Zobrazeno 1 - 10
of 129
pro vyhledávání: '"Nieves-Chinchilla, Teresa"'
Magnetic flux ropes within interplanetary coronal mass ejections are often characterized as simplistic cylindrical or toroidal tubes with field lines that twist around the cylinder or torus axis. Recent multi-point observations suggest that the overa
Externí odkaz:
http://arxiv.org/abs/2406.13022
Autor:
Pal, Sanchita, Santos, Luiz F. G. dos, Weiss, Andreas J., Narock, Thomas, Narock, Ayris, Nieves-Chinchilla, Teresa, Jian, Lan K., Good, Simon W.
Detecting large-scale flux ropes (FRs) embedded in interplanetary coronal mass ejections (ICMEs) and assessing their geoeffectiveness are essential since they can drive severe space weather. At 1 au, these FRs have an average duration of 1 day. Their
Externí odkaz:
http://arxiv.org/abs/2406.07798
Autor:
Davies, Emma E., Rüdisser, Hannah T., Amerstorfer, Ute V., Möstl, Christian, Bauer, Maike, Weiler, Eva, Amerstorfer, Tanja, Majumdar, Satabdwa, Hess, Phillip, Weiss, Andreas J., Reiss, Martin A., Green, Lucie M., Long, David M., Nieves-Chinchilla, Teresa, Trotta, Domenico, Horbury, Timothy S., O'Brien, Helen, Fauchon-Jones, Edward, Morris, Jean, Owen, Christopher J., Bale, Stuart D., Kasper, Justin C.
As both Parker Solar Probe (PSP) and Solar Orbiter (SolO) reach heliocentric distances closer to the Sun, they present an exciting opportunity to study the structure of CMEs in the inner heliosphere. We present an analysis of the global flux rope str
Externí odkaz:
http://arxiv.org/abs/2405.10810
Autor:
Salman, Tarik M., Nieves-Chinchilla, Teresa, Jian, Lan K., Lugaz, Noé, Carcaboso, Fernando, Davies, Emma E., Collado-Vega, Yaireska M.
We present a statistical investigation of the radial evolution of 28 interplanetary coronal mass ejections (ICMEs), measured in situ by the Parker Solar Probe (PSP) spacecraft from 2018 October to 2022 August. First, by analyzing the radial distribut
Externí odkaz:
http://arxiv.org/abs/2403.02594
Autor:
Palmerio, Erika, Carcaboso, Fernando, Khoo, Leng Ying, Salman, Tarik M., Sánchez-Cano, Beatriz, Lynch, Benjamin J., Rivera, Yeimy J., Pal, Sanchita, Nieves-Chinchilla, Teresa, Weiss, Andreas J., Lario, David, Mieth, Johannes Z. D., Heyner, Daniel, Stevens, Michael L., Romeo, Orlando M., Zhukov, Andrei N., Rodriguez, Luciano, Lee, Christina O., Cohen, Christina M. S., Rodríguez-García, Laura, Whittlesey, Phyllis L., Dresing, Nina, Oleynik, Philipp, Jebaraj, Immanuel C., Fischer, David, Schmid, Daniel, Richter, Ingo, Auster, Hans-Ulrich, Fraschetti, Federico, Mierla, Marilena
On 2022 February 15, an impressive filament eruption was observed off the solar eastern limb from three remote-sensing viewpoints, namely Earth, STEREO-A, and Solar Orbiter. In addition to representing the most-distant observed filament at extreme ul
Externí odkaz:
http://arxiv.org/abs/2401.01875
Type II radio bursts arise as a consequence of shocks typically driven by coronal mass ejections (CMEs). When these shocks propagate outward from the Sun, their associated radio emissions drift down in frequency as excited particles emit at the local
Externí odkaz:
http://arxiv.org/abs/2311.08266
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:
Pérez-Alanis, Carlos, Janvier, Miho, Nieves-Chinchilla, Teresa, Aguilar-Rodríguez, Ernesto, Démoulin, Pascal, Corona-Romero, Pedro
In situ observations of interplanetary (IP) coronal mass ejections (ICMEs) and IP shocks are important to study as they are the main components of the solar activity. Hundreds of IP shocks have been detected by various space missions at different tim
Externí odkaz:
http://arxiv.org/abs/2304.05733
Autor:
Dorelli, John C., Bard, Chris, Chen, Thomas Y., Da Silva, Daniel, Santos, Luiz Fernando Guides dos, Ireland, Jack, Kirk, Michael, McGranaghan, Ryan, Narock, Ayris, Nieves-Chinchilla, Teresa, Samara, Marilia, Sarantos, Menelaos, Schuck, Pete, Thompson, Barbara
Traditionally, data analysis and theory have been viewed as separate disciplines, each feeding into fundamentally different types of models. Modern deep learning technology is beginning to unify these two disciplines and will produce a new class of p
Externí odkaz:
http://arxiv.org/abs/2212.13328
We use in-situ data from the Wind spacecraft to survey the amplitude of turbulent fluctuations in the proton density and total magnetic field inside a large sample of near-Earth magnetic clouds (MCs) associated with coronal mass ejections (CMEs) from
Externí odkaz:
http://arxiv.org/abs/2210.17359