Zobrazeno 1 - 10
of 105
pro vyhledávání: '"Teresa Nieves‐Chinchilla"'
Autor:
Oksana Kruparova, Vratislav Krupar, Adam Szabo, David Lario, Teresa Nieves-Chinchilla, Juan Carlos Martinez Oliveros
Publikováno v:
The Astrophysical Journal Letters, Vol 970, Iss 1, p L13 (2024)
We report on a comprehensive study of interplanetary type III radio bursts linked to X-class solar flares from NOAA active region 13664, which instigated the intense 2024 Mother’s Day solar storm, marked by a geomagnetic storm of −412 nT, the str
Externí odkaz:
https://doaj.org/article/6e6a7cfa09c8466193bc0d5202886e6b
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 2, p 169 (2024)
Magnetic flux ropes (MFRs) at the center of interplanetary coronal mass ejections (ICMEs) are often characterized as simplistic cylindrical or toroidal tubes with field lines that twist around the cylinder or torus axis. Recent multipoint observation
Externí odkaz:
https://doaj.org/article/4ed0a45823e940dcac344b866147205f
Autor:
Emma E. Davies, Hannah T. Rüdisser, Ute V. Amerstorfer, Christian Möstl, Maike Bauer, Eva Weiler, Tanja Amerstorfer, Satabdwa Majumdar, Phillip Hess, Andreas J. Weiss, Martin A. Reiss, Lucie M. Green, David M. Long, Teresa Nieves-Chinchilla, Domenico Trotta, Timothy S. Horbury, Helen O’Brien, Edward Fauchon-Jones, Jean Morris, Christopher J. Owen, Stuart D. Bale, Justin C. Kasper
Publikováno v:
The Astrophysical Journal, Vol 973, Iss 1, p 51 (2024)
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 coronal mass ejections (CMEs) in the inner heliosphere. We present an analysis of
Externí odkaz:
https://doaj.org/article/52550604d334446a80811b376e4dc618
Autor:
Sanchita Pal, Luiz F. G. dos Santos, Andreas J. Weiss, Thomas Narock, Ayris Narock, Teresa Nieves-Chinchilla, Lan K. Jian, Simon W. Good
Publikováno v:
The Astrophysical Journal, Vol 972, Iss 1, p 94 (2024)
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. Thei
Externí odkaz:
https://doaj.org/article/4fb04f8a352f48ac8808704592125612
Autor:
Tarik Mohammad Salman, Teresa Nieves-Chinchilla, Lan K. Jian, Noé Lugaz, Fernando Carcaboso, Emma E. Davies, Yaireska M. Collado-Vega
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 1, p 118 (2024)
We present a statistical investigation of the radial evolution of 28 interplanetary coronal mass ejections (ICMEs), measured in situ by the Parker Solar Probe spacecraft from 2018 October to 2022 August. First, by analyzing the radial distribution of
Externí odkaz:
https://doaj.org/article/17e086afd9a34a8e9d4b4819033c0be5
Autor:
Carlos R. Braga, Vamsee Krishna Jagarlamudi, Angelos Vourlidas, Guillermo Stenborg, Teresa Nieves-Chinchilla
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 2, p 185 (2024)
The relationship between CME properties in the corona and their interplanetary counterparts is not well understood. Until recently, a wide spatial gap existed between the two regions, which prevented us from disentangling the spatial and temporal evo
Externí odkaz:
https://doaj.org/article/ee918009a1ef40758bc06a3b44bd63f5
Autor:
Erika Palmerio, Fernando Carcaboso, Leng Ying Khoo, Tarik M. Salman, Beatriz Sánchez-Cano, Benjamin J. Lynch, Yeimy J. Rivera, Sanchita Pal, Teresa Nieves-Chinchilla, Andreas J. Weiss, David Lario, Johannes Z. D. Mieth, Daniel Heyner, Michael L. Stevens, Orlando M. Romeo, Andrei N. Zhukov, Luciano Rodriguez, Christina O. Lee, Christina M. S. Cohen, Laura Rodríguez-García, Phyllis L. Whittlesey, Nina Dresing, Philipp Oleynik, Immanuel C. Jebaraj, David Fischer, Daniel Schmid, Ingo Richter, Hans-Ulrich Auster, Federico Fraschetti, Marilena Mierla
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 2, p 108 (2024)
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 u
Externí odkaz:
https://doaj.org/article/e800f7fe6dca4568b4eaee788292df75
Autor:
Sanchita Pal, Laura Balmaceda, Andreas J. Weiss, Teresa Nieves-Chinchilla, Fernando Carcaboso, Emilia Kilpua, Christian Möstl
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
From 29 January to 7 February 2022, the heliosphere was structured with large-scale interacting substructures that appeared with significant dissimilarities at distant observations separated longitudinally by ∼34°. Probing the complexity of the st
Externí odkaz:
https://doaj.org/article/796c3463c76f4154b7c8166573d15512
Autor:
Elizabeth A. Jensen, Nat Gopalswamy, Lynn B. Wilson, Lan K. Jian, Shing F. Fung, Teresa Nieves-Chinchilla, Marta Shelton, Lihua Li, Manohar Deshpande, Lloyd Purves, Joseph Lazio, Ward B. Manchester, Brian E. Wood, Jason E. Kooi, David B. Wexler, Stuart Bale, Alexei Pevtsov, Bernard V. Jackson, Megan N. Kenny
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
There continue to be open questions regarding the solar wind and coronal mass ejections (CMEs). For example: how do magnetic fields within CMEs and corotating/stream interaction regions (CIRs/SIRs) evolve in the inner heliosphere? What is the radiall
Externí odkaz:
https://doaj.org/article/3f143b2b35364dbba9f23cc3df356581
Autor:
Teresa Nieves-Chinchilla, Sanchita Pal, Tarik M. Salman, Fernando Carcaboso, Silvina E. Guidoni, Hebe Cremades, Ayris Narock, Laura A. Balmaceda, Benjamin J. Lynch, Nada Al-Haddad, Laura Rodríguez-García, Thomas W. Narock, Luiz F. G. Dos Santos, Florian Regnault, Christina Kay, Réka M. Winslow, Erika Palmerio, Emma E. Davies, Camilla Scolini, Andreas J. Weiss, Nathalia Alzate, Mariana Jeunon, Roger Pujadas
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
Magnetic flux ropes manifest as twisted bundles of magnetic field lines. They carry significant amounts of solar mass in the heliosphere. This paper underlines the need to advance our understanding of the fundamental physics of heliospheric flux rope
Externí odkaz:
https://doaj.org/article/788b7431186846f5b015903792d7340a