Zobrazeno 1 - 10
of 169
pro vyhledávání: '"Farrugia, Charles J."'
Autor:
Scolini, Camilla, Lugaz, Noe, Winslow, Reka M., Farrugia, Charles J., Magyar, Norbert, Bacchini, Fabio
Interplanetary coronal mass ejections (ICMEs) are defined as ''coherent'' if they are capable of responding to external perturbations in a collective manner. This implies that information must be able to propagate across ICME structures, and if this
Externí odkaz:
http://arxiv.org/abs/2312.04480
Autor:
Lugaz, Noé, Zhuang, Bin, Scolini, Camilla, Al-Haddad, Nada, Farrugia, Charles J., Winslow, Réka M., Regnault, Florian, Möstl, Christian, Davies, Emma E., Galvin, Antoinette B.
Coronal mass ejections (CMEs) are large-scale eruptions with a typical radial size at 1 au of 0.21 au but their angular width in interplanetary space is still mostly unknown, especially for the magnetic ejecta (ME) part of the CME. We take advantage
Externí odkaz:
http://arxiv.org/abs/2312.03942
Autor:
Palmerio, Erika, Lynch, Benjamin J., Lee, Christina O., Jian, Lan K., Nieves-Chinchilla, Teresa, Davies, Emma E., Wood, Brian E., Lugaz, Noé, Winslow, Réka M., Török, Tibor, Al-Haddad, Nada, Regnault, Florian, Jin, Meng, Scolini, Camilla, Carcaboso, Fernando, Farrugia, Charles J., Ledvina, Vincent E., Downs, Cooper, Kay, Christina, Pal, Sanchita, Salman, Tarik M., Allen, Robert C.
Publikováno v:
Bulletin of the AAS, 55(3), 307, 2023
Coronal mass ejections (CMEs) are large eruptions from the Sun that propagate through the heliosphere after launch. Observational studies of these transient phenomena are usually based on 2D images of the Sun, corona, and heliosphere (remote-sensing
Externí odkaz:
http://arxiv.org/abs/2309.05480
Autor:
Zhuang, Bin, Lugaz, Noé, Al-Haddad, Nada, Winslow, Réka M., Scolini, Camilla, Farrugia, Charles J., Galvin, Antoinette B.
A fundamental property of coronal mass ejections (CMEs) is their radial expansion, which determines the increase in the CME radial size and the decrease in the CME magnetic field strength as the CME propagates. CME radial expansion can be investigate
Externí odkaz:
http://arxiv.org/abs/2305.14339
Autor:
Lugaz, Noé, Salman, Tarik M., Farrugia, Charles J., Yu, Wenyuan, Zhuang, Bin, Al-Haddad, Nada, Scolini, Camilla, Winslow, Réka M., Möstl, Christian, Davies, Emma E., Galvin, Antoinette B.
We present an analysis of {\it in situ} and remote-sensing measurements of a coronal mass ejection (CME) that erupted on 2021 February 20 and impacted both the Solar TErrestrial RElations Observatory (STEREO)-A and the {\it Wind} spacecraft, which we
Externí odkaz:
http://arxiv.org/abs/2203.16477
Autor:
Xu, Xiaojun, Lee, Lou-Chuang, Xu, Qi, Chang, Qing, Wang, Jing, Wang, Ming, Xu, Shaosui, Möstl, Christian, Farrugia, Charles J., Wang, Xing, Ye, Yudong, Zhou, Zilu, Luo, Lei, He, Peishan, Cheng, Shaoguan
Publikováno v:
In Fundamental Research July 2024 4(4):882-889
Akademický článek
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Autor:
Heinemann, Stephan G., Temmer, Manuela, Farrugia, Charles J., Dissauer, Karin, Kay, Christina, Wiegelmann, Thomas, Dumbović, Mateja, Veronig, Astrid M., Podladchikova, Tatiana, Hofmeister, Stefan J., Lugaz, Noé, Carcaboso, Fernando
In a thorough study, we investigate the origin of a remarkable plasma and magnetic field configuration observed in situ on June 22, 2011 near L1, which appears to be a magnetic ejecta (ME) and a shock signature engulfed by a solar wind high-speed str
Externí odkaz:
http://arxiv.org/abs/1908.10161
Autor:
Vršnak, Bojan, Amerstorfer, Tanja, Dumbović, Mateja, Leitner, Martin, Veronig, Astrid M., Temmer, Manuela, Möstl, Christian, Amerstorfer, Ute V., Farrugia, Charles J., Galvin, Antoinette B.
Interplanetary evolution of eleven magnetic clouds (MCs) recorded by at least two radially aligned spacecraft is studied. The in situ magnetic field measurements are fitted to a cylindrically symmetric Gold-Hoyle force-free uniform-twist flux-rope co
Externí odkaz:
http://arxiv.org/abs/1904.08266
Observations of Extreme ICME Ram Pressure Compressing Mercury's Dayside Magnetosphere to the Surface
Autor:
Winslow, Réka M., Lugaz, Noé, Philpott, Lydia, Farrugia, Charles J., Johnson, Catherine L., Anderson, Brian J., Paty, Carol S., Schwadron, Nathan A., Asad, Manar Al
Mercury's magnetosphere is known to be affected by enhanced ram pressures and magnetic fields inside interplanetary coronal mass ejections (ICMEs). Here we report detailed observations of an ICME compressing Mercury's dayside magnetosphere to the sur
Externí odkaz:
http://arxiv.org/abs/1903.00577