Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Olga Panasenco"'
Autor:
Zesen Huang, Chen Shi, Marco Velli, Nikos Sioulas, Olga Panasenco, Trevor Bowen, Lorenzo Matteini, Mingtao Xia, Xiaofei Shi, Sheng Huang, Jia Huang, Lizet Casillas
Publikováno v:
The Astrophysical Journal Letters, Vol 973, Iss 1, p L26 (2024)
The heliosphere is permeated with highly structured solar wind originating from the Sun. One of the primary science objectives of Parker Solar Probe (PSP) is to determine the structures and dynamics of the plasma and magnetic fields at the sources of
Externí odkaz:
https://doaj.org/article/49c71d7fd5124c7ca164a5b1046753bb
Autor:
Alessandro Liberatore, Paulett C. Liewer, Angelos Vourlidas, Carlos R. Braga, Marco Velli, Olga Panasenco, Daniele Telloni, Salvatore Mancuso
Publikováno v:
The Astrophysical Journal, Vol 957, Iss 2, p 110 (2023)
This paper reports on a well-defined EUV wave associated with a coronal mass ejection (CME) observed on 2022 March 25. The CME was observed by Solar Orbiter (SolO) during its first close perihelion (0.32 au) and by several other spacecraft from diffe
Externí odkaz:
https://doaj.org/article/abd3721d44364d19b50d16141efccf65
Autor:
Paulett C. Liewer, Angelos Vourlidas, Guillermo Stenborg, Russell A. Howard, Jiong Qiu, Paulo Penteado, Olga Panasenco, Carlos R. Braga
Publikováno v:
The Astrophysical Journal, Vol 948, Iss 1, p 24 (2023)
Parker Solar Probe (PSP) crossed the heliospheric current sheet (HCS) near the perihelion on encounters E8 and E11, enabling the Wide-field Imager for Solar Probe (WISPR) to image the streamer belt plasma in high resolution while flying through it. W
Externí odkaz:
https://doaj.org/article/affdb1e6671d4509beedd8d76c7a5ae3
Autor:
Alessandro Liberatore, Joe Zender, Gerardo Capobianco, Silvano Fineschi, Olga Panasenco, Dana Tomuta, Manuel Castillo, Miguel Pérez-Ayúcar
The results obtained during the total Solar Eclipse on July 2, 2019, in Chile are presented together with the Eclipse K-corona Polarimeter (EKPol). The EKPol is equipped with an electro-optically modulating Liquid Crystal Variable Retarder (LCVR) for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::06593fa47ff86b75d63e4f08081f784a
https://doi.org/10.21203/rs.3.rs-2662654/v1
https://doi.org/10.21203/rs.3.rs-2662654/v1
Autor:
Stuart Bale, James Drake, Michael McManus, Mihir Desai, Samuel Badman, Davin Larson, Marc Swisdak, Nour Raouafi, Tai Phan, Marco Velli, David McComas, Christina Cohen, Donald Mitchell, Olga Panasenco, Justin Kasper
The fast solar wind that fills the heliosphere originates from deep within regions of open magnetic field on the Sun called ‘coronal holes’. However the energy source responsible for accelerating the outflowing plasma to such high speeds is still
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::24f949b731623b16012147742eb29a78
https://doi.org/10.21203/rs.3.rs-1954304/v1
https://doi.org/10.21203/rs.3.rs-1954304/v1
Autor:
Raffaella DAmicis, Roberto Bruno, Rossana De Marco, Marco Velli, Daniele Telloni, Denise Perrone, Luca Sorriso-Valvo, Olga Panasenco
Publikováno v:
European Geosciences Union, EGU General Assembly 2022, Vienna, Austria and online, 23-27 May 2022
info:cnr-pdr/source/autori:DAmicis R.; Bruno R.; De Marco R.; Velli M.; Telloni D.; Perrone D.; Sorriso-Valvo L.; Panasenco O./congresso_nome:European Geosciences Union, EGU General Assembly 2022/congresso_luogo:Vienna, Austria and online/congresso_data:23-27 May 2022/anno:2022/pagina_da:/pagina_a:/intervallo_pagine
