Zobrazeno 1 - 10
of 42
pro vyhledávání: '"Ryun Young Kwon"'
Autor:
Ming Zhang, Lei Cheng, Ju Zhang, Pete Riley, Ryun Young Kwon, David Lario, Laura Balmaceda, Nikolai V. Pogorelov
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 266, Iss 2, p 35 (2023)
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
Externí odkaz:
https://doaj.org/article/f5fa0f89a4b044a58e79bd0ed97e36e1
Publikováno v:
The Astrophysical Journal, Vol 943, Iss 2, p 134 (2023)
This paper presents a stochastic three-dimensional focused transport simulation of solar energetic particles (SEPs) produced by a data-driven coronal mass ejection (CME) shock propagating through a data-driven model of coronal and heliospheric magnet
Externí odkaz:
https://doaj.org/article/dc034308d09f48a795496e853c71e385
Autor:
Young-Sil Kwak, Jeong-Heon Kim, Sujin Kim, Yukinaga Miyashita, Taeyong Yang, Sung-Hong Park, Eun-Kyung Lim, Jongil Jung, Hosik Kam, Jaewook Lee, Hwanhee Lee, Ji-Hyun Yoo, Haein Lee, Ryun-Young Kwon, Jungjoon Seough, Uk-Won Nam, Woo Kyoung Lee, Junseok Hong, Jongdae Sohn, Jaeyoung Kwak, Hannah Kwak, Rok-Soon Kim, Yeon-Han Kim, Kyung-Suk Cho, Jaeheung Park, Jaejin Lee, Hoang Ngoc Huy Nguyen, Madeeha Talha
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 41, Iss 3, Pp 171-194 (2024)
This study reports comprehensive observations for the G5-level geomagnetic storm that occurred from May 10 to 12, 2024, the most intense event since the 2003 Halloween storm. The storm was triggered by a series of coronal mass ejections (CMEs) orig
Externí odkaz:
https://doaj.org/article/3348d31c3d7d4488b9edf511150a5f37
Autor:
Bin Zhuang, Noé Lugaz, David Lario, Ryun-Young Kwon, Nicolina Chrysaphi, Jonathan Niehof, Tingyu Gou, Lulu Zhao
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 2, p 119 (2024)
The main driver of the acceleration of solar energetic particles (SEPs) is believed to be shocks driven by coronal mass ejections. Extreme-ultraviolet (EUV) waves are thought to be the propagating footprint of the shock on the solar surface. One of t
Externí odkaz:
https://doaj.org/article/31a603a6b63f4f40825f2b2fbc6b89a3
This paper presents a stochastic three-dimensional (3D) focused transport simulation of solar energetic particles (SEPs) produced by a data-driven coronal mass ejection (CME) shock propagating through a data-driven model of coronal and heliospheric m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f4002207f2bf7263e23097c9358874a0
Publikováno v:
The Astrophysical Journal. 931:141
We analyze the formation and three-dimensional (3D) evolution of two coronal mass ejections (CMEs) and their associated waves in the low corona via a detailed multi-viewpoint analysis of extreme-ultraviolet observations. We analyze the kinematics in
Autor:
Ryun Young Kwon
We present a novel method to derive the shock density compression ratio of coronal shock waves that are occasionally observed as halo coronal mass ejections (CMEs). Our method uses the three-dimensional (3-D) geometry and enables us to access the rel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c92b70731e036d03ccceedd87d8d97d5
https://doi.org/10.5194/egusphere-egu21-10578
https://doi.org/10.5194/egusphere-egu21-10578
Autor:
Bojan Vršnak, Astrid Veronig, Angelos Vourlidas, D. Shaun Bloomfield, Cooper Downs, David Long, Alexander Warmuth, Ryun-Young Kwon
Global EUV waves remain a controversial phenomenon more than 20 yr after their discovery by SOHO/EIT. Although consensus is growing in the community that they are most likely large-amplitude waves or shocks, the wide variety of observations and techn
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3179829bde34764e122a61a300cc32bd
https://www.bib.irb.hr/1127576
https://www.bib.irb.hr/1127576
Autor:
Teresa Nieves-Chinchilla, Nathalia Alzate, Hebe Cremades, Laura Rodríguez-García, Luiz F. G. Dos Santos, Ayris Narock, Hong Xie, Adam Szabo, Erika Palmerio, Vratislav Krupar, Marc Pulupa, David Lario, Michael L. Stevens, Lynn B. Wilson, Ryun-Young Kwon, M. Leila Mays, O. Chris St. Cyr, Phillip Hess, Katharine K. Reeves, Daniel B. Seaton, Tatiana Niembro, Stuart D. Bale, Justin C. Kasper
Publikováno v:
The Astrophysical Journal. 930:88
We investigate the effects of the evolutionary processes in the internal magnetic structure of two interplanetary coronal mass ejections (ICMEs) detected in situ between 2020 November 29 and December 1 by the Parker Solar Probe (PSP). The sources of
Autor:
Stefaan Poedts, Ryun-Young Kwon, Brigitte Schmieder, Benjamin Grison, Pascal Démoulin, Karine Bocchialini, Rok-Soon Kim
Publikováno v:
Journal of Geophysical Research Space Physics
Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2020, 125 (6), ⟨10.1029/2019JA027529⟩
Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2020, 125 (6), ⟨10.1029/2019JA027529⟩
It is generally accepted that extreme space weather events tend to be related to strong flares and fast halo coronal mass ejections CMEs. In the present paper, we carefully identify the chain of events from the Sun to the Earth induced by all 12 X-cl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::976ccf4fe115cea96e97a24f53b254b4
https://hal.sorbonne-universite.fr/hal-03002008
https://hal.sorbonne-universite.fr/hal-03002008