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State specific recombination of astrophysically important ions with electrons (GA23-05439S)
conditions prevailing in interstellar plasma. In the temperature range 40 - 150 K of the studied ions in the afterglow plasma. The unique combination of experimental techniques will allow us to obtain key parameters for
Astronomy (including astrophysics,space science)
- 2023 - 2025 •
- 7 562 tis. Kč •
- 6 714 tis. Kč •
- GA ČR
Řešení projektu: 1. 1. 2023 - 31. 12. 2025
Uznané náklady
Podpora ze státního rozpočtu (89%)
Poskytovatel: Grantová agentura České republiky
Recombination of state selected H3+ ions at temperatures relevant for cold interstellar plasma – experimental study from 200 K down to 30 K (GA15-15077S)
of interstellar molecular clouds and provides a useful probe for physical conditions therein of H3+ ions in these interstellar plasmatic environments. Stationary afterglow......
BL - Fyzika plasmatu a výboje v plynech
- 2015 - 2017 •
- 3 819 tis. Kč •
- 3 819 tis. Kč •
- GA ČR
Řešení projektu: 1. 1. 2015 - 31. 12. 2017
Uznané náklady
Podpora ze státního rozpočtu (100%)
Poskytovatel: Grantová agentura České republiky
Dissociative recombination of H3+ ions with electrons in conditions of cosmic plasma (GA205/02/0610)
H3+ is a key ion in astrophysical plasmas, where it serves as the cornerstone astrophysical plasmas. Up to now obtained values of the rate coefficient cannot explain diffuse interstellar clouds. Our recent experimental resu...
BN - Astronomie a nebeská mechanika, astrofyzika
- 2002 - 2004 •
- 2 378 tis. Kč •
- 1 048 tis. Kč •
- GA ČR
Řešení projektu: 1. 1. 2002 - 1. 1. 2004
Uznané náklady
Podpora ze státního rozpočtu (44%)
Poskytovatel: Grantová agentura České republiky
Astrophysical plasma in laboratory (GA22-05935S)
models of interstellar plasma, which differ for CH+ by several orders of magnitude (obtained by microwave plasma diagnostics) in the afterglow plasma. The output......
Atomic, molecular and chemical physics (physics of atoms and molecules including collision, interaction with radiation, magnetic resonances, Mössbauer effect)
- 2022 - 2024 •
- 5 933 tis. Kč •
- 5 423 tis. Kč •
- GA ČR
Řešení projektu: 1. 1. 2022 - 31. 12. 2024
Uznané náklady
Podpora ze státního rozpočtu (91%)
Poskytovatel: Grantová agentura České republiky
Theoretical description of electron-driven molecular processes in plasma. (GA16-17230S)
of interstellar medium, planetary and stellar atmospheres and nuclear fusion plasmaThis project is devoted to theoretical description of fundamental reactive processes in plasma, which are either driven by collisions of el...
BG - Jaderná, atomová a molekulová fyzika, urychlovače
- 2016 - 2018 •
- 5 269 tis. Kč •
- 3 794 tis. Kč •
- GA ČR
Řešení projektu: 1. 1. 2016 - 31. 12. 2018
Uznané náklady
Podpora ze státního rozpočtu (72%)
Poskytovatel: Grantová agentura České republiky
Recombination of H3+, D3+, HD2+ and H2D+ ions with electrons in hydrogen plasma (GA202/02/0948)
Stationary Afterglow (AISA) plasma reactor with highly sensitive and specific in the decaying plasma for specific initial quantum states thus providing extremly valuable enviroment of the interstellar clouds. The experimen...
BL - Fyzika plasmatu a výboje v plynech
- 2002 - 2004 •
- 4 013 tis. Kč •
- 1 544 tis. Kč •
- GA ČR
Řešení projektu: 1. 1. 2002 - 1. 1. 2004
Uznané náklady
Podpora ze státního rozpočtu (38%)
Poskytovatel: Grantová agentura České republiky
Inelastic collisions of molecules with cold electrons (KJB400400803)
are dominant for a cooling (or heating) of the molecules inside cold plasmas or interstellar clouds. The theoretical approach will be used to determine state-to-state......
CF - Fyzikální chemie a teoretická chemie
- 2008 - 2010 •
- 1 780 tis. Kč •
- 1 780 tis. Kč •
- AV ČR
Řešení projektu: 1. 1. 2008 - 31. 12. 2010
Uznané náklady
Podpora ze státního rozpočtu (100%)
Poskytovatel: Akademie věd České republiky
From laboratory to space generation and spectroscopic characterization of interstellar molecules (GJ19-25116Y)
New radioastronomical observations open new challenges, also covered in this project: the identification of the carriers of the unknown lines in the interstellar characterize prebiotic and complex organic molecules in the interstellar
Atomic, molecular and chemical physics (physics of atoms and molecules including collision, interaction with radiation, magnetic resonances, Mössbauer effect)
- 2019 - 2022 •
- 3 137 tis. Kč •
- 3 137 tis. Kč •
- GA ČR
Řešení projektu: 1. 1. 2019 - 30. 6. 2022
Uznané náklady
Podpora ze státního rozpočtu (100%)
Poskytovatel: Grantová agentura České republiky
Solar wind as a natural laboratory structure, turbulence, and shocks. (GA16-04956S)
Solar wind can be considered as a natural laboratory for a study of processes in magnetized plasmas and the results of such studies can be scaled to diverse environments ranging from interstellar medium through plasmas in i...
BL - Fyzika plasmatu a výboje v plynech
- 2016 - 2018 •
- 4 900 tis. Kč •
- 3 080 tis. Kč •
- GA ČR
Řešení projektu: 1. 1. 2016 - 31. 12. 2018
Uznané náklady
Podpora ze státního rozpočtu (63%)
Poskytovatel: Grantová agentura České republiky
Reactions of hydroxyl anion OH– in interstellar medium, experimental astrochemistry (GA20-22000S)
The project is focused on a deeper understanding of the reactions of ions and molecules that influence the presence of the hydroxyl anion OH– in the interstellar clouds, this ion has not yet been detected in the interstellar environ...
Atomic, molecular and chemical physics (physics of atoms and molecules including collision, interaction with radiation, magnetic resonances, Mössbauer effect)
- 2020 - 2022 •
- 6 433 tis. Kč •
- 5 872 tis. Kč •
- GA ČR
Řešení projektu: 1. 1. 2020 - 31. 12. 2022
Uznané náklady
Podpora ze státního rozpočtu (91%)
Poskytovatel: Grantová agentura České republiky
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