Application of a dielectric breakdown induced by high-power lasers for a laboratory simulation of meteor plasma. Experimental Astronomy
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00098639%3A_____%2F21%3AN0000002" target="_blank" >RIV/00098639:_____/21:N0000002 - isvavai.cz</a>
Result on the web
<a href="https://www.researchgate.net/publication/348947998_Application_of_a_dielectric_breakdown_induced_by_high-power_lasers_for_a_laboratory_simulation_of_meteor_plasma" target="_blank" >https://www.researchgate.net/publication/348947998_Application_of_a_dielectric_breakdown_induced_by_high-power_lasers_for_a_laboratory_simulation_of_meteor_plasma</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s10686-020-09688-3" target="_blank" >10.1007/s10686-020-09688-3</a>
Alternative languages
Result language
angličtina
Original language name
Application of a dielectric breakdown induced by high-power lasers for a laboratory simulation of meteor plasma. Experimental Astronomy
Original language description
Spectra of meteor plasma, their dynamics and dominant spectral features are usually a subject of mathematical modelling and computations. In our study, on the other hand, we describe and evaluate the advantages and limitations of the experimental techniques employed for meteor spectra simulations. The experiments are performed by ablating meteorite samples using a series of laser sources, i.e. a large terawatt−class gas laser infrastructure PALS, a high-power Ti:Sapphire femtosecond laser, and laboratory Nd:YAG and ArF excimer lasers. We demonstrate that, notwithstanding the importance of theoretical spectra computation, laboratory experiments may remarkably enhance the qualitative and quantitative evaluation of the meteor emission spectra measured, as well as the assignment of important spectral features therein. We also perform completing experiments to compare the laser-target interaction observed with the expected dynamics of evaporation and disintegration of a real meteoroid body.
Czech name
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Czech description
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Classification
Type
J<sub>ost</sub> - Miscellaneous article in a specialist periodical
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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Continuities
V - Vyzkumna aktivita podporovana z jinych verejnych zdroju
Others
Publication year
2021
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Experimental Astronomy
ISSN
1572-9508
e-ISSN
1572-9508
Volume of the periodical
2021
Issue of the periodical within the volume
51.2
Country of publishing house
NL - THE KINGDOM OF THE NETHERLANDS
Number of pages
27
Pages from-to
425-451
UT code for WoS article
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EID of the result in the Scopus database
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