Photoionized plasmas in laboratory: a connection to astrophysics and planetary sciences

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F15%3A00310758" target="_blank" >RIV/68407700:21230/15:00310758 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/61389021:_____/15:00455695 RIV/68407700:21340/15:00310758 RIV/68378271:_____/15:00521909

Výsledek na webu

<a href="http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=2293866" target="_blank" >http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=2293866</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1117/12.2182032" target="_blank" >10.1117/12.2182032</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Photoionized plasmas in laboratory: a connection to astrophysics and planetary sciences

Popis výsledku v původním jazyce

In this work photoionized plasmas were created by irradiation of atomic and molecular gases by soft X-ray and extreme ultraviolet intense radiation pulses. Two different laser-produced plasma sources, employing a low energy Nd:YAG laser system (NL 129) and a high energy iodine laser system (PALS), were used for creation of photoionized plasmas. In both cases the SXR/EUV beam irradiated the gas stream, injected into a vacuum chamber synchronously with the radiation pulse. Radiation spectra, measured for photoionized plasmas produced in Ne and Ar gases, are dominated by L-shell emission lines except the Ne plasma produced using the high energy system where K-shell emission dominates. Additionally electron density measurements were performed by laser interferometry employing a femtosecond laser system synchronized with the irradiating system. Maximum electron density for Ne plasma, induced using the high energy system, reached 2.10(18)cm(-3). In case of employing the low energy system a detection limit was too high for interferometric measurements, thus only an upper estimation for electron density could be made.

Název v anglickém jazyce

Photoionized plasmas in laboratory: a connection to astrophysics and planetary sciences

Popis výsledku anglicky

In this work photoionized plasmas were created by irradiation of atomic and molecular gases by soft X-ray and extreme ultraviolet intense radiation pulses. Two different laser-produced plasma sources, employing a low energy Nd:YAG laser system (NL 129) and a high energy iodine laser system (PALS), were used for creation of photoionized plasmas. In both cases the SXR/EUV beam irradiated the gas stream, injected into a vacuum chamber synchronously with the radiation pulse. Radiation spectra, measured for photoionized plasmas produced in Ne and Ar gases, are dominated by L-shell emission lines except the Ne plasma produced using the high energy system where K-shell emission dominates. Additionally electron density measurements were performed by laser interferometry employing a femtosecond laser system synchronized with the irradiating system. Maximum electron density for Ne plasma, induced using the high energy system, reached 2.10(18)cm(-3). In case of employing the low energy system a detection limit was too high for interferometric measurements, thus only an upper estimation for electron density could be made.

Druh

D - Stať ve sborníku

CEP obor

—

OECD FORD obor

10306 - Optics (including laser optics and quantum optics)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2015

Kód důvěrnosti údajů

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

Název statě ve sborníku

EUV and X-ray Optics: Synergy between Laboratory and Space IV

ISBN

978-1-62841-631-2

ISSN

0277-786X

e-ISSN

—

Počet stran výsledku

10

Strana od-do

—

Název nakladatele

SPIE

Místo vydání

Bellingham (stát Washington)

Místo konání akce

Praha

Datum konání akce

13. 4. 2015

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

000356859800021