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The CHIANTI atomic database

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas. George Mason University (USA). University of Michigan (USA). University of Cambridge (UK). CHIANTI consists of a critically evaluated set of up-to-date atomic data, together with user-friendly programs written in Interactive Data Language (IDL) and Python to calculate the spectra from astrophysical plasmas. The CHIANTI package is freely available. If you use the package, we only ask you to appropriately acknowledge CHIANTI.

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The CHIANTI atomic database | chiantidatabase.org Reviews

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An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas. George Mason University (USA). University of Michigan (USA). University of Cambridge (UK). CHIANTI consists of a critically evaluated set of up-to-date atomic data, together with user-friendly programs written in Interactive Data Language (IDL) and Python to calculate the spectra from astrophysical plasmas. The CHIANTI package is freely available. If you use the package, we only ask you to appropriately acknowledge CHIANTI.

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The CHIANTI atomic database | chiantidatabase.org Reviews

https://chiantidatabase.org

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas. George Mason University (USA). University of Michigan (USA). University of Cambridge (UK). CHIANTI consists of a critically evaluated set of up-to-date atomic data, together with user-friendly programs written in Interactive Data Language (IDL) and Python to calculate the spectra from astrophysical plasmas. The CHIANTI package is freely available. If you use the package, we only ask you to appropriately acknowledge CHIANTI.

INTERNAL PAGES

chiantidatabase.org

1

The CHIANTI atomic database

http://www.chiantidatabase.org/chianti_download.html

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas. George Mason University (USA). University of Michigan (USA). University of Cambridge (UK). The CHIANTI package is currently distributed in two ways:. An analysis environment for the solar physics community;. As a stand-alone package downloadable here. We recommend you to use CHIANTI within SolarSoft. And to setup automatic upgrades. It is easy to follow the instructions to download and setup the package.

2

CHIANTI Family

http://www.chiantidatabase.org/family.html

Members of the CHIANTI family. Virtual Observatory Software for Observers. ChiantiPy - Python interface to the CHIANTI database. Chianti on the Web - an interactive web interface to the CHIANTI database.

3

The CHIANTI atomic database

http://www.chiantidatabase.org/help.html

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas. George Mason University (USA). University of Michigan (USA). University of Cambridge (UK). The CHIANTI team has set up a Google Group. Which is used by the team to send new announcements about CHIANTI and is also a place where users can post comments or questions. Once you've joined the group, questions or comments can be sent to chianti@googlegroups.com. He will then send an invitation for you to join the group.

4

The CHIANTI atomic database

http://www.chiantidatabase.org/links.html

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas. George Mason University (USA). University of Michigan (USA). University of Cambridge (UK). The Iron Project has provided atomic data for all of the iron ions. The UK APAP Network. This network has been formed to calculate electron and photon collisional properties with atoms and ions. The NIST spectroscopic database. The Solar Software Library (SolarSoft). A large list of Databases for Atomic and Plasma Physics. A package develope...

5

The CHIANTI atomic database

http://www.chiantidatabase.org/chianti.html

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas. George Mason University (USA). University of Michigan (USA). University of Cambridge (UK). CHIANTI consists of a critically evaluated set of up-to-date atomic data, together with user-friendly programs written in Interactive Data Language (IDL) and Python to calculate the spectra from astrophysical plasmas. The CHIANTI package is freely available. If you use the package, we only ask you to appropriately acknowledge CHIANTI.

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cdsweb.u-strasbg.fr

spaced - a free web template by spyka webmaster

http://cdsweb.u-strasbg.fr/OP.htx

The Iron Project - The Opacity Project. The Opacity Project - The Iron Project. About us - List of members. Atomic and Plasmas physic db. 2008 mySite. Design: spyka webmaster. Available from Just Free Templates. An access to the old version of the Opacity Project database (topbase) as described in the paper by Cunto et al. ( 1993A&A.275L.5C. Is still possible from here.

pyoung.org

CHIANTI, Dr Peter Young

http://www.pyoung.org/chianti

The CHIANTI atomic database. The CHIANTI atomic database was first released in 1996 and is now widely used in Solar Physics and Astronomy. I became involved during the project development phase when I was a PhD student working under Dr Helen Mason at Cambridge University, and I am one of the current five-member team that maintains the database. The CHIANTI team were awarded the Group Achievement Award by the Royal Astronomical Society in 2010. Please visit the main CHIANTI website.