info:cnr-pdr/source/autori:DAmicis R.; Bruno R.; De Marco R.; Velli M.; Telloni D.; Perrone D.; Sorriso-Valvo L.; Panasenco O./congresso_nome:European Geosciences Union, EGU General Assembly 2022/congresso_luogo:Vienna, Austria and online/congresso_data:23-27 May 2022/anno:2022/pagina_da:/pagina_a:/intervallo_pagine
The solar wind is a highly variable, weakly collisional plasma originating from the Sun. The recent launches of PSP and Solar Orbiter have opened the way for the exploration of the innermost regions of our solar system and will greatly advance our un
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9464b2d8624cdb9e756dd64f1caa9d31
https://doi.org/10.5194/egusphere-egu22-12654
https://doi.org/10.5194/egusphere-egu22-12654
Autor:
Daniele Telloni, Gary P. Zank, Luca Sorriso-Valvo, Raffaella D’Amicis, Olga Panasenco, Roberto Susino, Roberto Bruno, Denise Perrone, Laxman Adhikari, Haoming Liang, Masaru Nakanotani, Lingling Zhao, Lina Z. Hadid, Beatriz Sánchez-Cano, Daniel Verscharen, Marco Velli, Catia Grimani, Raffaele Marino, Francesco Carbone, Salvatore Mancuso, Ruggero Biondo, Paolo Pagano, Fabio Reale, Stuart D. Bale, Justin C. Kasper, Anthony W. Case, Thierry Dudok de Wit, Keith Goetz, Peter R. Harvey, Kelly E. Korreck, Davin Larson, Roberto Livi, Robert J. MacDowall, David M. Malaspina, Marc Pulupa, Michael L. Stevens, Phyllis Whittlesey, Marco Romoli, Vincenzo Andretta, Vania Da Deppo, Silvano Fineschi, Petr Heinzel, John D. Moses, Giampiero Naletto, Gianalfredo Nicolini, Daniele Spadaro, Marco Stangalini, Luca Teriaca, Gerardo Capobianco, Giuseppe E. Capuano, Chiara Casini, Marta Casti, Paolo Chioetto, Alain J. Corso, Yara De Leo, Michele Fabi, Federica Frassati, Fabio Frassetto, Silvio Giordano, Salvo L. Guglielmino, Giovanna Jerse, Federico Landini, Alessandro Liberatore, Enrico Magli, Giuseppe Massone, Mauro Messerotti, Maurizio Pancrazzi, Maria G. Pelizzo, Paolo Romano, Clementina Sasso, Udo Schühle, Alessandra Slemer, Thomas Straus, Michela Uslenghi, Cosimo A. Volpicelli, Luca Zangrilli, Paola Zuppella, Lucia Abbo, Frédéric Auchère, Regina Aznar Cuadrado, Arkadiusz Berlicki, Angela Ciaravella, Philippe Lamy, Alessandro Lanzafame, Marco Malvezzi, Piergiorgio Nicolosi, Giuseppe Nisticò, Hardi Peter, Sami K. Solanki, Leonard Strachan, Kanaris Tsinganos, Rita Ventura, Jean-Claude Vial, Joachim Woch, Gaetano Zimbardo
Publikováno v:
The Astrophysical Journal
The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in combination with the remote-sensing observation of the coronal source region provided by the METIS coronagraph aboard Solar Orbiter. The coronal outflow
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::22445a3ae086ef24456bde8beb6673e8
https://hdl.handle.net/11576/2710572
https://hdl.handle.net/11576/2710572
Autor:
Vladimir Krasnoselskikh, Bruce T. Tsurutani, Thierry Dudok de Wit, Simon Walker, Michael Balikhin, Marianne Balat-Pichelin, Marco Velli, Stuart D. Bale, Milan Maksimovic, Oleksiy Agapitov, Wolfgang Baumjohann, Matthieu Berthomier, Roberto Bruno, Steven R. Cranmer, Bart de Pontieu, Domingos de Sousa Meneses, Jonathan Eastwood, Robertus Erdelyi, Robert Ergun, Viktor Fedun, Natalia Ganushkina, Antonella Greco, Louise Harra, Pierre Henri, Timothy Horbury, Hugh Hudson, Justin Kasper, Yuri Khotyaintsev, Matthieu Kretzschmar, Säm Krucker, Harald Kucharek, Yves Langevin, Benoît Lavraud, Jean-Pierre Lebreton, Susan Lepri, Michael Liemohn, Philippe Louarn, Eberhard Moebius, Forrest Mozer, Zdenek Nemecek, Olga Panasenco, Alessandro Retino, Jana Safrankova, Jack Scudder, Sergio Servidio, Luca Sorriso-Valvo, Jan Souček, Adam Szabo, Andris Vaivads, Grigory Vekstein, Zoltan Vörös, Teimuraz Zaqarashvili, Gaetano Zimbardo, Andrei Fedorov
