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39 (0,218s)

Project

Space Weather MHD and Empirical Models of the Magnetosheath (ME 386)

. The main attention will be paid to MHD effects as magnetic merging, wave processes University) will use our experimental results for the development of a new MHD......

BL - Fyzika plasmatu a výboje v plynech

  • 2000 - 2002
  • 829 tis. Kč
  • 334 tis. Kč
  • MŠMT
Project

Plasma turbulence at ion scales in the solar wind (GA18-08861S)

spectral and spatial properties of decaying turbulence from large, MHD, scales, starting with the incompressible MHD approximation and extending it to Hall MHD and compressible MHD. Using the expanding box model w...

Astronomy (including astrophysics,space science)

  • 2018 - 2020
  • 3 537 tis. Kč
  • 3 276 tis. Kč
  • GA ČR
Project

Magnetic reconnection in 2D and 3D and its connection to solar surface magnetic activity (IAA300030804)

of electromagnetic fields and plasmas is either ideal or resistive MHD. This project is aimed to calculatestationary reconnection processes in the frame of non-ideal MHD. First the limitations of ideal MHD will be studied ...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2008 - 2010
  • 1 660 tis. Kč
  • 1 660 tis. Kč
  • AV ČR
Project

Waves in expanding magnetic flux tubes in the solar atmosphere (8J18AT031)

of MHD waves. It is very actual topic in solar physics in association to set-up realistic magnetic flux tube atmospheres in an MHD code to model thereafter of MHD waves. b) Investigating the influence of the expansion of f...

Astronomy (including astrophysics,space science)

  • 2018 - 2019
  • 143 tis. Kč
  • 143 tis. Kč
  • MŠMT
Project

Space Weather and Numerical Simulations Application to Predictions (ME 501)

The aim of the project is to determine how magnetohydrodynamic (MHD) simulations can help in predictions of space weather. Simulations will cover modeling of various solar structures, their eruption and propagation through the interplanetary...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2002 - 2004
  • 489 tis. Kč
  • 270 tis. Kč
  • MŠMT
Project

Characterization of MAGE proteins cofactors for E3 ubiquitin ligases? (IAA501630902)

that contain a "MAGE homology domain" (MHD) but have widely differing functions. The Smc5-6 predictions suggest that part of MHD has similarities to cullin components of E3 ligases complexes. We will carry out structural analyses o...

EB - Genetika a molekulární biologie

  • 2009 - 2011
  • 2 893 tis. Kč
  • 2 893 tis. Kč
  • AV ČR
Project

Realistic solar prominence models combining radiative transfer modeling and MHD simulatios (GAP209/12/0906)

We will construct first prominence models employing sophisticated non-LTE radiative transfer modeling to obtain the synthetic radiation emerging from realistically modeled plasma of the prominence fine structures, following the 3D configuration of th...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2012 - 2014
  • 2 925 tis. Kč
  • 2 925 tis. Kč
  • GA ČR
Project

3D tracking of solar fine structures (7AMB16AT010)

as connected traceable 3D structures in MHD simulations. Analyses of their interactions the simulated and observed phenomena and thus evaluate the reliability of MHD simulation of the established collaboration is the development of...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2016 - 2017
  • 36 tis. Kč
  • 36 tis. Kč
  • MŠMT
Project

Qualitative Theory of the MHD and Related Equations (GC22-08633J)

The project is oriented to studies of a wide class of equations of magneto-hydro-dynamics (MHD), modeling flows of electrically conductive fluids (both incompressible and compressible, without or with Hall's effect). The presence of magnetic...

Pure mathematics

  • 2022 - 2023
  • 3 966 tis. Kč
  • 3 966 tis. Kč
  • GA ČR
Project

The role of singular points for magnetic reconnection in solar and space plasmas (GA16-05011S)

in the frame of resistive MHD and different fluid approaches, like Hall-MHD or eventually...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2016 - 2018
  • 1 647 tis. Kč
  • 1 428 tis. Kč
  • GA ČR
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