Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Milan Gošić"'
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 271, Iss 1, p 24 (2024)
We present the most comprehensive collection of stratified-in-optical-depth thermodynamic models of the lower solar atmosphere. This database, named IRIS ^2+ , consists of 40,320 synthetic representative profiles (RPs) and their corresponding represe
Externí odkaz:
https://doaj.org/article/7873101591d24929857ad8d461d7ac63
Autor:
Juan Martínez-Sykora, Jaime de la Cruz Rodríguez, Milan Gošić, Alberto Sainz Dalda, Viggo H. Hansteen, Bart De Pontieu
Publikováno v:
The Astrophysical Journal Letters, Vol 943, Iss 2, p L14 (2023)
The heating of the chromosphere in internetwork regions remains one of the foremost open questions in solar physics. In the present study, we tackle this old problem by using a very-high-spatial-resolution simulation of quiet-Sun conditions performed
Externí odkaz:
https://doaj.org/article/d6df9ccf440643ec9e9e5f18bd48179f
Autor:
Viggo H. Hansteen, Juan Martinez-Sykora, Mats Carlsson, Bart De Pontieu, Milan Gošić, Souvik Bose
Publikováno v:
The Astrophysical Journal, Vol 944, Iss 2, p 131 (2023)
The Mg ii h and k lines are among the best diagnostic tools of the upper solar chromosphere. This region of the atmosphere is of particular interest, as it is the lowest region of the Sun’s atmosphere where the magnetic field is dominant in the ene
Externí odkaz:
https://doaj.org/article/99deab86000a4f25b36edf163aaf749f
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 518:4930-4942
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the origin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54d8557bfbc56334cc051e0699673acb
https://doi.org/10.1093/mnras/stac3352
https://doi.org/10.1093/mnras/stac3352
Autor:
Viggo H. Hansteen, Juan Martinez-Sykora, Mats Carlsson, Bart De Pontieu, Milan Gošić, Souvik Bose
The Mg II h&k lines are amongst the best diagnostic tools of the upper solar chromosphere. This region of the atmosphere is of particular interest as it is the lowest region of the Sun's atmosphere where the magnetic field is dominant in the energeti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9bfe257857e9bb370738b39d64492dc3
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
instname
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Internetwork (IN) magnetic fields are highly dynamic, short-lived magnetic structures that populate the interior of supergranular cells. Since they emerge all over the Sun, these small-scale fields bring a substantial amount of flux, and therefore en
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3720727cde46d28a633d61416b702f0
http://hdl.handle.net/10261/240934
http://hdl.handle.net/10261/240934
Autor:
Kanya Kusano, Erico L. Rempel, Rodrigo A. Miranda, David Ruffolo, Milan Gošić, Abraham C.-L. Chian, Qiang Hu, Daniela Grasso, Heng Q. Feng, Luis R. Bellot Rubio, Pablo R. Muñoz, D. J. Wu, Suzana S. A. Silva, Tiago F. P. Gomes
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Talk delivered in 22nd EGU General Assembly, held online 4-8 May, 2020, id.4289, https://meetingorganizer.copernicus.org/EGU2020/EGU2020-4289.html.-- https://www.egu2020.eu/
The dynamics of solar and interplanetary plasmas is governed by coheren
The dynamics of solar and interplanetary plasmas is governed by coheren
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2fcba7281bededbee2bba09cf557c961
http://hdl.handle.net/10261/238228
http://hdl.handle.net/10261/238228
Autor:
Jayant Joshi, Daniel Nóbrega-Siverio, Vasco Manuel de Jorge Henriques, Clara Froment, H. Skogsrud, Ada Ortiz, Göran B. Scharmer, Eamon Scullion, C. Quintero Noda, Milan Gošić, Georgios Chintzoglou, Mats Carlsson, R. Timmons, Lucia Kleint, Pia Zacharias, Tiago M. D. Pereira, T. Leifsen, M. M. Woods, Viggo Hansteen, Mikolaj Szydlarski, Petra Kohutova, Juan Martinez-Sykora, Gregal J. M. Vissers, Souvik Bose, Ainar Drews, David Graham, Shahin Jafarzadeh, A. Sainz Dalda, D. Schmit, A. Popovas, L. Rouppe van der Voort, J. de la Cruz Rodríguez, B. De Pontieu
Publikováno v:
Astronomy & Astrophysics
NASA's Interface Region Imaging Spectrograph (IRIS) provides high resolution observations of the solar atmosphere through UV spectroscopy and imaging. Since the launch of IRIS in June 2013, we have conducted systematic observation campaigns in coordi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dc9acd3f7a018f7c6cd656cfba6b5ad9
Publikováno v:
The Astrophysical Journal
Inversion codes allow reconstructing a model atmosphere from observations. With the inclusion of optically thick lines that form in the solar chromosphere, such modelling is computationally very expensive because a non-LTE evaluation of the radiation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5ab6bcc9ad79e815eb8ee909fb87dcd5
http://arxiv.org/abs/1904.08390
http://arxiv.org/abs/1904.08390
Autor:
Boris V. Gudiksen, Mats Carlsson, Juan Martinez-Sykora, Bart De Pontieu, Milan Gošić, Viggo Hansteen
The presence of magnetic field is crucial in the transport of energy through the solar atmosphere. Recent ground-based and space-borne observations of the quiet Sun have revealed that magnetic field accumulates at photospheric heights, via a local dy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9a889c103bf0dc232492e627804b2db1
http://arxiv.org/abs/1904.04464
http://arxiv.org/abs/1904.04464