @default.
• W4380051310 cites W2087364146 @default.
• W4380051310 cites W2090959428 @default.
• W4380051310 cites W2091421803 @default.
• W4380051310 cites W2094483427 @default.
• W4380051310 cites W2095030524 @default.
• W4380051310 cites W2095295189 @default.
• W4380051310 cites W2100369045 @default.
• W4380051310 cites W2108345010 @default.
• W4380051310 cites W2109690032 @default.
• W4380051310 cites W2110976562 @default.
• W4380051310 cites W2111078819 @default.
• W4380051310 cites W2127112787 @default.
• W4380051310 cites W2134801226 @default.
• W4380051310 cites W2150886504 @default.
• W4380051310 cites W2155776578 @default.
• W4380051310 cites W2169996752 @default.
• W4380051310 cites W2170892989 @default.
• W4380051310 cites W2531566725 @default.
• W4380051310 cites W2583450549 @default.
• W4380051310 cites W2589486709 @default.
• W4380051310 cites W2751433178 @default.
• W4380051310 cites W2760520718 @default.
• W4380051310 cites W2806372425 @default.
• W4380051310 cites W2919878451 @default.
• W4380051310 cites W2944134073 @default.
• W4380051310 cites W2964036261 @default.
• W4380051310 cites W3098399176 @default.
• W4380051310 cites W3101472739 @default.
• W4380051310 cites W3101938487 @default.
• W4380051310 cites W3102375159 @default.
• W4380051310 cites W3121481239 @default.
• W4380051310 cites W3125945692 @default.
• W4380051310 cites W3201668206 @default.
• W4380051310 cites W4206376982 @default.
• W4380051310 cites W4210713059 @default.
• W4380051310 cites W4214566275 @default.
• W4380051310 cites W4255988644 @default.
• W4380051310 cites W4281492990 @default.
• W4380051310 cites W4291109640 @default.

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