Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Mehmet Sarp Yalim"'
Autor:
Mehmet Sarp Yalim, Stefaan Poedts
Publikováno v:
Advances in Astronomy, Vol 2014 (2014)
The Sun Watcher Using Active Pixel System Detector and Image Processing (SWAP) telescope and Large Yield Radiometer (LYRA) are the two Sun observation instruments on-board PROBA2. SWAP extreme ultraviolet images, if presented in terms of the integrat
Externí odkaz:
https://doaj.org/article/0e9799df49394627affa82547b60af3c
Context: Resistive Ohmic dissipation has been suggested as a mechanism for heating the solar chromosphere, but few studies have established this association. Aim: We aim to determine how Ohmic dissipation by electric currents can heat the solar chrom
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b44bbdeba6f6b06c272c4cbde714c33
Coronal Mass Ejections (CMEs) are one of the primary drivers of extreme space weather. They are large eruptions of mass and magnetic field from the solar corona and can travel the distance between Sun and Earth in half a day to a few days. Prediction
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f20cb1b79d9afa895ae17742641c64c1
http://arxiv.org/abs/2002.10409
http://arxiv.org/abs/2002.10409
The physics of the solar chromosphere is complex from both theoretical and modeling perspectives. The plasma temperature from the photosphere to corona increases from ~5,000 K to ~1 million K over a distance of only ~10,000 km from the chromosphere a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::241187da643985ccc6c7f0ccc0a6fbea
Publikováno v:
The Astrophysical Journal. 899:L4
The physics of the solar chromosphere is complex from both theoretical and modeling perspectives. The plasma temperature from the photosphere to corona increases from ~5,000 K to ~1 million K over a distance of only ~10,000 km from the chromosphere a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ae59de573478ff08b0101ade3c67d02b
https://doi.org/10.3847/2041-8213/aba69a
https://doi.org/10.3847/2041-8213/aba69a
Coronal Mass Ejections (CMEs) are major drivers of extreme space weather conditions, this being a matter of serious concern for our modern technologically-dependent society. Development of numerical approaches that would simulate CME generation and p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ed7a68623db742b632cf634e0dbcffc6
http://arxiv.org/abs/1807.05310
http://arxiv.org/abs/1807.05310
We have developed a data-driven magnetohydrodynamic (MHD) model of the global solar corona which uses characteristically-consistent boundary conditions (BCs) at the inner boundary. Our global solar corona model can be driven by different observationa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::077b1ba85f1480c7c0fa6536592c84a6
Publikováno v:
Computer Physics Communications. 185:2538-2557
This paper describes an ideal Magnetohydrodynamics (MHD) solver for global magnetospheric simulations based on a B1+B0 splitting approach, which has been implemented within the COOLFluiD platform and adapted to run on modern heterogeneous architectur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f445733caad94d6e87d32930cf1fb25
https://doi.org/10.1016/j.cpc.2014.06.001
https://doi.org/10.1016/j.cpc.2014.06.001
Autor:
Stefaan Poedts, Mehmet Sarp Yalim
Publikováno v:
Advances in Astronomy, Vol 2014 (2014)
The Sun Watcher Using Active Pixel System Detector and Image Processing (SWAP) telescope and Large Yield Radiometer (LYRA) are the two Sun observation instruments on-board PROBA2. SWAP extreme ultraviolet images, if presented in terms of the integrat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::02458dcc049bae430b1ad89a3b448fa6
https://doi.org/10.1155/2014/957461
https://doi.org/10.1155/2014/957461
Simulating Solar Coronal Mass Ejections Constrained by Observations of Their Speed and Poloidal Flux
Publikováno v:
The Astrophysical Journal. 875:L17
We demonstrate how the parameters of a Gibson-Low flux-rope-based coronal mass ejection (CME) can be constrained using remote observations. Our Multi Scale Fluid-Kinetic Simulation Suite (MS-FLUKSS) has been used to simulate the propagation of a CME
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::817a251d192bd8d980fd7a0163ce2742
https://doi.org/10.3847/2041-8213/ab14e9
https://doi.org/10.3847/2041-8213/ab14e9