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MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center
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 indivi...
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Published in: | Journal of astrophysics and astronomy 2015-12, Vol.36 (4), p.693-703, Article 0 |
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container_issue | 4 |
container_start_page | 693 |
container_title | Journal of astrophysics and astronomy |
container_volume | 36 |
creator | Vujčič, V. Jevremović, D. Mihajlov, A. A. Ignjatović, Lj. M. Srećković, V. A. Dimitrijević, M. S. Malović, M. |
description | 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
2
+
and helium He
2
+
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). |
doi_str_mv | 10.1007/s12036-015-9344-y |
format | article |
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2
+
and helium He
2
+
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).</description><identifier>ISSN: 0250-6335</identifier><identifier>EISSN: 0973-7758</identifier><identifier>DOI: 10.1007/s12036-015-9344-y</identifier><language>eng</language><publisher>New Delhi: Springer India</publisher><subject>Astronomy ; Astrophysics ; Astrophysics and Astroparticles ; Cross sections ; Data centers ; Helium ; Hydrogen ; Ionization ; Ions ; Kinetics ; Mathematical models ; Molecular ions ; Molecules ; Observations and Techniques ; Photodissociation ; Physics ; Physics and Astronomy ; Plasma ; Review ; Web services</subject><ispartof>Journal of astrophysics and astronomy, 2015-12, Vol.36 (4), p.693-703, Article 0</ispartof><rights>Indian Academy of Sciences 2015</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c486t-4554197390719b2746e4a935183717c37bbc82f2de762693b2354be2ea4c7513</citedby><cites>FETCH-LOGICAL-c486t-4554197390719b2746e4a935183717c37bbc82f2de762693b2354be2ea4c7513</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttps://hal.science/hal-02400515$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Vujčič, V.</creatorcontrib><creatorcontrib>Jevremović, D.</creatorcontrib><creatorcontrib>Mihajlov, A. A.</creatorcontrib><creatorcontrib>Ignjatović, Lj. M.</creatorcontrib><creatorcontrib>Srećković, V. A.</creatorcontrib><creatorcontrib>Dimitrijević, M. S.</creatorcontrib><creatorcontrib>Malović, M.</creatorcontrib><title>MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center</title><title>Journal of astrophysics and astronomy</title><addtitle>J Astrophys Astron</addtitle><description>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
2
+
and helium He
2
+
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).</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Astrophysics and Astroparticles</subject><subject>Cross sections</subject><subject>Data centers</subject><subject>Helium</subject><subject>Hydrogen</subject><subject>Ionization</subject><subject>Ions</subject><subject>Kinetics</subject><subject>Mathematical models</subject><subject>Molecular ions</subject><subject>Molecules</subject><subject>Observations and Techniques</subject><subject>Photodissociation</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Plasma</subject><subject>Review</subject><subject>Web services</subject><issn>0250-6335</issn><issn>0973-7758</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqN0U1L7DAUBuAiV9Cr_gB3ATfeRTSfTeNumPELRlwougxpPONEMo03aZX597ZWRATBVUJ43sMhb1HsU3JECVHHmTLCS0yoxJoLgdcbxTbRimOlZPWnvzNJcMm53Cr-5vxECNWC6e3CXl3P8ewETdA0huCzj40NaGZbW9sMyDYP6B5qdAPpxTtAr75d-ga1S0B3PrVdbydtXHn3Lq9iANcFm94HoCk0LaTdYnNhQ4a9j3OnuD07vZ1e4Pn1-eV0MsdOVGWLhZSC9gtroqiumRIlCKu5pBVXVDmu6tpVbMEeQJWs1LxmXIoaGFjhlKR8p_g3jl3aYJ6TX9m0NtF6czGZm-GNMEGIpPJlsIejfU7xfwe5NSufHYRgG4hdNlRpzjRjVP-CllLLquIDPfhGn2KX-u8clNSaiJLIXtFRuRRzTrD4XJYSM1RpxipNX6UZqjTrPsPGTO5t8wjpy-QfQ2-h1pzK</recordid><startdate>20151201</startdate><enddate>20151201</enddate><creator>Vujčič, V.</creator><creator>Jevremović, D.</creator><creator>Mihajlov, A. 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A. ; Ignjatović, Lj. M. ; Srećković, V. A. ; Dimitrijević, M. S. ; Malović, M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c486t-4554197390719b2746e4a935183717c37bbc82f2de762693b2354be2ea4c7513</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Astrophysics and Astroparticles</topic><topic>Cross sections</topic><topic>Data centers</topic><topic>Helium</topic><topic>Hydrogen</topic><topic>Ionization</topic><topic>Ions</topic><topic>Kinetics</topic><topic>Mathematical models</topic><topic>Molecular ions</topic><topic>Molecules</topic><topic>Observations and Techniques</topic><topic>Photodissociation</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Plasma</topic><topic>Review</topic><topic>Web services</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Vujčič, V.</creatorcontrib><creatorcontrib>Jevremović, D.</creatorcontrib><creatorcontrib>Mihajlov, A. A.</creatorcontrib><creatorcontrib>Ignjatović, Lj. M.</creatorcontrib><creatorcontrib>Srećković, V. A.</creatorcontrib><creatorcontrib>Dimitrijević, M. 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A.</au><au>Ignjatović, Lj. M.</au><au>Srećković, V. A.</au><au>Dimitrijević, M. S.</au><au>Malović, M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center</atitle><jtitle>Journal of astrophysics and astronomy</jtitle><stitle>J Astrophys Astron</stitle><date>2015-12-01</date><risdate>2015</risdate><volume>36</volume><issue>4</issue><spage>693</spage><epage>703</epage><pages>693-703</pages><artnum>0</artnum><issn>0250-6335</issn><eissn>0973-7758</eissn><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
2
+
and helium He
2
+
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).</abstract><cop>New Delhi</cop><pub>Springer India</pub><doi>10.1007/s12036-015-9344-y</doi><tpages>11</tpages></addata></record> |
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subjects | Astronomy Astrophysics Astrophysics and Astroparticles Cross sections Data centers Helium Hydrogen Ionization Ions Kinetics Mathematical models Molecular ions Molecules Observations and Techniques Photodissociation Physics Physics and Astronomy Plasma Review Web services |
title | MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center |
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