Zobrazeno 1 - 10
of 155
pro vyhledávání: '"Sánchez‐Cano, Beatriz"'
Autor:
Palmerio, Erika, Kay, Christina, Al-Haddad, Nada, Lynch, Benjamin J., Trotta, Domenico, Yu, Wenyuan, Ledvina, Vincent E., Sánchez-Cano, Beatriz, Riley, Pete, Heyner, Daniel, Schmid, Daniel, Fischer, David, Richter, Ingo, Auster, Hans-Ulrich
Understanding and predicting the structure and evolution of coronal mass ejections (CMEs) in the heliosphere remains one of the most sought-after goals in heliophysics and space weather research. A powerful tool for improving current knowledge and ca
Externí odkaz:
http://arxiv.org/abs/2411.12706
Extent of the Magnetotail of Venus From the Solar Orbiter, Parker Solar Probe and BepiColombo Flybys
Autor:
Edberg, Niklas J. T., Andrews, David J., Boldú, J. Jordi, Dimmock, Andrew P., Khotyaintsev, Yuri V., Kim, Konstantin, Persson, Moa, Auster, Uli, Constantinescu, Dragos, Heyner, Daniel, Mieth, Johannes, Richter, Ingo, Curry, Shannon M., Hadid, Lina Z., Pisa, David, Sorriso-Valvo, Luca, Lester, Mark, Sánchez-Cano, Beatriz, Stergiopoulou, Katerina, Romanelli, Norberto, Fischer, David, Schmid, Daniel, Volwerk, Martin
Publikováno v:
Journal of Geophysical Research: Space Physics, 129, e2024JA032603
We analyze data from multiple flybys by the Solar Orbiter, BepiColombo, and Parker Solar Probe (PSP) missions to study the interaction between Venus' plasma environment and the solar wind forming the induced magnetosphere. Through examination of magn
Externí odkaz:
http://arxiv.org/abs/2410.21856
Autor:
Ma, Mengxuan, Yang, Liping, Shen, Fang, Shen, Chenglong, Chi, Yutian, Wang, Yuming, Zhou, Yufen, Zhang, Man, Heyner, Daniel, Auster, Uli, Richter, Ingo, Sanchez-Cano, Beatriz
The magnetic orientation of coronal mass ejections (CMEs) is of great importance to understand their space weather effects. Although many evidences suggest that CMEs can undergo significant rotation during the early phases of evolution in the solar c
Externí odkaz:
http://arxiv.org/abs/2410.20803
Autor:
Palmerio, Erika, Luhmann, Janet G., Mays, M. Leila, Caplan, Ronald M., Lario, David, Richardson, Ian G., Whitman, Kathryn, Lee, Christina O., Sánchez-Cano, Beatriz, Wijsen, Nicolas, Li, Yan, Cardoso, Carlota, Pinto, Marco, Heyner, Daniel, Schmid, Daniel, Auster, Hans-Ulrich, Fischer, David
Multi-spacecraft observations of solar energetic particle (SEP) events not only enable a deeper understanding and development of particle acceleration and transport theories, but also provide important constraints for model validation efforts. Howeve
Externí odkaz:
http://arxiv.org/abs/2401.05309
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
Autor:
Gerekos, Christopher, Steinbrügge, Gregor, Jebaraj, Immanuel, Casillas, Andreas, Donini, Elena, Sánchez-Cano, Beatriz, Lester, Mark, Magdalenić, Jasmina, Peters, Sean, Romero-Wolf, Andrew, Blankenship, Donald
Publikováno v:
Astronomy & Astrophysics 683, A56 (2024)
Multispacecraft and multiwavelength observations of solar eruptions such as flares and coronal mass ejections are essential to understand the complex processes behind these events. The study of solar burst events in the radio-frequency spectrum has r
Externí odkaz:
http://arxiv.org/abs/2307.01747
Autor:
Wijsen, Nicolas, Lario, David, Sánchez-Cano, Beatriz, Jebaraj, Immanuel C., Dresing, Nina, Richardson, Ian G., Aran, Angels, Kouloumvakos, Athanasios, Ding, Zheyi, Niemela, Antonio, Palmerio, Erika, Carcaboso, Fernando, Vainio, Rami, Afanasiev, Alexandr, Pinto, Marco, Pacheco, Daniel, Poedts, Stefaan, Heyner, Daniel
We present simulation results of a gradual solar energetic particle (SEP) event detected on 2021 October 9 by multiple spacecraft, including BepiColombo (Bepi) and near-Earth spacecraft such as the Advanced Composition Explorer (ACE). A peculiarity o
Externí odkaz:
http://arxiv.org/abs/2305.09525
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:
Cecconi, Baptiste, Witasse, Olivier, Jackman, Caitriona M., Sánchez-Cano, Beatriz, Mays, M. Leila
The Saturn Kilometric Radiation (SKR) was observed for the first time during the flyby of Saturn by the Voyager spacecraft in 1980. These radio emissions, in the range of a few kHz to 1 MHz, are emitted by electrons travelling around auroral magnetic
Externí odkaz:
http://arxiv.org/abs/2110.12713
Autor:
Palmerio, Erika, Nieves-Chinchilla, Teresa, Kilpua, Emilia K. J., Barnes, David, Zhukov, Andrei N., Jian, Lan K., Witasse, Olivier, Provan, Gabrielle, Tao, Chihiro, Lamy, Laurent, Bradley, Thomas J., Mays, M. Leila, Möstl, Christian, Roussos, Elias, Futaana, Yoshifumi, Masters, Adam, Sánchez-Cano, Beatriz
One of the grand challenges in heliophysics is the characterisation of coronal mass ejection (CME) magnetic structure and evolution from eruption at the Sun through heliospheric propagation. At present, the main difficulties are related to the lack o
Externí odkaz:
http://arxiv.org/abs/2110.02190