| The solar energetic particle event on 2013 April 11: an investigation of its solar origin and longitudinal spread D Lario, NE Raouafi, RY Kwon, J Zhang, R Gómez-Herrero, N Dresing, ... The Astrophysical Journal 797 (1), 8, 2014 | 90 | 2014 |
| Understanding the physical nature of coronal “EIT waves” DM Long, DS Bloomfield, PF Chen, C Downs, PT Gallagher, RY Kwon, ... Solar physics 292 (1), 7, 2017 | 87 | 2017 |
| Longitudinal properties of a widespread solar energetic particle event on 2014 February 25: evolution of the associated CME shock D Lario, RY Kwon, A Vourlidas, NE Raouafi, DK Haggerty, GC Ho, ... The Astrophysical Journal 819 (1), 72, 2016 | 87 | 2016 |
| New insights into the physical nature of coronal mass ejections and associated shock waves within the framework of the three-dimensional structure RY Kwon, J Zhang, O Olmedo The Astrophysical Journal 794 (2), 148, 2014 | 81 | 2014 |
| STEREO observations of fast magnetosonic waves in the extended solar corona associated with EIT/EUV waves RY Kwon, L Ofman, O Olmedo, M Kramar, JM Davila, BJ Thompson, ... The Astrophysical Journal 766 (1), 55, 2013 | 62 | 2013 |
| Relationship between multiple type II solar radio bursts and CME observed by STEREO/SECCHI KS Cho, SC Bong, YJ Moon, A Shanmugaraju, RY Kwon, YD Park Astronomy & Astrophysics 530, A16, 2011 | 60 | 2011 |
| The solar energetic particle event of 2010 August 14: Connectivity with the solar source inferred from multiple spacecraft observations and modeling D Lario, RY Kwon, IG Richardson, NE Raouafi, BJ Thompson, ... The Astrophysical Journal 838 (1), 51, 2017 | 51 | 2017 |
| A high-frequency type II solar radio burst associated with the 2011 February 13 coronal mass ejection KS Cho, N Gopalswamy, RY Kwon, RS Kim, S Yashiro The Astrophysical Journal 765 (2), 148, 2013 | 44 | 2013 |
| Investigating the wave nature of the outer envelope of halo coronal mass ejections RY Kwon, A Vourlidas The Astrophysical Journal 836 (2), 246, 2017 | 40 | 2017 |
| Determination of the heliospheric radial magnetic field from the standoff distance of a CME-driven shock observed by the STEREO spacecraft W Poomvises, N Gopalswamy, S Yashiro, RY Kwon, O Olmedo The Astrophysical Journal 758 (2), 118, 2012 | 40 | 2012 |
| The density compression ratio of shock fronts associated with coronal mass ejections RY Kwon, A Vourlidas Journal of Space Weather and Space Climate 8, A08, 2018 | 37 | 2018 |
| Are halo-like solar coronal mass ejections merely a matter of geometric projection effects? RY Kwon, J Zhang, A Vourlidas The Astrophysical Journal Letters 799 (2), L29, 2015 | 37 | 2015 |
| On the link between the release of solar energetic particles measured at widespread heliolongitudes and the properties of the associated coronal shocks D Lario, RY Kwon, P Riley, NE Raouafi The Astrophysical Journal 847 (2), 103, 2017 | 35 | 2017 |
| Global coronal seismology in the extended solar corona through fast magnetosonic waves observed by STEREO SECCHI COR1 RY Kwon, M Kramar, T Wang, L Ofman, JM Davila, J Chae, J Zhang The Astrophysical Journal 776 (1), 55, 2013 | 32 | 2013 |
| Validation of global EUV wave MHD simulations and observational techniques C Downs, A Warmuth, DM Long, DS Bloomfield, RY Kwon, AM Veronig, ... The Astrophysical Journal 911 (2), 118, 2021 | 28 | 2021 |
| The first widespread solar energetic particle event of solar cycle 25 on 2020 November 29-Shock wave properties and the wide distribution of solar energetic particles A Kouloumvakos, RY Kwon, L Rodríguez-García, D Lario, N Dresing, ... Astronomy & Astrophysics 660, A84, 2022 | 27 | 2022 |
| Stereoscopic determination of heights of extreme ultraviolet bright points using data taken by SECCHI/EUVI aboard STEREO RY Kwon, J Chae, J Zhang The Astrophysical Journal 714 (1), 130, 2010 | 23 | 2010 |
| Direct first parker solar probe observation of the interaction of two successive interplanetary coronal mass ejections in 2020 November T Nieves-Chinchilla, N Alzate, H Cremades, L Rodríguez-García, ... The Astrophysical Journal 930 (1), 88, 2022 | 19 | 2022 |
| Three-dimensional structure and evolution of extreme-ultraviolet bright points observed by STEREO/SECCHI/EUVI RY Kwon, J Chae, JM Davila, J Zhang, YJ Moon, W Poomvises, SI Jones The Astrophysical Journal 757 (2), 167, 2012 | 17 | 2012 |
| Evidence for a Magnetic Reconnection Origin of Plasma Outflows along Post-CME Rays J Chae, K Cho, RY Kwon, EK Lim The Astrophysical Journal 841 (1), 49, 2017 | 16 | 2017 |
david larioThe Johns Hopkins University. Applied Physics LaboratoryVerified email at jhuapl.edu
