Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Charles J Farrugia"'
Autor:
Xiaojun Xu, Lou-Chuang Lee, Qi Xu, Qing Chang, Jing Wang, Ming Wang, Shaosui Xu, Christian Möstl, Charles J. Farrugia, Xing Wang, Yudong Ye, Zilu Zhou, Lei Luo, Peishan He, Shaoguan Cheng
Publikováno v:
Fundamental Research, Vol 4, Iss 4, Pp 882-889 (2024)
A mechanism for energy transfer from the solar wind to the Martian ionosphere through open magnetic flux rope is proposed based on the observations by Mars Atmosphere and Volatile EvolutioN (MAVEN). The satellite was located in the dayside magnetoshe
Externí odkaz:
https://doaj.org/article/0b92c8e28c42406c8c33d57dc60b1945
Autor:
Al-Haddad, Nada, Lugaz, Noe, Poedts, Stefaan, and, Charles J. Farrugia, Nieves-Chinchilla, Teresa
The evolution of the magnetic field and plasma quantities inside a coronal mass ejection (CME) with distance are known from statistical studies using data from 1 au monitors, planetary missions, Helios, and Ulysses. This does not cover the innermost
Externí odkaz:
http://arxiv.org/abs/1910.04811
Autor:
Sahanaj A. Banu, Réka M. Winslow, Camilla Scolini, Emma E. Davies, Charles J. Farrugia, Amy K. Murphy, Noé Lugaz, Nada Al-Haddad
Publikováno v:
The Astrophysical Journal, Vol 976, Iss 1, p 79 (2024)
In this study, we utilize magnetic field data from the Juno mission’s cruise phase to visually identify and analyze 338 interplanetary small flux ropes (SFRs) across a heliocentric distance range of 1–5.5 au. The events are uniformly distributed
Externí odkaz:
https://doaj.org/article/3f6832e4aed44792b5701edaf2151ded
Autor:
Wenyuan Yu, Nada Al-Haddad, Charles J. Farrugia, Noé Lugaz, Bin Zhuang, Florian Regnault, Antoinette B. Galvin
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 2, p 289 (2024)
The aim of this study is to use multispacecraft measurements of interplanetary magnetic clouds (MCs) to better constrain and understand the effect of expansion on their magnetic field properties. We develop a parameter ( γ ) for comparing magnetic f
Externí odkaz:
https://doaj.org/article/5ec62e5ea2b545cf92338bcda3bfbf3b
Autor:
Noé Lugaz, Bin Zhuang, Camilla Scolini, Nada Al-Haddad, Charles J. Farrugia, Réka M. Winslow, Florian Regnault, Christian Möstl, Emma E. Davies, Antoinette B. Galvin
Publikováno v:
The Astrophysical Journal, Vol 962, Iss 2, p 193 (2024)
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:
https://doaj.org/article/497cde3acc624baf83b3e30a73f0d7bb
Autor:
Camilla Scolini, Noé Lugaz, Réka M. Winslow, Charles J. Farrugia, Norbert Magyar, Fabio Bacchini
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 1, p 135 (2024)
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 thi
Externí odkaz:
https://doaj.org/article/9c434420e1c84d5e99e083462902f530
Autor:
Réka M. Winslow, Camilla Scolini, Lan K. Jian, Teresa Nieves-Chinchilla, Manuela Temmer, Fernando Carcaboso, Brigitte Schmieder, Stefaan Poedts, Benjamin J. Lynch, Brian E. Wood, Erika Palmerio, Noé Lugaz, Charles J. Farrugia, Christina O. Lee, Emma E. Davies, Florian Regnault, Tarik M. Salman, Tibor Török, Nada Al-Haddad, Angelos Vourlidas, Ward B. Manchester, Meng Jin, Benoit Lavraud, Antoinette B. Galvin
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
This perspective paper brings to light the need for comprehensive studies on the evolution of interplanetary coronal mass ejection (ICME) complexity during propagation. To date, few studies of ICME complexity exist. Here, we define ICME complexity an
Externí odkaz:
https://doaj.org/article/40f90fe46fc04559838ba41b0357ef6f
Autor:
Bin Zhuang, Noé Lugaz, Nada Al-Haddad, Réka M. Winslow, Camilla Scolini, Charles J. Farrugia, Antoinette B. Galvin
Publikováno v:
The Astrophysical Journal, Vol 952, Iss 1, p 7 (2023)
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:
https://doaj.org/article/cc6402dc2b224e2bbb679de52934aaa2
Autor:
Charles J. Farrugia
Publikováno v:
Comma. 2021:129-135
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::49c13433e0a0cdd67f62d67a4c6936e7
https://doi.org/10.3828/coma.2021.15
https://doi.org/10.3828/coma.2021.15
Autor:
Noé Lugaz, Charles J. Farrugia, Chia-Lin Huang, Reka M. Winslow, Harlan E. Spence, Nathan A. Schwadron
Publikováno v:
Nature Communications, Vol 7, Iss 1, Pp 1-7 (2016)
The interaction between the Earth’s magnetic field and the solar wind results in the formation of a collisionless bow shock. Here, the authors study an even in which the solar wind Mach number remained steadily below one, leading to the evanescence
Externí odkaz:
https://doaj.org/article/0b0c42bfbf3a41fd97a12d02373794bd