Zobrazeno 1 - 10
of 52
pro vyhledávání: '"Stanislav Gunár"'
Autor:
Sven Wedemeyer, Gregory Fleishman, Jaime de la Cruz Rodríguez, Stanislav Gunár, João M. da Silva Santos, Patrick Antolin, Juan Camilo Guevara Gómez, Mikolaj Szydlarski, Henrik Eklund
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
The Atacama Large Millimeter/submillimeter Array (ALMA) offers new diagnostic possibilities that complement other commonly used diagnostics for the study of the Sun. In particular, ALMA’s ability to serve as an essentially linear thermometer of the
Externí odkaz:
https://doaj.org/article/659dec7960fa401988e134207b640e9e
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
This review comes at the time when ALMA successfully obtained the first regular observations of both a prominence and a filament. These observations have a spatial resolution of 1-2 arcsec, far better than previous prominence observations in the mm/s
Externí odkaz:
https://doaj.org/article/125eaa8de63e48688b5a6ab95fa24253
Autor:
Stanislav Gunár, Nicolas Labrosse, Manuel Luna, Brigitte Schmieder, Petr Heinzel, Therese A. Kucera, Peter J. Levens, Arturo López Ariste, Duncan H. Mackay, Maciej Zapiór
Publikováno v:
Space Science Reviews. 219
The term ‘tornado’ has been used in recent years to describe several solar phenomena, from large-scale eruptive prominences to small-scale photospheric vortices. It has also been applied to the generally stable quiescent prominences, sparking a r
Autor:
Sonja Jejčič, Petr Heinzel, Brigitte Schmieder, Stanislav Gunár, Pierre Mein, Nicole Mein, Guiping Ruan
Publikováno v:
The astrophysical journal, vol. 932, no. 1, 3, 2022.
We continued our investigation of the plasma characteristics of a quiescent prominence that occurred on 2017 March 30. The prominence was observed simultaneously by several instruments, including the Interface Region Imaging Spectrograph (IRIS) and t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8534fe749ba7f3fd57f668837eed0620
https://lirias.kuleuven.be/handle/20.500.12942/709162
https://lirias.kuleuven.be/handle/20.500.12942/709162
Autor:
Petr Heinzel, Arkadiusz Berlicki, Miroslav Bárta, Paweł Rudawy, Stanislav Gunár, Nicolas Labrosse, Krzysztof Radziszewski
We present first prominence observations obtained with ALMA in Band 3 at the wavelength of 3 mm. High-resolution observations have been coaligned with the MSDP H$\alpha$ data from Wroclaw-Bialk\'{o}w large coronagraph at similar spatial resolution. W
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1c2c56aa1ad57974555f05811a53b6f0
http://arxiv.org/abs/2202.12761
http://arxiv.org/abs/2202.12761
Publikováno v:
The Astrophysical Journal. 934:133
We demonstrate that changes in the incident radiation in Mg ii h and k lines have a significant impact on the results of radiative transfer modeling of prominence-like plasmas. To uncover the extent of this impact and allow easy comparison, here we s
Publikováno v:
The Astrophysical Journal Supplement Series. 261:17
The solar radiation in the cores of the Mg ii h and k spectral lines plays a significant role in the illumination of prominences, coronal mass ejections (CMEs), spicules, flare loops, and surges. Moreover, the radiation in these lines strongly correl
Autor:
Yi Chai, Roman Brajša, Dale Gary, Joaquim Costa, Stanislav Gunar, Guillermo Gimenez de Castro, Hugh Hudson, Pamela Klaassen, Gregory Fleishman, Atul Mohan, Mats Kirkaune, Alberto Pellizzoni, Mark Booth, Galina Motorina, Caius L. Selhorst, Maryam Saberi, Masumi Shimojo, Paulo J. A. Simoes, Davor Sudar, Ivica Skokić, Stephen M. White, Fabian Menezes, Amelie Saintonge, John Orlowski-Scherer, Antonio Hales, Claudia Cicone, Tony Mroczkowski, Doug Johnstone, Luca Di Mascolo, Minju Lee, Eelco van Kampen, Thomas Maccarone, Daizhong Liu, Matthew Smith, Martin A. Cordiner, Alexander E. Thelen, Miroslav Barta, Sven Wedemeyer
Publikováno v:
Open Research Europe, Vol 4 (2024)
Observations at (sub-)millimeter wavelengths offer a complementary perspective on our Sun and other stars, offering significant insights into both the thermal and magnetic composition of their chromospheres. Despite the fundamental progress in (sub-)
Externí odkaz:
https://doaj.org/article/4f6da9fb81b840cea6169317c6b98420
Autor:
Pierre Mein, Brigitte Schmieder, Sonja Jejčič, Guiping Ruan, Nicole Mein, Stanislav Gunár, Yao Chen, Petr Heinzel
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2019, 886 (2), pp.134. ⟨10.3847/1538-4357/ab4b50⟩
The Astrophysical Journal, American Astronomical Society, 2019, 886 (2), pp.134. ⟨10.3847/1538-4357/ab4b50⟩
ispartof: ASTROPHYSICAL JOURNAL vol:886 issue:2 status: published
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::860fa79fad039d438ab0e1272fbac43e
https://hal.archives-ouvertes.fr/hal-03124068
https://hal.archives-ouvertes.fr/hal-03124068
Publikováno v:
The Astrophysical Journal Supplement Series. 255:16