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20 (0,087s)

Project

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

Solar chromosphere belongs to the key aspects of understanding the flare particles and formation of chromospheric lines and continua during solar flares. Using, dynamics, and chromospheric response to presence of return cur...

Astronomy (including astrophysics,space science)

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

Spectroscopic and statistical investigation of the evolution of magnetic bright points (MEB061109)

The aim of this project is analysis of magnetic bright points (MBP), which can be observed in solar photosphere (molecular line CH) and chromosphere (spectral line Ca II H). Observations in these lines will allow us to study the MBPs statist...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2011 - 2012
  • 70 tis. Kč
  • 70 tis. Kč
  • MŠMT
Project

Quiet-Sun Magnetic Fields and Newly Emerging Flux – Dynamics, Energetics, and Upper Atmospheric Response (GC18-08097J)

. The chromospheric response to emerging flux are field-aligned dark structures containing cool the photosphere, over chromosphere and transition region, to the corona, derive its three will investigate how (magneto)acoustic chr...

Astronomy (including astrophysics,space science)

  • 2018 - 2020
  • 4 813 tis. Kč
  • 4 174 tis. Kč
  • GA 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 physics ...

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)

One of the big challenges of astrophysics in the following decades is to understand the magnetic coupling of the solar photosphere, chromosphere, and of the overlying corona. Knowledge of the magnetic field strength and orientation in the qu...

BN - Astronomie a nebeská mechanika, astrofyzika

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

Forward modeling and inversion of polarized solar spectra in multi-dimensional geometries (GA19-20632S)

structure of the solar chromosphere via the forward modeling in realistic atmosphere...

Astronomy (including astrophysics,space science)

  • 2019 - 2022
  • 2 716 tis. Kč
  • 2 716 tis. Kč
  • GA ČR
Project

Development of optical and mechanical systems and methods (IBS1082001)

Project composes of three parts:1. Development of Šolc birefringent K-filter for observation of solar chromosphere. 2. Development of astronomical telescope for high schools. 3. Development of manufacturing and measurement aspherical surface...

BH - Optika, masery a lasery

  • 2000 - 2004
  • 6 700 tis. Kč
  • 6 700 tis. Kč
  • AV 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 and the chromospheric network. Previous work on which this proposal is based was undertaken during......

BN - Astronomie a nebeská mechanika, astrofyzika

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

Research and development of optical and mechanical systems and methotds (1QS100820502)

Project is composed from two parts: 1. Development of the new type of birefringent polarization-interferential filters for observation of solar chromosphere in the set of spectral lines. Development of the new type of quartz filter with the ...

BH - Optika, masery a lasery

  • 2005 - 2009
  • 7 445 tis. Kč
  • 7 445 tis. Kč
  • AV 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 regions on the Sun. For this purpose we intend the digital image processing of...

BD - Teorie informace

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