Publikováno v:
Experimental Astronomy
Experimental Astronomy, 2022, 54, pp.277-315. ⟨10.1007/s10686-022-09878-1⟩
Experimental Astronomy, 2022, 54, pp.277-315. ⟨10.1007/s10686-022-09878-1⟩
The primary scientific goal of ICARUS (Investigation of Coronal AcceleRation and heating of solar wind Up to the Sun), a mother-daughter satellite mission, proposed in response to the ESA “Voyage 2050” Call, will be to determine how the magnetic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c4f5ffa97035a01cd3772f9e60998e11
https://hal-insu.archives-ouvertes.fr/insu-04089866/file/s10686-022-09878-1.pdf
https://hal-insu.archives-ouvertes.fr/insu-04089866/file/s10686-022-09878-1.pdf
Observation and Modeling of the Solar Wind Turbulence Evolution in the Sub-Mercury Inner Heliosphere
Autor:
Daniele Telloni, Laxman Adhikari, Gary P. Zank, Lina Z. Hadid, Beatriz Sánchez-Cano, Luca Sorriso-Valvo, Lingling Zhao, Olga Panasenco, Chen Shi, Marco Velli, Roberto Susino, Daniel Verscharen, Anna Milillo, Tommaso Alberti, Yasuhito Narita, Andrea Verdini, Catia Grimani, Roberto Bruno, Raffaella D’Amicis, Denise Perrone, Raffaele Marino, Francesco Carbone, Francesco Califano, Francesco Malara, Julia E. Stawarz, Ronan Laker, Alessandro Liberatore, Stuart D. Bale, Justin C. Kasper, Daniel Heyner, Thierry Dudok de Wit, Keith Goetz, Peter R. Harvey, Robert J. MacDowall, David M. Malaspina, Marc Pulupa, Anthony W. Case, Kelly E. Korreck, Davin Larson, Roberto Livi, Michael L. Stevens, Phyllis Whittlesey, Hans-Ulrich Auster, Ingo Richter
Publikováno v:
The Astrophysical Journal Letters. 938:L8
This letter exploits the radial alignment between the Parker Solar Probe and BepiColombo in late 2022 February, when both spacecraft were within Mercury’s orbit. This allows the study of the turbulent evolution, namely, the change in spectral and i
Autor:
Victor Réville, Phyllis Whittlesey, Anthony W. Case, Robert J. MacDowall, Olga Panasenco, Davin Larson, Peter Harvey, Justin C. Kasper, Kelly E. Korreck, Keith Goetz, Michael L. Stevens, Michel Moncuquet, Marco Velli, David M. Malaspina, Stuart D. Bale, Milan Maksimovic, Roberto Livi, Marc Pulupa, Thierry Dudok de Wit, Chen Shi, J. W. Bonnell, J. L. Verniero, Anna Tenerani
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 650, pp.A21. ⟨10.1051/0004-6361/202039818⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 650, pp.A21. ⟨10.1051/0004-6361/202039818⟩
Astronomy and Astrophysics-A&A, 2021, 650, pp.A21. ⟨10.1051/0004-6361/202039818⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 650, pp.A21. ⟨10.1051/0004-6361/202039818⟩
Context. Parker Solar Probe (PSP) measures the magnetic field and plasma parameters of the solar wind at unprecedentedly close distances to the Sun. These data provide great opportunities to study the early-stage evolution of magnetohydrodynamic (MHD
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fad11e1abe569b7cbc212e9a4fb337c7
https://hal-insu.archives-ouvertes.fr/insu-03342995/document
https://hal-insu.archives-ouvertes.fr/insu-03342995/document