Zobrazeno 1 - 10
of 220
pro vyhledávání: '"REALE, FABIO"'
Autor:
Schulz, Norbert S., Huenemoerder, David P., Principe, David A., Gagne, Marc, Günther, Hans Moritz, Kastner, Joel, Nichols, Joy, Pollock, Andrew, Preibisch, Thomas, Testa, Paola, Reale, Fabio, Favata, Fabio, Canizares, Claude R.
The Orion Nebula Cluster (ONC) is the closest site of very young ($\sim$ 1 Myrs) massive star formation. The ONC hosts more than 1600 young and X-ray bright stars with masses ranging from $\sim$ 0.1 to 35 $M_\odot$. The Chandra HETGS Orion Legacy Pro
Externí odkaz:
http://arxiv.org/abs/2404.19676
Autor:
Telloni, Daniele, Romoli, Marco, Velli, Marco, Zank, Gary P., Adhikari, Laxman, Downs, Cooper, Burtovoi, Aleksandr, Susino, Roberto, Spadaro, Daniele, Zhao, Lingling, Liberatore, Alessandro, Shi, Chen, De Leo, Yara, Abbo, Lucia, Frassati, Federica, Jerse, Giovanna, Landini, Federico, Nicolini, Gianalfredo, Pancrazzi, Maurizio, Russano, Giuliana, Sasso, Clementina, Andretta, Vincenzo, Da Deppo, Vania, Fineschi, Silvano, Grimani, Catia, Heinzel, Petr, Moses, John D., Naletto, Giampiero, Stangalini, Marco, Teriaca, Luca, Uslenghi, Michela, Berlicki, Arkadiusz, Bruno, Roberto, Capobianco, Gerardo, Capuano, Giuseppe E., Casini, Chiara, Casti, Marta, Chioetto, Paolo, Corso, Alain J., D'Amicis, Raffaella, Fabi, Michele, Frassetto, Fabio, Giarrusso, Marina, Giordano, Silvio, Guglielmino, Salvo L., Magli, Enrico, Massone, Giuseppe, Messerotti, Mauro, Nisticò, Giuseppe, Pelizzo, Maria G., Reale, Fabio, Romano, Paolo, Schühle, Udo, Solanki, Sami K., Straus, Thomas, Ventura, Rita, Volpicelli, Cosimo A., Zangrilli, Luca, Zimbardo, Gaetano, Zuppella, Paola, Bale, Stuart D., Kasper, Justin C.
This Letter reports the first observational estimate of the heating rate in the slowly expanding solar corona. The analysis exploits the simultaneous remote and local observations of the same coronal plasma volume with the Solar Orbiter/Metis and the
Externí odkaz:
http://arxiv.org/abs/2306.10819
Publikováno v:
A&A, 654, L3. (2021)
The determination of the chemical composition of interplanetary coronal mass ejection (ICME) plasma is an open issue. More specifically, it is not yet fully understood how remote sensing observations of the solar corona plasma during solar disturbanc
Externí odkaz:
http://arxiv.org/abs/2211.12993
Autor:
Biondo, Ruggero, Bemporad, Alessandro, Pagano, Paolo, Telloni, Daniele, Reale, Fabio, Romoli, Marco, Andretta, Vincenzo, Antonucci, Ester, Da Deppo, Vania, De Leo, Yara, Fineschi, Silvano, Heinzel, Petr, Moses, Daniel, Naletto, Giampiero, Nicolini, Gianalfredo, Spadaro, Daniele, Stangalini, Marco, Teriaca, Luca, Landini, Federico, Sasso, Clementina, Susino, Roberto, Jerse, Giovanna, Uslenghi, Michela, Pancrazzi, Maurizio
Publikováno v:
A&A 668, A144 (2022)
As a key feature, NASA's Parker Solar Probe (PSP) and ESA-NASA's Solar Orbiter (SO) missions cooperate to trace solar wind and transients from their sources on the Sun to the inner interplanetary space. The goal of this work is to accurately reconstr
Externí odkaz:
http://arxiv.org/abs/2211.12994
Autor:
Testa, Paola, Reale, Fabio
The X-ray emission from the Sun reveals a very dynamic hot atmosphere, the corona, which is characterized by a complex morphology and broad range of timescales of variability and spatial structuring. The solar magnetic fields play a fundamental role
Externí odkaz:
