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pro vyhledávání: '"YALIM, Mehmet Sarp"'
The transport of waves and turbulence beyond the photosphere is central to the coronal heating problem. Turbulence in the quiet solar corona has been modeled on the basis of the nearly incompressible magnetohydrodynamic (NI MHD) theory to describe th
Externí odkaz:
http://arxiv.org/abs/2301.04319
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:
http://arxiv.org/abs/2007.12361
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:
http://arxiv.org/abs/2007.12275
Simulating Solar Coronal Mass Ejections constrained by Observations of their Speed and Poloidal flux
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:
http://arxiv.org/abs/1904.00140
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:
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:
http://arxiv.org/abs/1703.00566
Autor:
YALIM, Mehmet Sarp
Ideal magnetohydrodynamics (MHD) simulations are known to have problems in satisfying the solenoidal constraint (i.e. the divergence of magnetic field should be equal to zero, $ ablacdotvec{B} = 0$). The simulations become unstable unless specific me
Autor:
Yalim, Mehmet Sarp, Zank, Gary, Beck, Christian, Choudhary, Debi Prasad, Prasad, Avijeet, Hu, Qiang, Frisse, Makayla
Publikováno v:
Yalim, Mehmet Sarp Zank, Gary Beck, Christian Choudhary, Debi Prasad Prasad, Avijeet Hu, Qiang Frisse, Makayla . Understanding the heating mechanism of the solar active region atmosphere in chromosphere. Jo
Jo
Jo
Externí odkaz:
http://hdl.handle.net/10852/106792
Publikováno v:
In Computer Physics Communications October 2014 185(10):2538-2557
Autor:
Yalim, Mehmet Sarp1 yalimsarp@hotmail.com, Poedts, Stefaan1
Publikováno v:
Advances in Astronomy. 2014, p1-13. 13p.