Modelling the magnetic structure of a large-scale horse-shoe-like filament in a decaying and diffuse active region

Autor: Kaifeng Kang, Yang Guo, Ilia I Roussev, Rony Keppens, Jun Lin

Publikováno v: Monthly Notices of the Royal Astronomical Society. 518:388-404

A large-scale, horse-shoe-like filament was investigated and the magnetic field around it was reconstructed. This is an intermediate filament (IF) that appeared on the solar disk for the first time at 02:00 UT on 2015 November 7, and took 8 days to m

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a25d1bfc1a8307f21e10e03719dcd5e
https://doi.org/10.1093/mnras/stac3156

Review of solar energetic particle models

Autor: Kathryn Whitman, Ricky Egeland, Ian G. Richardson, Clayton Allison, Philip Quinn, Janet Barzilla, Irina Kitiashvili, Viacheslav Sadykov, Hazel M. Bain, Mark Dierckxsens, M. Leila Mays, Tilaye Tadesse, Kerry T. Lee, Edward Semones, Janet G. Luhmann, Marlon Núñez, Stephen M. White, Stephen W. Kahler, Alan G. Ling, Don F. Smart, Margaret A. Shea, Valeriy Tenishev, Soukaina F. Boubrahimi, Berkay Aydin, Petrus Martens, Rafal Angryk, Michael S. Marsh, Silvia Dalla, Norma Crosby, Nathan A. Schwadron, Kamen Kozarev, Matthew Gorby, Matthew A. Young, Monica Laurenza, Edward W. Cliver, Tommaso Alberti, Mirko Stumpo, Simone Benella, Athanasios Papaioannou, Anastasios Anastasiadis, Ingmar Sandberg, Manolis K. Georgoulis, Anli Ji, Dustin Kempton, Chetraj Pandey, Gang Li, Junxiang Hu, Gary P. Zank, Eleni Lavasa, Giorgos Giannopoulos, David Falconer, Yash Kadadi, Ian Fernandes, Maher A. Dayeh, Andrés Muñoz-Jaramillo, Subhamoy Chatterjee, Kimberly D. Moreland, Igor V. Sokolov, Ilia I. Roussev, Aleksandre Taktakishvili, Frederic Effenberger, Tamas Gombosi, Zhenguang Huang, Lulu Zhao, Nicolas Wijsen, Angels Aran, Stefaan Poedts, Athanasios Kouloumvakos, Miikka Paassilta, Rami Vainio, Anatoly Belov, Eugenia A. Eroshenko, Maria A. Abunina, Artem A. Abunin, Christopher C. Balch, Olga Malandraki, Michalis Karavolos, Bernd Heber, Johannes Labrenz, Patrick Kühl, Alexander G. Kosovichev, Vincent Oria, Gelu M. Nita, Egor Illarionov, Patrick M. O’Keefe, Yucheng Jiang, Sheldon H. Fereira, Aatiya Ali, Evangelos Paouris, Sigiava Aminalragia-Giamini, Piers Jiggens, Meng Jin, Christina O. Lee, Erika Palmerio, Alessandro Bruno, Spiridon Kasapis, Xiantong Wang, Yang Chen, Blai Sanahuja, David Lario, Carla Jacobs, Du Toit Strauss, Ruhann Steyn, Jabus van den Berg, Bill Swalwell, Charlotte Waterfall, Mohamed Nedal, Rositsa Miteva, Momchil Dechev, Pietro Zucca, Alec Engell, Brianna Maze, Harold Farmer, Thuha Kerber, Ben Barnett, Jeremy Loomis, Nathan Grey, Barbara J. Thompson, Jon A. Linker, Ronald M. Caplan, Cooper Downs, Tibor Török, Roberto Lionello, Viacheslav Titov, Ming Zhang, Pouya Hosseinzadeh

Publikováno v: Advances in Space Research.

Solar Energetic Particles (SEP) events are interesting from a scientific perspective as they are the product of a broad set of physical processes from the corona out through the extent of the heliosphere, and provide insight into processes of particl

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b67272d272fda020c5397d3a5545985b
https://doi.org/10.1016/j.asr.2022.08.006

Numerical simulations of shear-induced consecutive coronal mass ejections

Autor: Marilena Mierla, Skralan Hosteaux, Ilia I. Roussev, Dana-Camelia Talpeanu, Stefaan Poedts, Emmanuel Chané, Elke D'Huys

Methods: Stealth CMEs represent a particular class of solar eruptions that are clearly distinguished in coronagraph observations, but they don't have a clear source signature. A particular type of stealth CMEs occurs in the trailing current sheet of

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e120978d769014ee0e4dcd8f103d0d28
https://lirias.kuleuven.be/handle/123456789/653360

OUP accepted manuscript

Autor: Zhixing Mei, Xiaoyan Xie, Huang Min, Qunbo Lv, Ilia I. Roussev, Jun Lin

Publikováno v: Monthly Notices of the Royal Astronomical Society.

Based on the catastrophe model of the solar eruption, we explore the disturbances caused by solar eruptions via numerical experiments, with special attention given to large-scale waves. In addition to the phenomena shown by previous works, a new stru

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::224638414b92cb97f6f66592ad9f03e8
https://doi.org/10.1093/mnras/stz2576

Toward Quantitative Model for Simulation and Forecast of Solar Energetic Particles Production during Gradual Events - I: Magnetohydrodynamic Background Coupled to the SEP Model

Autor: A. Taktakishvili, Tamas I. Gombosi, Ilia I. Roussev, D. Borovikov, Igor Sokolov

Solar Energetic Particles (SEPs) are an important aspect of space weather. SEP events posses a high destructive potential, since they may cause disruptions of communication systems on Earth and be fatal to crew members onboard spacecrafts and, in ext

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::25fa73514ab91ee2abb231c4acc8a260
http://arxiv.org/abs/1806.07030