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MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center

Samo za registrovane korisnike
2015
Autori
Vujcić, V.
Jevremović, D.
Mihajlov, A. A.
Ignjatović, Ljubiša M.
Srecković, V. A.
Dimitrijević, M. S.
Malović, Miodrag
Članak u časopisu (Objavljena verzija)
Metapodaci
Prikaz svih podataka o dokumentu
Apstrakt
MOL-D database is a collection of cross-sections and rate coefficients for specific collisional processes and a web service within the Serbian Virtual Observatory (SerVO) and the Virtual Atomic and Molecular Data Center (VAMDC). This database contains photo-dissociation cross-sections for the individual ro-vibrational states of the diatomic molecular ions and rate coefficients for the atom-Rydberg atom chemi-ionization and inverse electron-ion-atom chemi-recombination processes. At the moment it contains data for photodissociation cross-sections of hydrogen H and helium He molecular ions and the corresponding averaged thermal photodissociation cross-sections. The ro-vibrational energy states and the corresponding dipole matrix elements are provided as well. Hydrogen and helium molecular ion data are important for calculation of solar and stellar atmosphere models and for radiative transport, as well as for kinetics of other astrophysical and laboratory plasma (i.e. early Universe).
Ključne reči:
Atomic and molecular processes: photodissociation/association / chemi-ionization/recombination / astronomical databases: miscellaneous / plasmas / spectral line profiles
Izvor:
Journal of Astrophysics and Astronomy, 2015, 36, 4, 693-703
Izdavač:
  • Indian Acad Sciences, Bangalore
Finansiranje / projekti:
  • VAMDC
  • Combination of Collaborative Projects and Coordination and Support Actions Funding Scheme of the Seventh Framework Program
  • Uticaj sudara na spektre astrofizičke plazme (RS-176002)
  • Astroinformatika: primena IT u astronomiji i srodnim disciplinama (RS-44002)

DOI: 10.1007/s12036-015-9344-y

ISSN: 0250-6335

WoS: 000368698700024

Scopus: 2-s2.0-84956623715
[ Google Scholar ]
16
15
URI
http://TechnoRep.tmf.bg.ac.rs/handle/123456789/3059
Kolekcije
  • Radovi istraživača (Inovacioni centar) / Researchers’ publications (Innovation Centre)
Institucija/grupa
Inovacioni centar
TY  - JOUR
AU  - Vujcić, V.
AU  - Jevremović, D.
AU  - Mihajlov, A. A.
AU  - Ignjatović, Ljubiša M.
AU  - Srecković, V. A.
AU  - Dimitrijević, M. S.
AU  - Malović, Miodrag
PY  - 2015
UR  - http://TechnoRep.tmf.bg.ac.rs/handle/123456789/3059
AB  - MOL-D database is a collection of cross-sections and rate coefficients for specific collisional processes and a web service within the Serbian Virtual Observatory (SerVO) and the Virtual Atomic and Molecular Data Center (VAMDC). This database contains photo-dissociation cross-sections for the individual ro-vibrational states of the diatomic molecular ions and rate coefficients for the atom-Rydberg atom chemi-ionization and inverse electron-ion-atom chemi-recombination processes. At the moment it contains data for photodissociation cross-sections of hydrogen H and helium He molecular ions and the corresponding averaged thermal photodissociation cross-sections. The ro-vibrational energy states and the corresponding dipole matrix elements are provided as well. Hydrogen and helium molecular ion data are important for calculation of solar and stellar atmosphere models and for radiative transport, as well as for kinetics of other astrophysical and laboratory plasma (i.e. early Universe).
PB  - Indian Acad Sciences, Bangalore
T2  - Journal of Astrophysics and Astronomy
T1  - MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center
EP  - 703
IS  - 4
SP  - 693
VL  - 36
DO  - 10.1007/s12036-015-9344-y
ER  - 
@article{
author = "Vujcić, V. and Jevremović, D. and Mihajlov, A. A. and Ignjatović, Ljubiša M. and Srecković, V. A. and Dimitrijević, M. S. and Malović, Miodrag",
year = "2015",
abstract = "MOL-D database is a collection of cross-sections and rate coefficients for specific collisional processes and a web service within the Serbian Virtual Observatory (SerVO) and the Virtual Atomic and Molecular Data Center (VAMDC). This database contains photo-dissociation cross-sections for the individual ro-vibrational states of the diatomic molecular ions and rate coefficients for the atom-Rydberg atom chemi-ionization and inverse electron-ion-atom chemi-recombination processes. At the moment it contains data for photodissociation cross-sections of hydrogen H and helium He molecular ions and the corresponding averaged thermal photodissociation cross-sections. The ro-vibrational energy states and the corresponding dipole matrix elements are provided as well. Hydrogen and helium molecular ion data are important for calculation of solar and stellar atmosphere models and for radiative transport, as well as for kinetics of other astrophysical and laboratory plasma (i.e. early Universe).",
publisher = "Indian Acad Sciences, Bangalore",
journal = "Journal of Astrophysics and Astronomy",
title = "MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center",
pages = "703-693",
number = "4",
volume = "36",
doi = "10.1007/s12036-015-9344-y"
}
Vujcić, V., Jevremović, D., Mihajlov, A. A., Ignjatović, L. M., Srecković, V. A., Dimitrijević, M. S.,& Malović, M.. (2015). MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center. in Journal of Astrophysics and Astronomy
Indian Acad Sciences, Bangalore., 36(4), 693-703.
https://doi.org/10.1007/s12036-015-9344-y
Vujcić V, Jevremović D, Mihajlov AA, Ignjatović LM, Srecković VA, Dimitrijević MS, Malović M. MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center. in Journal of Astrophysics and Astronomy. 2015;36(4):693-703.
doi:10.1007/s12036-015-9344-y .
Vujcić, V., Jevremović, D., Mihajlov, A. A., Ignjatović, Ljubiša M., Srecković, V. A., Dimitrijević, M. S., Malović, Miodrag, "MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center" in Journal of Astrophysics and Astronomy, 36, no. 4 (2015):693-703,
https://doi.org/10.1007/s12036-015-9344-y . .

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