SH012
Particle Acceleration and Transport at the Sun and in the Inner Heliosphere II

Tuesday, 8 December 2020: 05:30-06:30
Virtual
Primary Convener:  Linghua Wang, Peking University, Beijing, China
Conveners:  Gang Li, PLA University of Science and Technology, Nanjing, China and Robert F Wimmer-Schweingruber, University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany
Primary Liaison:  Linghua Wang, Peking University, Beijing, China
Chairs:  Linghua Wang, Peking University, Beijing, China, Gang Li, PLA University of Science and Technology, Nanjing, China and Robert F Wimmer-Schweingruber, University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany
OSPA Liaison:  Linghua Wang, Peking University, Beijing, China
05:30
SH012-01
Energetic Particles Observations Near the Sun from the Integrated Science Investigation of the Sun (ISʘIS) Instrument Suite on Parker Solar Probe (765725)
Eric R Christian1, David J McComas2, Nathan Schwadron3, Christina Cohen4, Alan C Cummings5, Andrew Davis6, Georgia Adair de Nolfo1, Mihir Indrajit Desai7, Joe Giacalone8, Matthew E Hill9, Colin Joyce2, Stamatios Mike Krimigis10, Allan Wayne Labrador11, Richard A Leske5, William H Matthaeus12, Ralph L McNutt Jr13, Richard Mewaldt14, Donald G Mitchell9, J. Grant Mitchell1, Jamie Sue Rankin15, Edmond C Roelof9, Edward C Stone14, Jamey R Szalay2 and Mark E Wiedenbeck16, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (3)University of New Hampshire, Durham, NH, United States, (4)Caltech, Pasadena, CA, United States, (5)CALTECH, Pasadena, CA, United States, (6)California Institute of Technology, Pasadena, United States, (7)Southwest Research Institute, San Antonio, TX, United States, (8)University of Arizona, Planetary Sciences, Tucson, AZ, United States, (9)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (10)Applied Physics Laboratory Johns Hopkins, Space, Laurel, MD, United States, (11)Mail Code 290-17, Pasadena, CA, United States, (12)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (13)Johns Hopkins Univ/APL, Laurel, MD, United States, (14)California Institute of Technology, Pasadena, CA, United States, (15)Princeton University, Princeton, NJ, United States, (16)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
05:34
Q&A
05:38
SH012-02
Statistical Analysis of the Relation between Coronal Mass Ejections and Solar Energetic Particles (677688)
Kosuke Kihara1, Nariaki Nitta2, Seiji Yashiro3, Ayumi Asai1 and Kiyoshi Ichimoto1, (1)Kyoto University, Kyoto, Japan, (2)Lockheed Martin Advanced Technology Center, Palo Alto, CA, United States, (3)Catholic University of America, Washington, DC, United States
05:42
Q&A
05:44
SH012-03
Coronal Acceleration of Large and Acute SEP Events (668343)
Matthew Young1, Nathan Schwadron2, Matthew Gorby2, Jon Linker3, Ronald M. Caplan3, Cooper Downs3, Tibor Torok4, Pete Riley4, Roberto Lionello3, Viacheslav S. Titov3, Richard Mewaldt5 and Christina Cohen6, (1)University of New Hampshire Main Campus, Durham, NH, United States, (2)University of New Hampshire, Durham, NH, United States, (3)Predictive Science Inc., San Diego, CA, United States, (4)Predictive Science, Inc., San Diego, CA, United States, (5)California Institute of Technology, Pasadena, CA, United States, (6)Caltech, Pasadena, CA, United States
05:48
Q&A
05:50
SH012-04
How does the state of the overlying solar corona influence SEP acceleration in CME-driven shocks? (735247)
Kamen A Kozarev1, Rositsa Miteva1, Mohamed Nedal1, Pietro Zucca2 and Momchil Dechev1, (1)Institute of Astronomy, Bulgarian Academy of Sciences, Sofia, Bulgaria, (2)ASTRON, Dwingeloo, Netherlands
05:54
Q&A
05:56
SH012-05
The Acceleration of Energetic Particles at Coronal Shocks and Q/A Dependence of Spectral Breaks (721554)
Xiangliang Kong, Shandong University, Jinan, China, Feiyu Yu, Shandong University, Weihai, China, Fan Guo, Los Alamos National Lab, Los Alamos, NM, United States, Yao Chen, Shandong Univ. at Weihai, Weihai, Shandong, China and Joe Giacalone, University of Arizona, Planetary Sciences, Tucson, AZ, United States
06:00
Q&A
06:02
SH012-06
Non-Markovian Pitch-Angle Scattering as the Origin of Particle Superdiffusive Transport Parallel to the Average Magnetic Field (674465)
Gaetano Zimbardo, University of Calabria, Calabria, Italy and Silvia Perri, Dipartimento di Fisica, Fisica, Arcavacata di Rende, Italy
06:06
Q&A
06:08
SH012-07
A Fractional Kinetic Transport Theory for Energetic Particle Acceleration and Propagation in Dynamic Small-scale Flux Rope Regions in the Solar Wind. (700254)
Jakobus Albertus le Roux, University of Alabama in Huntsville, Huntsville, AL, United States, Gary Paul Zank, Univ of Alabama, Huntsville, Huntsville, AL, United States, Senbei Du, University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States and Gary M Webb, Univ of Alabama, Huntsville, AL, United States
06:12
Q&A
06:14
SH012-08
High-Energy Proton Intensity Enhancements Associated with the Passage of Interplanetary Shocks (683248)
David Lario1 and Ian G Richardson1,2, (1)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, (2)University of Maryland College Park, Department of Astronomy, College Park, MD, United States
06:18
Q&A
06:20
SH012-09
First Solar Energetic Particles Measured On The Lunar Far-side (681513)
Zigong Xu1, Jingnan Guo2,3, Robert F Wimmer-Schweingruber4, Johan Lauritz Freiherr von Forstner4, Henning Lohf5, Yuming Wang2, Nina Dresing6, Shenyi Zhang7 and Bernd Heber5, (1)University of Kiel, Institute of Experimental and Applied Physics, Kiel, Germany, (2)University of Science and Technology of China, Hefei, China, (3)University of Science and Technology of China, School of Earth and Space Sciences, Hefei, China, (4)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (5)University of Kiel, Kiel, Germany, (6)IEAP University of Kiel, Kiel, Germany, (7)NSSC National Space Science Center, CAS, Beijing, China
06:24
Q&A
06:26
Discussion
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