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Projects

3 199 projects (0,335s)

Project

X-ray Optics for Astrophysics (LH14039)

this type of optics for observing X-ray sources with low intensity (i.e. nucleusThe main goal of this project is to study material and reflective properties of thin substrates for a new design of X-ray op...

BH - Optika, masery a lasery

  • 2014 - 2016
  • 1 868 tis. Kč
  • 1 868 tis. Kč
  • MŠMT
Project

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

prominences. Multi-spectral observations from the X-rays and the ultraviolet, such as the velocities of the ejecta, maximum temperatures and X-ray fluxes, and the dynamics of the X-ray s...

BN - Astronomie a nebeská mechanika, astrofyzika

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

Development of algorithms for X-ray all-sky monitoring with Lobster Eye optics and Timepix detector. (GJ18-10088Y)

This project describes the innovative connection of lobster eye-type optics and uncooled pixel detector Timepix intended for observation of cosmic X-ray radiation can then be observed with X-ray t...

Atomic, molecular and chemical physics (physics of atoms and molecules including collision, interaction with radiation, magnetic resonances, Mössbauer effect)

  • 2018 - 2020
  • 7 645 tis. Kč
  • 7 645 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)

model, which however cannot explain all aspects of X-ray sources, or dynamics of some observed structures. The new Standard solar flare model in 3D has successfully these predictions. To do that, we will utilize multiwavel...

Astronomy (including astrophysics,space science)

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

Geometrical properties of the accretion disc corona in Active Galactic Nuclei (GA17-02430S)

) is their large flux variability in the X-ray energy domain, when the source can change its that the source of this radiation - X-ray corona - is quite small, extending only up to a few the geometrical properties ...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2017 - 2019
  • 4 370 tis. Kč
  • 4 034 tis. Kč
  • GA ČR
Project

Diagnostics of the non-thermal electron distributions in the solar korona (GA205/09/1705)

the intensities of EUV and X-ray spectral lines will be used for analysis of physical plasma theimpulsive phase of solar flares. The X-ray data from RESIK X-ray spectrograph and EUV spectra from ...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2009 - 2011
  • 2 676 tis. Kč
  • 2 676 tis. Kč
  • GA ČR
Project

Galactic gastronomy Green Peas and Blueberries (GA22-22643S)

. Our recent X-ray observations, however, indicated the presence of an AGN in 2/3 Green Peas observed with the European X-ray satellite XMM-Newton. We were awarded new observations of the...

Astronomy (including astrophysics,space science)

  • 2022 - 2024
  • 5 739 tis. Kč
  • 5 739 tis. Kč
  • GA ČR
Project

Effects of general relativity on the micro-variability of X-ray sources (KJB300030703)

Rapid variability of X-ray sources is astrophysically relevant subject, because of X-ray sources. In the first part, we would study lightcurves and power-spectra of oscillating tori in X-ray binar...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2007 - 2009
  • 507 tis. Kč
  • 507 tis. Kč
  • AV ČR
Project

Astrophysical black holes and their environment (GP14-20970P)

and X-ray measurements are available with the European large space laboratory, XMM-Newton, will be studied. Finally, X-ray spectroscopy of a Seyfert galaxy Fairall 51 will be performed. A series of observation...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2014 - 2016
  • 2 325 tis. Kč
  • 2 325 tis. Kč
  • GA ČR
Project

X-ray polarization from accretion discs (LD12010)

This project will focus on the X-ray polarization expected from black hole accretion discs. The polarization in the lamp-post scenario will be investigated. We will be used to simulate the observations with polarimeters onb...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2012 - 2015
  • 1 834 tis. Kč
  • 1 834 tis. Kč
  • MŠMT
  • 1 - 10 out of 3 199