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258 (0,097s)

Project

The study of plasma processes in solar flare loops (IAA303404)

BN - Astronomie a nebeská mechanika, astrofyzika

  • 1994 - 1996
  • 559 tis. Kč
  • 858 tis. Kč
  • AV ČR
Project

Slipping magnetic reconnection in solar flares multi-spectral analysis, dynamics, and non-thermal cooling simulations (GA17-16447S)

the flare features observed in different parts of the spectrum. Relationships of the apparent slipping velocities of the flare loops or kernels to other flare features in solar flares, recently confirmed ...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2017 - 2019
  • 5 124 tis. Kč
  • 4 431 tis. Kč
  • GA ČR
Project

Three-dimensional magnetic reconnection in early phases of solar flares and eruptions Observations and the Standard Model in 3D (GA20-07908S)

types are related to observed dynamics, including slippage of flare loops, supraSolar flares are described for a long time by the two-dimensional (2D) Standard of some observed structures. The new Standard solar flare<...

Astronomy (including astrophysics,space science)

  • 2020 - 2023
  • 6 179 tis. Kč
  • 6 179 tis. Kč
  • GA ČR
Project

Cool structures in solar and stellar coronae (GA19-17102S)

Cool structures in solar and stellar coronae, and namely solar prominences, coronal mass ejections (CME) and cool flare loops, have many common aspects and their study requires a combination of top-level observations and numerical s...

Astronomy (including astrophysics,space science)

  • 2019 - 2022
  • 3 515 tis. Kč
  • 3 356 tis. Kč
  • GA ČR
Project

Study of primary eruptive processes in the solar atmosphere (IAA3003707)

the evolution of active prominesces, solar flares and post-flare loops. We suggest to build...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 1997 - 2000
  • 3 156 tis. Kč
  • 1 996 tis. Kč
  • AV ČR
Project

Advanced modelling of solar flare processes and their chromospheric emission (GA19-09489S)

Solar chromosphere belongs to the key aspects of understanding the flare processes because it is the region where majority of the flare radiative output in the flare modelling but relevant to both propagation and energy dep...

Astronomy (including astrophysics,space science)

  • 2019 - 2022
  • 5 151 tis. Kč
  • 4 879 tis. Kč
  • GA ČR
Project

Spectral and image diagnostics of fast processes in solar flares (GA205/96/1199)

in solar flare optical spectra and images. It is closelyrelated to the current theoretical project of numerical simulation of the flare plasma heating. Creation of an up-to-date experiment background for observation of flares

BN - Astronomie a nebeská mechanika, astrofyzika

  • 1996 - 1998
  • 1 046 tis. Kč
  • 666 tis. Kč
  • GA ČR
Project

Diagnostics of primary energy-release processes in solar flares and their modelling (IAA3003202)

in solar flares based on the analysis of X-ray, radi, UV, and optical emissions of solar flares and on their modelling. Data from both present (YOHKOH, SOHO, TRACE to better understand the primary energy-release processes of solar ...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2002 - 2006
  • 4 302 tis. Kč
  • 2 374 tis. Kč
  • AV ČR
Project

Spectropolarimetric diagnostics of fast processes in solar flares (GA205/00/1726)

and extremally short temporal resolution of the Ondoejov Multichannel Flare Spectrograph filtergrams and unpolarized line profiles in solar flares using fast videocameras. The analyzed lines profiles, mainly from starting phases of...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2000 - 2002
  • 2 337 tis. Kč
  • 1 108 tis. Kč
  • GA ČR
Project

Superflares Their origins and connection with planets (GF22-30516K)

Stars exhibit various forms of magnetic activity phenomena, one of the most energetic ones being sudden outbreaks of radiation - flares. Highly energetic flares may it became feasible to study flares on a large number of st...

Astronomy (including astrophysics,space science)

  • 2022 - 2025
  • 6 776 tis. Kč
  • 6 776 tis. Kč
  • GA ČR
  • 1 - 10 out of 258