Zobrazeno 1 - 10
of 94
pro vyhledávání: '"Galvin, Antoinette"'
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:
Klein, Kristopher G., Spence, Harlan, Alexandrova, Olga, Argall, Matthew, Arzamasskiy, Lev, Bookbinder, Jay, Broeren, Theodore, Caprioli, Damiano, Case, Anthony, Chandran, Benjamin, Chen, Li-Jen, Dors, Ivan, Eastwood, Jonathan, Forsyth, Colin, Galvin, Antoinette, Genot, Vincent, Halekas, Jasper, Hesse, Michael, Hine, Butler, Horbury, Tim, Jian, Lan, Kasper, Justin, Kretzschmar, Matthieu, Kunz, Matthew, Lavraud, Benoit, Contel, Olivier Le, Mallet, Alfred, Maruca, Bennett, Matthaeus, William, Niehof, Jonathan, O'Brian, Helen, Owen, Christopher, Retino, Alessandro, Reynolds, Christopher, Roberts, Owen, Schekochihin, Alexander, Skoug, Ruth, Smith, Charles, Smith, Sonya, Steinberg, John, Stevens, Michael, Szabo, Adam, TenBarge, Jason, Torbert, Roy, Vasquez, Bernard, Verscharen, Daniel, Whittlesey, Phyllis, Wickizer, Brittany, Zank, Gary, Zweibel, Ellen
HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma turbulence, a ubiquitous process occurring in the heliosphere and in p
Externí odkaz:
http://arxiv.org/abs/2306.06537
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:
Davies, Emma E., Winslow, Réka M., Scolini, Camilla, Forsyth, Robert J., Möstl, Christian, Lugaz, Noé, Galvin, Antoinette B.
We present a catalogue of 35 interplanetary coronal mass ejections (ICMEs) observed by the Juno spacecraft and at least one other spacecraft during its cruise phase to Jupiter. We identify events observed by MESSENGER, Venus Express, Wind, and STEREO
Externí odkaz:
http://arxiv.org/abs/2205.09472
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:
Palmerio, Erika, Lee, Christina O., Mays, M. Leila, Luhmann, Janet G., Lario, David, Sánchez-Cano, Beatriz, Richardson, Ian G., Vainio, Rami, Stevens, Michael L., Cohen, Christina M. S., Steinvall, Konrad, Möstl, Christian, Weiss, Andreas J., Nieves-Chinchilla, Teresa, Li, Yan, Larson, Davin E., Heyner, Daniel, Bale, Stuart D., Galvin, Antoinette B., Holmström, Mats, Khotyaintsev, Yuri V., Maksimovic, Milan, Mitrofanov, Igor G.
Predictions of coronal mass ejections (CMEs) and solar energetic particles (SEPs) are a central issue in space weather forecasting. In recent years, interest in space weather predictions has expanded to include impacts at other planets beyond Earth a
Externí odkaz:
http://arxiv.org/abs/2203.16433
Autor:
Scolini, Camilla, Winslow, Réka M., Lugaz, Noé, Salman, Tarik M., Davies, Emma E., Galvin, Antoinette B.
We present the first statistical analysis of complexity changes affecting the magnetic structure of interplanetary coronal mass ejections (ICMEs), with the aim of answering the questions: How frequently do ICMEs undergo magnetic complexity changes du
Externí odkaz:
http://arxiv.org/abs/2111.12637
We present the first PSP-observed CME that hits a second spacecraft before the end of the PSP encounter, providing an excellent opportunity to study short-term CME evolution. The CME was launched from the Sun on 10 October 2019 and was measured in si
Externí odkaz:
http://arxiv.org/abs/2106.04685
We study two interplanetary coronal mass ejections (ICMEs) observed at Mercury and 1 AU by spacecraft in longitudinal conjunction, investigating the question: what causes the drastic alterations observed in some ICMEs during propagation, while other
Externí odkaz:
http://arxiv.org/abs/2105.10602
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