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741 (0,117s) •

Project

Multi-spectral study of solar filaments and their EUV channels (GAP209/10/1706)

Multi-spectral studies of the filaments and prominences are capable of describing them globally as objects consisting of certain amount of solar plasma. Using such approach the mass loading of the prominence or filament can...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2010 - 2012
    • •
  • 1 265 tis. Kč
    • •
  • 1 265 tis. Kč
    • •
  • GA 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 realistically modeled plasma of the prominence fine structures, following the 3D configuration of the magnetic field within the prominence provided b...

BN - Astronomie a nebeská mechanika, astrofyzika

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

Three-dimensional modelling of quiescent solar prominences (GA16-17586S)

of entire prominences with their multiple fine structures. These models combine together 3D magnetic field simulations with realistic prominence plasma representation to directly relate them with the real-life prominences....

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2016 - 2018
    • •
  • 4 086 tis. Kč
    • •
  • 3 033 tis. Kč
    • •
  • GA ČR
Project

Image Processing of Solar Coronal Event Observation (ME 358)

We proposed to study built-up, evolution, interaction of the coronal flux tubes and to study a coronal mass ejection with the eruptive prominences arising above the active data and data of the ground-based observations of the solar ...

BD - Teorie informace

  • 2000 - 2001
    • •
  • 596 tis. Kč
    • •
  • 380 tis. Kč
    • •
  • MŠMT
Project

Dynamic three-dimensional models of quiescent solar prominences (GA19-16890S)

-of-the-art 3D models of entire prominences with their multiple fine structures. These 3D Whole-Prominence Fine Structure (WPFS) models combine together 3D magnetic field simulations, realistic prominence plasma distributed...

Astronomy (including astrophysics,space science)

  • 2019 - 2022
    • •
  • 3 798 tis. Kč
    • •
  • 3 715 tis. Kč
    • •
  • GA ČR
Project

Science with Solar Orbiter Focusing on eruptive processes (GA22-34841S)

will focus on solar fares, CMEs and related eruptive prominences. We will study the flare heating, multi-wavelength flare emission and relations to CMEs. Eruptive prominencesSolar Orbiter is an ESA-NASA mission wh...

Specific languages

  • 2022 - 2024
    • •
  • 8 672 tis. Kč
    • •
  • 8 672 tis. Kč
    • •
  • GA ČR
Project

Study of hydrogen emission in the solar atmosphere utilizing the SOHO Mission (IAA3003902)

) in structures like solar prominences (mostly quiescent), the quiet chromosphere to different solar atmospheric structures; - To specify which kind of observation by SUMER formation in the solar atmosphere.......

BN - Astronomie a nebeská mechanika, astrofyzika

  • 1999 - 2001
    • •
  • 1 385 tis. Kč
    • •
  • 405 tis. Kč
    • •
  • AV ČR
Project

Multidimensional modeling of polarized spectra of the outer solar atmosphere (GA16-16861S)

One of the most important goals of the solar physics in the coming years will be to understand the magnetism of the outer solar atmosphere (chromosphere, transition region, and corona). Magnetic fields play a significant role in the...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2016 - 2018
    • •
  • 3 667 tis. Kč
    • •
  • 2 719 tis. Kč
    • •
  • GA ČR
Project

Spectropolarimetric modeling and diagnostics of magnetic fields in the upper atmosphere of the quiet Sun (GPP209/12/P741)

is to understand the magnetic coupling of the solar photosphere, chromosphere regions,that cover more than 90% of the solar surface, is important for resolving models of the quiet chromosphere and in the models of quiescent pro...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2012 - 2014
    • •
  • 1 650 tis. Kč
    • •
  • 1 650 tis. Kč
    • •
  • GA ČR
Project

Spectral diagnostics of solr flares and prominences (IAA3003203)

Based on our previous work and extensive experience, we suggest to carry out highly advanced spectroscopic studies of flares and prominences, using most updated methods of non-LTE radiative-transfer theory. We plan to continue the developmen...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2002 - 2006
    • •
  • 2 164 tis. Kč
    • •
  • 1 567 tis. Kč
    • •
  • AV ČR
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