Main spectral features of meteors studied using a terawatt-class high-power laser

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21340%2F19%3A00347614" target="_blank" >RIV/68407700:21340/19:00347614 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/68378271:_____/19:00517287 RIV/61388955:_____/19:00517287 RIV/61389021:_____/19:00517287 RIV/00216208:11310/19:10409813

Výsledek na webu

<a href="https://doi.org/10.1051/0004-6361/201935816" target="_blank" >https://doi.org/10.1051/0004-6361/201935816</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1051/0004-6361/201935816" target="_blank" >10.1051/0004-6361/201935816</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Main spectral features of meteors studied using a terawatt-class high-power laser

Popis výsledku v původním jazyce

Context. Meteor spectra are commonly interpreted using data from databases and tables. Several studies have demonstrated very sophisticated calculations of elemental compositions of meteoroid bodies based on the computation of synthetic meteor spectra or on the spectral analysis of airglow plasma containing evaporated, atomized, and ionized meteoroid matter. However, considering accuracy, reliability of computations, lack of laboratory experimental data in this field, as well as the complicated physical structure of meteor plasma, such qualitative assignment or quantitative calculations are still extensively discussed in the scientific community. Even on the laboratory level, many studies have shown the high complexity of the acquisition and interpretation of the data that are recorded with techniques of emission spectroscopy that are in fashion and philosophy similar to the spectral analysis of meteor plasma, that is, detection and quantification of the elements that are ablated from complicated multicomponent matrices.

Název v anglickém jazyce

Main spectral features of meteors studied using a terawatt-class high-power laser

Popis výsledku anglicky

Context. Meteor spectra are commonly interpreted using data from databases and tables. Several studies have demonstrated very sophisticated calculations of elemental compositions of meteoroid bodies based on the computation of synthetic meteor spectra or on the spectral analysis of airglow plasma containing evaporated, atomized, and ionized meteoroid matter. However, considering accuracy, reliability of computations, lack of laboratory experimental data in this field, as well as the complicated physical structure of meteor plasma, such qualitative assignment or quantitative calculations are still extensively discussed in the scientific community. Even on the laboratory level, many studies have shown the high complexity of the acquisition and interpretation of the data that are recorded with techniques of emission spectroscopy that are in fashion and philosophy similar to the spectral analysis of meteor plasma, that is, detection and quantification of the elements that are ablated from complicated multicomponent matrices.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/EF16_019%2F0000778" target="_blank" >EF16_019/0000778: Centrum pokročilých aplikovaných přírodních věd</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Rok uplatnění

2019

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Astronomy & Astrophysics

ISSN

0004-6361

e-ISSN

1432-0746

Svazek periodika

630

Číslo periodika v rámci svazku

A127

Stát vydavatele periodika

FR - Francouzská republika

Počet stran výsledku

20

Strana od-do

—

Kód UT WoS článku

000516616800001

EID výsledku v databázi Scopus

2-s2.0-85073202712