| Date | Event |
|---|---|
| 26 – 30 Aug | 32nd Summer School and International Symposium on the Physics of Ionized Gases (SPIG 2024), Belgrade, Serbia |
| Date | Event |
|---|---|
| 22 – 25 Jul | 22nd International Conference on Atomic Processes in Plasmas (APiP 2023), Tokyo, Japan
Contact: NAKAMURA Nobuyuki Astrophysics Atomic Spectroscopy Collisional-Radiative Processes Collisions in Plasmas CXRS Dense Plasma Physics EBIT Edge Plasma Electron – Ion Collisions Electron Microscopy Experimental Fusion Heavy Particle Collisions High Energy Physics Highly Charged Ions Inertial Confinement Fusion Injected Impurities Ion Beams Laser-Plasma Interactions Line Shapes Non-LTE Processes Plasma Diagnostics Plasma Impurities R-Matrix calculations Radiation Transport Warm Dense Matter X-Ray Spectroscopy |
The Atomic Data and Analysis Structure (ADAS) is an interconnected set of computer codes and data collections for modelling the radiating properties of ions and atoms in plasmas. Its applications are in plasmas in the interstellar medium, and stellar atmospheres, industrial processes, and experimental thermonuclear fusion devices.
URL: http://www.adas.ac.uk/index.php
Host Institution: Department of Physics, University of Strathclyde
Contact: Martin O'MULLANE
Update status: Continuously updated.
ADAS Astrophysics Atomic Spectroscopy Collisional-Radiative Processes Collisions in Plasmas Computational Chemistry Electron – Ion Collisions Electron – Molecule Collisions Electronic Structure Calculations Heavy Particle Collisions Uncertainty Quantification
An atomic database for spectroscopic diagnostics of astrophysical plasmas. The supporting Python software library, ChiantiPy seems to be actively maintained.
URL: https://www.chiantidatabase.org/chianti_linelist.html
Host Institution: Department of Applied Mathematics and Theoretical Physics (DAMTP), University of Cambridge
Contact: Giulio DEL ZANNA
Update status: Last updated: 2015 (version 8.0).
A database of molecular line lists that can be used for spectral characterisation and simulation of exoplanet and cool star atmospheres. Since some line lists in this collection are extremely large (up to 1014 lines), a service to produce absorption cross section data at a user-defined resolution is provided.
URL: http://exomol.com/
Host Institution: University College London (UCL)
Contact: Jonathan TENNYSON
Update status: Continuously updated.
Gestion et Etude des Informations Spectroscopiques Atmosphériques: Management and Study of Spectroscopic Information is a spectroscopic line list database for atmospheric applications with an interactive interface.
URL: https://geisa.aeris-data.fr/
Host Institution: Université Paris-Saclay
Contact: Raymond ARMANTE
Update status: Continuously updated.
The "Grotrian" Electronic Structure of Atoms Information System is a collection of experimental and theoretical data on energy levels and transitions in atoms and ions with an interactive interface maintained by researchers at Novosibirsk State University in Russia.
Contact Email: grotrian@nsu.ru
URL: http://grotrian.nsu.ru/en/
Host Institution: Novosibirsk State University
Contact: Vladislav Kazakov
Update status: Continuously updated.
Astrophysics Atomic Spectroscopy Computational Chemistry Electronic Structure Calculations
A companion database to the CDMS catalogue, this is a compilation of rotational transition frequencies and intensities of molecules of astrophysical interest.
URL: https://spec.jpl.nasa.gov/ftp/pub/catalog/catform.html
Host Institution: Jet Propulsion Laboratory
Contact: Brian DROUIN
Update status: Continuously updated.
The Kinetic Database for Astrochemistry is a database of kinetic data of interest for astrochemical (interstellar medium and planetary atmospheres) studies.
URL: http://kida.astrophy.u-bordeaux.fr/
Host Institution: Laboratoire d'Astrophysique de Bordeaux
Contact: Pierre GRATIER
Update status: Continuously updated.
Atomic and molecular spectroscopic line data for a number of astrophysically interesting species, including energy levels, statistical weights, Einstein A-coefficients and collisional rate coefficients.
URL: https://home.strw.leidenuniv.nl/~moldata/
Host Institution: Leiden University
Contact: Floris VAN DER TAK
Update status: Continuously updated.
A database of electron- and ion-scattering cross sections, swarm parameters, reaction rates, energy distribution functions and other data required for modelling low-temperature plasmas initiated in 2010 by researchers at Laboratoire des Plasmas et Conversion d’Energie (LAPLACE), a laboratory operated jointly by the CNRS, the University of Toulouse and the Institut Polytechnique of Toulouse.
Contact Email: info@lxcat.net
URL: https://fr.lxcat.net/data/set_type.php
Host Institution: Eindhoven University of Technology (Technische Universiteit Eindhoven, TU/e)
Contact: Jan VAN DIJK
Update status: Continuously updated.
Astrophysics Collisional-Radiative Processes Collisions in Plasmas Electron – Ion Collisions Electron – Molecule Collisions Low Temperature Plasmas
A database of photodissociation cross sections with an interactive interface, run by the Institute of Physics Belgrade and Astronomical Observatory Belgrade.
URL: http://servo.aob.rs/mold/
Host Institution: University of Belgrade
Contact: None
Update status: Continuously updated.
Two databases: TIPbase, containing fine-structure atomic data computed for ions of astrophysical interest; and TOPbase, an online atomic database created as part of the Opacity Project.
URL: https://tiptopbase.obspm.fr/
Host Institution: Paris Observatory (Observatoire de Paris)
Contact: Claudio MENDOZA
Update status: Last updated: although the database itself may not have been updated for some time (2009?), the data service itself continues to run effectively.
The UMIST Database for Astrochemistry contains reaction rate coefficient data for species of astrophysical interest, with a particular emphasis on hydrocarbons and their ions.
URL: http://udfa.ajmarkwick.net/
Host Institution: University of Manchester
Contact: Andrew MARKWICK
Update status: Last updated: 2012.
The Vienna Atomic Line Database (VALD) is a collection of atomic and molecular transition parameters of astronomical interest. Now identifying as VALD3, it is provided by mirrored servers in Uppsala, Sweden, Vienna, Austria, and Moscow, Russia.
Host Institution: Uppsala University
Contact: Nikolai PISKUNOV
Update status: Continuously updated.