Zobrazeno 1 - 10
of 85
pro vyhledávání: '"Andrea Lani"'
Autor:
Błażej Kuźma, Michaela Brchnelova, Barbara Perri, Tinatin Baratashvili, Fan Zhang, Andrea Lani, Stefaan Poedts
Publikováno v:
The Astrophysical Journal, Vol 942, Iss 1, p 31 (2023)
We developed a novel global coronal COCONUT (Coolfluid Corona Unstructured) model based on the COOLFluiD code. The steady-state model is predetermined by magnetograms set as boundary conditions, while inside the numerical domain the corona is describ
Externí odkaz:
https://doaj.org/article/409e6df62997455bab62e2b7830f07be
Autor:
Barbara Perri, Błażej Kuźma, Michaela Brchnelova, Tinatin Baratashvili, Fan Zhang, Peter Leitner, Andrea Lani, Stefaan Poedts
Publikováno v:
The Astrophysical Journal, Vol 943, Iss 2, p 124 (2023)
This paper is dedicated to the new implicit unstructured coronal code COCONUT, which aims at providing fast and accurate inputs for space-weather forecasting as an alternative to empirical models. We use all 20 available magnetic maps of the solar ph
Externí odkaz:
https://doaj.org/article/742c85affe41427aafc55bdac6749e73
Autor:
luis linan, Florian Regnault, Barbara Perri, Michaela Brchnelova, Blazej Kuzma, Andrea Lani, Stefaan Poedts
Some space weather forecasting tools, such as the EUropean Heliosphere FORecasting Information Asset (EUHFORIA), consist of two parts. The first is a semi-empirical coronal model used to create the background solar wind, and the second is a heliosphe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b8107186f45a8dc6a24298278df7b288
https://doi.org/10.5194/egusphere-egu23-17122
https://doi.org/10.5194/egusphere-egu23-17122
Autor:
Barbara Perri, Silke Kennis, Michaela Brchnelova, Tinatin Baratashvili, Blazej Kuzma, Fan Zhang, Andrea Lani, Stefaan Poedts
Connectivity between our star and our planet is a huge but necessary challenge. Indeed, remote-sensing instruments allow us to observe with great details the surface of the Sun, while in-situ measurements let us see the consequences at Earth. However
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b1a79d739ab37bc7d0062c1c85c4e932
https://doi.org/10.5194/egusphere-egu23-3536
https://doi.org/10.5194/egusphere-egu23-3536
Autor:
Adrian F. Daly, Leslie A. Dunnington, David F. Rodriguez-Buritica, Erica Spiegel, Francesco Brancati, Giovanna Mantovani, Vandana M. Rawal, Fabio Rueda Faucz, Hadia Hijazi, Jean-Hubert Caberg, Anna Maria Nardone, Mario Bengala, Paola Fortugno, Giulia Del Sindaco, Marta Ragonese, Helen Gould, Salvatore Cannavò, Patrick Pétrossians, Andrea Lania, James R. Lupski, Albert Beckers, Constantine A. Stratakis, Brynn Levy, Giampaolo Trivellin, Martin Franke
Publikováno v:
Genome Medicine, Vol 16, Iss 1, Pp 1-11 (2024)
Abstract Background X-linked acrogigantism (X-LAG; MIM: 300942) is a severe form of pituitary gigantism caused by chromosome Xq26.3 duplications involving GPR101. X-LAG-associated duplications disrupt the integrity of the topologically associating do
Externí odkaz:
https://doaj.org/article/3554c83b75ce4cf485ca6c1f7161c979
Autor:
Błażej Kuźma, Michaela Brchnelova, Barbara Perri, Tinatin Baratashvili, Fan Zhang, Andrea Lani, Stefaan Poedts
Publikováno v:
The Astrophysical Journal
We developed a novel global coronal COCONUT (Coolfluid Corona Unstructured) model based on the COOLFluiD code. The steady-state model is predetermined by magnetograms set as boundary conditions, while inside the numerical domain the corona is describ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0ac65633c41c363712fa9c78fc24b9da
https://lirias.kuleuven.be/handle/20.500.12942/706340
https://lirias.kuleuven.be/handle/20.500.12942/706340
In the recent years, global coronal models have experienced an ongoing increase in popularity as tools for forecasting solar weather. Within the domain of up to 21.5Rsun, magnetohydrodynamics (MHD) is used to resolve the coronal structure using magne
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f8cd8c07e25b260902b53a0ee2b9b588
https://lirias.kuleuven.be/handle/20.500.12942/705009
https://lirias.kuleuven.be/handle/20.500.12942/705009
Publikováno v:
EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022
Global magnetohydrodynamic (MHD) computational fluid dynamics (CFD) simulations have become an important tool for solar weather research. These simulations use solar magnetogram data to compute structures in the solar corona. We have developed one su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0e60fd965cc7a5bf8b2de688a51b6118
https://doi.org/10.5194/egusphere-egu22-12255
https://doi.org/10.5194/egusphere-egu22-12255
Autor:
Barbara Perri, Peter Leitner, Michaela Brchnelova, Tinatin Baratashvili, Blazej Kuzma, Fan Zhang, Andrea Lani, Stefaan Poedts, Andrey Kochanov, Evangelia Samara, Allan Sacha Brun, Antoine Strugarek
Publikováno v:
EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022
Space weather has the difficult task to try to anticipate the propagation of eruptive events such as coronal mass ejections (CMEs) in order to assess their possible impact on the Earth’s space environment. This requires an accurate description of t