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The collisional atomic processes in geo-cosmical plasmas: data needed for spectroscopy. / Srećković, V. A.; Ignjatović, Lj. M.; Dimitrijević, M. S.; Bezuglov, N. N.; Klyucharev, A. N.

в: Contributions of the Astronomical Observatory Skalnate Pleso, Том 50, № 1, 15.01.2020, стр. 55-65.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Srećković, VA, Ignjatović, LM, Dimitrijević, MS, Bezuglov, NN & Klyucharev, AN 2020, 'The collisional atomic processes in geo-cosmical plasmas: data needed for spectroscopy', Contributions of the Astronomical Observatory Skalnate Pleso, Том. 50, № 1, стр. 55-65. https://doi.org/10.31577/caosp.2020.50.1.55

APA

Srećković, V. A., Ignjatović, L. M., Dimitrijević, M. S., Bezuglov, N. N., & Klyucharev, A. N. (2020). The collisional atomic processes in geo-cosmical plasmas: data needed for spectroscopy. Contributions of the Astronomical Observatory Skalnate Pleso, 50(1), 55-65. https://doi.org/10.31577/caosp.2020.50.1.55

Vancouver

Srećković VA, Ignjatović LM, Dimitrijević MS, Bezuglov NN, Klyucharev AN. The collisional atomic processes in geo-cosmical plasmas: data needed for spectroscopy. Contributions of the Astronomical Observatory Skalnate Pleso. 2020 Янв. 15;50(1):55-65. https://doi.org/10.31577/caosp.2020.50.1.55

Author

Srećković, V. A. ; Ignjatović, Lj. M. ; Dimitrijević, M. S. ; Bezuglov, N. N. ; Klyucharev, A. N. / The collisional atomic processes in geo-cosmical plasmas: data needed for spectroscopy. в: Contributions of the Astronomical Observatory Skalnate Pleso. 2020 ; Том 50, № 1. стр. 55-65.

BibTeX

@article{4b9740754d0b4549a9c4e562b47d1d1c,
title = "The collisional atomic processes in geo-cosmical plasmas: data needed for spectroscopy",
abstract = "The rate coefficients for the chemi-ionization (CI) processes in Na ∗ (n) + Na, Li ∗ (n) + Na, Li ∗ (n) + Li and H ∗ (n) + Li collisions are calculated for wide region of temperatures and the principal quantum numbers. The presented values of the rate coefficients are very useful for the improvement of modelling and analysis of different layers of weakly ionized plasmas in atmospheres of various stars where these and other CI processes could be important and could change the optical characteristics. Also, the results are ofinterest in spectroscopy of low temperature laboratory plasma.",
keywords = "Atomic processes, Planets and satellites: general, Line: profiles, Plasmas, ISM: clouds, CHEMI-IONIZATION PROCESSES, VOLCANIC GASES, NEUTRAL SODIUM, RYDBERG ATOMS, SPECTRUM, LITHIUM, ALKALI, STAR, Atomic processes, – Planets and satellites: general, Line: profiles, Plasmas, ISM: clouds",
author = "Sre{\'c}kovi{\'c}, {V. A.} and Ignjatovi{\'c}, {Lj. M.} and Dimitrijevi{\'c}, {M. S.} and Bezuglov, {N. N.} and Klyucharev, {A. N.}",
note = "Funding Information: This work is made within projects of the Ministry of Education, Science and Technological Development of Serbia 176002 and III44002. Publisher Copyright: {\textcopyright} 2020, Astronomical Institute, Slovak Academy of Sciences.",
year = "2020",
month = jan,
day = "15",
doi = "10.31577/caosp.2020.50.1.55",
language = "Английский",
volume = "50",
pages = "55--65",
journal = "Contributions of the Astronomical Observatory Skalnate Pleso",
issn = "1335-1842",
publisher = "Astronomical Institute, Slovak Academy of Sciences",
number = "1",

}

RIS

TY - JOUR

T1 - The collisional atomic processes in geo-cosmical plasmas: data needed for spectroscopy

AU - Srećković, V. A.

AU - Ignjatović, Lj. M.

AU - Dimitrijević, M. S.

AU - Bezuglov, N. N.

AU - Klyucharev, A. N.

N1 - Funding Information: This work is made within projects of the Ministry of Education, Science and Technological Development of Serbia 176002 and III44002. Publisher Copyright: © 2020, Astronomical Institute, Slovak Academy of Sciences.

PY - 2020/1/15

Y1 - 2020/1/15

N2 - The rate coefficients for the chemi-ionization (CI) processes in Na ∗ (n) + Na, Li ∗ (n) + Na, Li ∗ (n) + Li and H ∗ (n) + Li collisions are calculated for wide region of temperatures and the principal quantum numbers. The presented values of the rate coefficients are very useful for the improvement of modelling and analysis of different layers of weakly ionized plasmas in atmospheres of various stars where these and other CI processes could be important and could change the optical characteristics. Also, the results are ofinterest in spectroscopy of low temperature laboratory plasma.

AB - The rate coefficients for the chemi-ionization (CI) processes in Na ∗ (n) + Na, Li ∗ (n) + Na, Li ∗ (n) + Li and H ∗ (n) + Li collisions are calculated for wide region of temperatures and the principal quantum numbers. The presented values of the rate coefficients are very useful for the improvement of modelling and analysis of different layers of weakly ionized plasmas in atmospheres of various stars where these and other CI processes could be important and could change the optical characteristics. Also, the results are ofinterest in spectroscopy of low temperature laboratory plasma.

KW - Atomic processes

KW - Planets and satellites: general

KW - Line: profiles

KW - Plasmas

KW - ISM: clouds

KW - CHEMI-IONIZATION PROCESSES

KW - VOLCANIC GASES

KW - NEUTRAL SODIUM

KW - RYDBERG ATOMS

KW - SPECTRUM

KW - LITHIUM

KW - ALKALI

KW - STAR

KW - Atomic processes

KW - – Planets and satellites: general

KW - Line: profiles

KW - Plasmas

KW - ISM: clouds

UR - http://www.scopus.com/inward/record.url?scp=85079276532&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/f90e2759-1c2a-32bc-99ae-2f474f04f005/

U2 - 10.31577/caosp.2020.50.1.55

DO - 10.31577/caosp.2020.50.1.55

M3 - статья

VL - 50

SP - 55

EP - 65

JO - Contributions of the Astronomical Observatory Skalnate Pleso

JF - Contributions of the Astronomical Observatory Skalnate Pleso

SN - 1335-1842

IS - 1

ER -

ID: 51202299