Zobrazeno 1 - 10
of 81
pro vyhledávání: '"Titov Viacheslav A."'
Autor:
Hrudkina Natalia S., Markov Oleg E., Shapoval Alexander A., Titov Viacheslav A., Aliiev Igramotdin S., Abhari Payman, Malii Khrystyna V.
Publikováno v:
FME Transactions, Vol 50, Iss 1, Pp 90-98 (2022)
The article is considered a comparative analysis for predicting defect such as dimple by energy method of power balance, upper bound method and finite element method. The upper bound method takes into account the geometrical position and dimension of
Externí odkaz:
https://doaj.org/article/c25d297bca2447c990598a6c27749da1
Autor:
Linker, Jon, Torok, Tibor, Downs, Cooper, Caplan, Ronald, Titov, Viacheslav, Reyes, Andres, Lionello, Roberto, Riley, Pete
Coronal Mass Ejections (CMEs) are immense eruptions of plasma and magnetic fields that are propelled outward from the Sun, sometimes with velocities greater than 2000 km/s. They are responsible for some of the most severe space weather at Earth, incl
Externí odkaz:
http://arxiv.org/abs/2311.03596
Autor:
Ben-Nun, Michal, Török, Tibor, Palmerio, Erika, Downs, Cooper, Titov, Viacheslav S., Linton, Mark G., Caplan, Ronald M., Lionello, Roberto
The trajectories of coronal mass ejections (CMEs) are often seen to substantially deviate from a purely radial propagation direction. Such deviations occur predominantly in the corona and have been attributed to "channeling" or deflection of the erup
Externí odkaz:
http://arxiv.org/abs/2310.02412
Autor:
Lionello, Roberto, Downs, Cooper, Mason, Emily I., Linker, Jon A., Caplan, Ronald M., Riley, Pete, Titov, Viacheslav S., DeRosa, Marc L.
We describe, test, and apply a technique to incorporate full-sun, surface flux evolution into an MHD model of the global solar corona. Requiring only maps of the evolving surface flux, our method is similar to that of Lionello et al. (2013), but we i
Externí odkaz:
http://arxiv.org/abs/2306.12551
We propose a new ``helicity-pumping'' method for energizing coronal equilibria that contain a magnetic flux rope (MFR) toward an eruption. We achieve this in a sequence of magnetohydrodynamics relaxations of small line-tied pulses of magnetic helicit
Externí odkaz:
http://arxiv.org/abs/2205.03982
Autor:
Young, Matthew A., Schwadron, Nathan A., Gorby, Matthew, Linker, Jon, Caplan, Ronald M., Downs, Cooper, Török, Tibor, Riley, Pete, Lionello, Roberto, Titov, Viacheslav, Mewaldt, Richard A., Cohen, Christina M. S.
This work presents results from simulations of the 14 July 2000 ("Bastille Day") solar proton event. We used the Energetic Particle Radiation Environment Model (EPREM) and the CORona-HELiosphere (CORHEL) software suite within the SPE Threat Assessmen
Externí odkaz:
http://arxiv.org/abs/2012.09078
Autor:
Whitman, Kathryn, Egeland, Ricky, Richardson, Ian G., Allison, Clayton, Quinn, Philip, Barzilla, Janet, Kitiashvili, Irina, Sadykov, Viacheslav, Bain, Hazel M., Dierckxsens, Mark, Mays, M. Leila, Tadesse, Tilaye, Lee, Kerry T., Semones, Edward, Luhmann, Janet G., Núñez, Marlon, White, Stephen M., Kahler, Stephen W., Ling, Alan G., Smart, Don F., Shea, Margaret A., Tenishev, Valeriy, Boubrahimi, Soukaina F., Aydin, Berkay, Martens, Petrus, Angryk, Rafal, Marsh, Michael S., Dalla, Silvia, Crosby, Norma, Schwadron, Nathan A., Kozarev, Kamen, Gorby, Matthew, Young, Matthew A., Laurenza, Monica, Cliver, Edward W., Alberti, Tommaso, Stumpo, Mirko, Benella, Simone, Papaioannou, Athanasios, Anastasiadis, Anastasios, Sandberg, Ingmar, Georgoulis, Manolis K., Ji, Anli, Kempton, Dustin, Pandey, Chetraj, Li, Gang, Hu, Junxiang, Zank, Gary P., Lavasa, Eleni, Giannopoulos, Giorgos, Falconer, David, Kadadi, Yash, Fernandes, Ian, Dayeh, Maher A., Muñoz-Jaramillo, Andrés, Chatterjee, Subhamoy, Moreland, Kimberly D., Sokolov, Igor V., Roussev, Ilia I., Taktakishvili, Aleksandre, Effenberger, Frederic, Gombosi, Tamas, Huang, Zhenguang, Zhao, Lulu, Wijsen, Nicolas, Aran, Angels, Poedts, Stefaan, Kouloumvakos, Athanasios, Paassilta, Miikka, Vainio, Rami, Belov, Anatoly, Eroshenko, Eugenia A., Abunina, Maria A., Abunin, Artem A., Balch, Christopher C., Malandraki, Olga, Karavolos, Michalis, Heber, Bernd, Labrenz, Johannes, Kühl, Patrick, Kosovichev, Alexander G., Oria, Vincent, Nita, Gelu M., Illarionov, Egor, O’Keefe, Patrick M., Jiang, Yucheng, Fereira, Sheldon H., Ali, Aatiya, Paouris, Evangelos, Aminalragia-Giamini, Sigiava, Jiggens, Piers, Jin, Meng, Lee, Christina O., Palmerio, Erika, Bruno, Alessandro, Kasapis, Spiridon, Wang, Xiantong, Chen, Yang, Sanahuja, Blai, Lario, David, Jacobs, Carla, Strauss, Du Toit, Steyn, Ruhann, van den Berg, Jabus, Swalwell, Bill, Waterfall, Charlotte, Nedal, Mohamed, Miteva, Rositsa, Dechev, Momchil, Zucca, Pietro, Engell, Alec, Maze, Brianna, Farmer, Harold, Kerber, Thuha, Barnett, Ben, Loomis, Jeremy, Grey, Nathan, Thompson, Barbara J., Linker, Jon A., Caplan, Ronald M., Downs, Cooper, Török, Tibor, Lionello, Roberto, Titov, Viacheslav, Zhang, Ming, Hosseinzadeh, Pouya
Publikováno v:
In Advances in Space Research 15 December 2023 72(12):5161-5242
Autor:
Lin, Longfei, Peng, Wenfei, Zhu, Shuai, Wu, Zhijun, Zhu, Jian, Shao, Yiyu, Li, He, Oleksandr, Moliar, Titov, Viacheslav
Publikováno v:
In Journal of Materials Processing Tech. August 2023 317
Publikováno v:
In Journal of Materials Research and Technology May-June 2023 24:1132-1149
Autor:
Török, Tibor, Downs, Cooper, Linker, Jon A., Lionello, Roberto, Titov, Viacheslav S., Mikić, Zoran, Riley, Pete, Caplan, Ron M., Wijaya, Janvier
Solar eruptions are the main driver of space-weather disturbances at the Earth. Extreme events are of particular interest, not only because of the scientific challenges they pose, but also because of their possible societal consequences. Here we pres
Externí odkaz:
http://arxiv.org/abs/1801.05903