Zobrazeno 1 - 10
of 92
pro vyhledávání: '"Criscuoli, Serena"'
Precise, high-cadence, long-term records of stellar spectral variability at different temporal scales lead to better understanding of a wide variety of phenomena including stellar atmospheres and dynamos, convective motions, and rotational periods. H
Externí odkaz:
http://arxiv.org/abs/2305.05510
Autor:
Ledvina, Vincent E., Kazachenko, Maria D., Criscuoli, Serena, Tilipman, Dennis, Ermolli, Ilaria, Falco, Mariachiara, Guglielmino, Salvatore, Jafarzadeh, Shahin, van der Voort, Luc Rouppe, Zuccarello, Francesca
We analyzed spectropolarimetric data from the Swedish 1-meter Solar Telescope to investigate physical properties of small-scale magnetic cancellations in the quiet Sun photosphere. Specifically, we looked at the full Stokes polarization profiles alon
Externí odkaz:
http://arxiv.org/abs/2206.04644
Autor:
Nita, Gelu, Ahmadzadeh, Azim, Criscuoli, Serena, Davey, Alisdair, Gary, Dale, Georgoulis, Manolis, Hurlburt, Neal, Kitiashvili, Irina, Kempton, Dustin, Kosovichev, Alexander, Martens, Piet, McGranaghan, Ryan, Oria, Vincent, Reardon, Kevin, Sadykov, Viacheslav, Timmons, Ryan, Wang, Haimin, Wang, Jason T. L.
Solar and Heliosphere physics are areas of remarkable data-driven discoveries. Recent advances in high-cadence, high-resolution multiwavelength observations, growing amounts of data from realistic modeling, and operational needs for uninterrupted sci
Externí odkaz:
http://arxiv.org/abs/2203.09544
Autor:
Ermolli, Ilaria, Giorgi, Fabrizio, Murabito, Mariarita, Stangalini, Marco, Guido, Vincenzo, Molinaro, Marco, Romano, Paolo, Guglielmino, Salvatore L., Viavattene, Giorgio, Cauzzi, Gianna, Criscuoli, Serena, Reardon, Kevin P., Tritschler, Alexandra
Publikováno v:
A&A 661, A74 (2022)
The IBIS data Archive (IBIS-A) stores data acquired with the Interferometric BIdimensional Spectropolarimeter (IBIS), which was operated at the Dunn Solar Telescope of the US National Solar Observatory from 2003 to 2019. The instrument provided serie
Externí odkaz:
http://arxiv.org/abs/2202.09946
Autor:
Rackham, Benjamin V., Espinoza, Néstor, Berdyugina, Svetlana V., Korhonen, Heidi, MacDonald, Ryan J., Montet, Benjamin T., Morris, Brett M., Oshagh, Mahmoudreza, Shapiro, Alexander I., Unruh, Yvonne C., Quintana, Elisa V., Zellem, Robert T., Apai, Dániel, Barclay, Thomas, Barstow, Joanna K., Bruno, Giovanni, Carone, Ludmila, Casewell, Sarah L., Cegla, Heather M., Criscuoli, Serena, Fischer, Catherine, Fournier, Damien, Giampapa, Mark S., Giles, Helen, Iyer, Aishwarya, Kopp, Greg, Kostogryz, Nadiia M., Krivova, Natalie, Mallonn, Matthias, McGruder, Chima, Molaverdikhani, Karan, Newton, Elisabeth R., Panja, Mayukh, Peacock, Sarah, Reardon, Kevin, Roettenbacher, Rachael M., Scandariato, Gaetano, Solanki, Sami, Stassun, Keivan G., Steiner, Oskar, Stevenson, Kevin B., Tregloan-Reed, Jeremy, Valio, Adriana, Wedemeyer, Sven, Welbanks, Luis, Yu, Jie, Alam, Munazza K., Davenport, James R. A., Deming, Drake, Dong, Chuanfei, Ducrot, Elsa, Fisher, Chloe, Gilbert, Emily, Kostov, Veselin, López-Morales, Mercedes, Line, Mike, Močnik, Teo, Mullally, Susan, Paudel, Rishi R., Ribas, Ignasi, Valenti, Jeff A.
Study Analysis Group 21 (SAG21) of NASA's Exoplanet Exploration Program Analysis Group (ExoPAG) was organized to study the effect of stellar contamination on space-based transmission spectroscopy, a method for studying exoplanetary atmospheres by mea
Externí odkaz:
http://arxiv.org/abs/2201.09905
Solar variability occurs over a broad range of spatial and temporal scales, from the Sun's brightening over its lifetime to the fluctuations commonly associated with magnetic activity over minutes to years. The latter activity includes most prominent
Externí odkaz:
http://arxiv.org/abs/2111.02928
Autor:
Abduallah, Yasser, Wang, Jason T. L., Shen, Yucong, Alobaid, Khalid A., Criscuoli, Serena, Wang, Haimin
The Earth's primary source of energy is the radiant energy generated by the Sun, which is referred to as solar irradiance, or total solar irradiance (TSI) when all of the radiation is measured. A minor change in the solar irradiance can have a signif
Externí odkaz:
http://arxiv.org/abs/2107.11042
Autor:
Criscuoli, Serena, Kazachenko, Maria, Kitashvili, Irina, Kosovichev, Alexander, Pillet, Valentín Martínez, Nita, Gelu, Sadykov, Viacheslav, Wray, Alan
The next decade will be an exciting period for solar astrophysics, as new ground- and space-based instrumentation will provide unprecedented observations of the solar atmosphere and heliosphere. The synergy between modeling effort and comprehensive a
Externí odkaz:
http://arxiv.org/abs/2101.00011
Autor:
Zills, Garrett1, Criscuoli, Serena2 scriscuo@nso.edu, Bertello, Luca2, Pevtsov, Alexei2, Buzasi, Derek L.3, Airapetian, Vladimir4
Publikováno v:
Frontiers in Astronomy & Space Sciences. 2024, p01-10. 10p.
Autor:
Zuccarello, Francesca, Guglielmino, Salvo L., Capparelli, Vincenzo, Mathioudakis, Mihalis, Keys, Peter H., Criscuoli, Serena, Falco, Mariachiara, Murabito, Mariarita
During solar flares, magnetic energy can be converted into electromagnetic radiation from radio waves to $\gamma$ rays. Enhancements in the continuum at visible wavelengths give rise to white-light flares, as well as continuum enhancements in the FUV
Externí odkaz:
http://arxiv.org/abs/1912.00859