http://arxiv.org/abs/2206.03530
Autor:
Telloni, Daniele, Andretta, Vincenzo, Antonucci, Ester, Bemporad, Alessandro, Capuano, Giuseppe E., Fineschi, Silvano, Giordano, Silvio, Habbal, Shadia, Perrone, Denise, Pinto, Rui F., Sorriso-Valvo, Luca, Spadaro, Daniele, Susino, Roberto, Woodham, Lloyd D., Zank, Gary P., Romoli, Marco, Bale, Stuart D., Kasper, Justin C., Auchère, Frédéric, Bruno, Roberto, Capobianco, Gerardo, Case, Anthony W., Casini, Chiara, Casti, Marta, Chioetto, Paolo, Corso, Alain J., Da Deppo, Vania, De Leo, Yara, de Wit, Thierry Dudok, Frassati, Federica, Frassetto, Fabio, Goetz, Keith, Guglielmino, Salvo L., Harvey, Peter R., Heinzel, Petr, Jerse, Giovanna, Korreck, Kelly E., Landini, Federico, Larson, Davin, Liberatore, Alessandro, Livi, Roberto, MacDowall, Robert J., Magli, Enrico, Malaspina, David M., Massone, Giuseppe, Messerotti, Mauro, Moses, John D., Naletto, Giampiero, Nicolini, Gianalfredo, Nisticò, Giuseppe, Panasenco, Olga, Pancrazzi, Maurizio, Pelizzo, Maria G., Pulupa, Marc, Reale, Fabio, Romano, Paolo, Sasso, Clementina, Schühle, Udo, Stangalini, Marco, Stevens, Michael L., Strachan, Leonard, Straus, Thomas, Teriaca, Luca, Uslenghi, Michela, Velli, Marco, Verscharen, Daniel, Volpicelli, Cosimo A., Whittlesey, Phyllis, Zangrilli, Luca, Zimbardo, Gaetano, Zuppella, Paola
Publikováno v:
Telloni, D., Andretta, V., Antonucci, E., et al. 2021, ApJL, 920, L14
This Letter addresses the first Solar Orbiter (SO) -- Parker Solar Probe (PSP) quadrature, occurring on January 18, 2021, to investigate the evolution of solar wind from the extended corona to the inner heliosphere. Assuming ballistic propagation, th
Externí odkaz:
http://arxiv.org/abs/2110.11031
Autor:
Riedl, Julia M., Van Doorsselaere, Tom, Reale, Fabio, Goossens, Marcel, Petralia, Antonino, Pagano, Paolo
Acoustic waves excited in the photosphere and below might play an integral part in the heating of the solar chromosphere and corona. However, it is yet not fully clear how much of the initially acoustic wave flux reaches the corona and in what form.
Externí odkaz:
http://arxiv.org/abs/2109.02971
Autor:
De Pontieu, Bart, Testa, Paola, Martinez-Sykora, Juan, Antolin, Patrick, Karampelas, Konstantinos, Hansteen, Viggo, Rempel, Matthias, Cheung, Mark C. M., Reale, Fabio, Danilovic, Sanja, Pagano, Paolo, Polito, Vanessa, De Moortel, Ineke, Nobrega-Siverio, Daniel, Van Doorsselaere, Tom, Petralia, Antonino, Asgari-Targhi, Mahboubeh, Boerner, Paul, Carlsson, Mats, Chintzoglou, Georgios, Daw, Adrian, DeLuca, Ed, Golub, Leon, Matsumoto, Takuma, Ugarte-Urra, Ignacio, McIntosh, Scott, team, the MUSE
The Multi-slit Solar Explorer (MUSE) is a proposed NASA MIDEX mission, currently in Phase A, composed of a multi-slit EUV spectrograph (in three narrow spectral bands centered around 171A, 284A, and 108A) and an EUV context imager (in two narrow pass
Externí odkaz:
http://arxiv.org/abs/2106.15584
Autor:
Wang, Tongjiang, Ofman, Leon, Yuan, Ding, Reale, Fabio, Kolotkov, Dmitrii Y., Srivastava, Abhishek K.
Publikováno v:
Space Sci Rev (2021) 217:34
Rapidly decaying long-period oscillations often occur in hot coronal loops of active regions associated with small (or micro-) flares. This kind of wave activity was first discovered with the SOHO/SUMER spectrometer from Doppler velocity measurements
Externí odkaz:
http://arxiv.org/abs/2102.11376
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