www-amdis.iaea.org

IAEA, NDS AMD Unit Databases

https://www-amdis.iaea.org/databases.php

Databases on Atomic, Molecular and Plasma-Surface Interactions. Databases maintained by the IAEA A M Data Unit. Databases accessed through GENIE. Other A M and PSI databases relevant to Fusion. Further lists of databases for A M and PSI data. Databases maintained by the IAEA A M Data Unit. Since about 2000 the data in AMBDAS. Have been provided almost exclusively by two institutions:. National Institute for Standards and Technology (NIST), Gaithersburg, MD, USA (spectroscopic data). Collision processes d...

labastro.eu

DATABASES - Laboratory Astrophysics

http://www.labastro.eu/databases-.html

DATABASES - Laboratory Astrophysics. 1 Gas phase astrochemistry. 2 Spectroscopy of the ISM. 3 Spectroscopy in hot bodies. 4 Solid state/interstellar ice processes. 5 Stellar and planetary formation. 6 Primitive and planetary material. 7 High energy processes and space plasma. 8 Stellar evolution and nuclear astrophysics. 9 Astrophysical conditions for the emergence of life. Laboratory Astrophysics outside Europe. Atomic Data and Analysis Structure. Atomic and Molecular Bibliographic Data System. Theoreti...

cdsweb.u-strasbg.fr

spaced - a free web template by spyka webmaster

http://cdsweb.u-strasbg.fr/topbase/testop/TheOP.html

The Iron Project - The Opacity Project. OP opacities have been recently revised to include inner-shell contributions [5]. The new data and a suite of easy-to-use codes to compute Rosseland means and radiative accelerations [6] can be downloaded as a tar file below. OPCD 3.3 opserver:. Small tar file with the new software to install OPserver locally. Since the bulky OP data set with monochromatic opacities is not included, only the OPserver version that accesses data remotely from the Ohio Supercomput...

hea-www.cfa.harvard.edu

PINTofALE

http://hea-www.cfa.harvard.edu/PINTofALE

Package for Interactive Analysis of Line Emission. Was originally developed to analyze spectroscopic data from optically-thin coronal plasmas, though much of the software is sufficiently general to be of use in a much wider range of astrophysical data analyses. It is based on a modular set of. Opens up the ` black box' of atomic data required for UV/X-ray analyses and allows the user full control over the data that are used in any given analysis. A more detailed view.). Please note that the. The minimal ...

spaceweather.gmu.edu

Projects | Space Weather Lab

http://www.spaceweather.gmu.edu/category/projects

Department of Physics and Astronomy. Current Space Science Seminars. Archived Space Science Seminars. Space Weather Forecasting Contest. Sub A item 1. Sub B item 1. Sub B item 2. Sub C item 1. Sub C item 2. Sub D item 1. Sub D item 2. Sub D item 3. Sub C item 3. Sub C item 4. Sub C item 5. Sub B item 3. Sub A item 2. Sub A item 3. Sub A item 4. Bob Weigel, Director. Space Weather Lab Network Map. Space Weather Lab Events. Space Weather Lab News. All Space Weather Lab posts. Archived Space Science Seminars.

amdpp.phys.strath.ac.uk

The UK APAP Network

http://amdpp.phys.strath.ac.uk/UK_APAP

The UK APAP Network. The UK APAP (Atomic Processes for Astrophysical Plasmas) Network focuses on the calculation electron and photon collisional data for atoms and ions, intended for astrophysical plasma modelling and spectral analysis. These data are interfaced with the applications of the astrophysical community via databases of fundamental data and derived collisional-radiative rate coefficients, together with level populations, spectral syntheses and line ratios for emission studies. The spac...

grotrian.nsu.ru

Other resources for atomic spectroscopy

http://grotrian.nsu.ru/en/links

Information system Electronic structure of atoms. Other resources for atomic spectroscopy. NIST Atomic Spectra Database. Atomic Molecular and Optical Database Systems (AMODS). The Atomic Line List. Kurucz Atomic Line Database. Energy levels and atomic spectra of ACTINIDES. Atomic Data for Astrophysics (ADfA). The Controlled Fusion Atomic Data Center (CFADC). ALADDIN Database of International Atomic Energy Agency - Nuclear Data Section/Atomic and Molecular Data Unit.

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The CHIANTI atomic database

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas. George Mason University (USA). University of Michigan (USA). University of Cambridge (UK). CHIANTI consists of a critically evaluated set of up-to-date atomic data, together with user-friendly programs written in Interactive Data Language (IDL) and Python to calculate the spectra from astrophysical plasmas. The CHIANTI package is freely available. If you use the package, we only ask you to appropriately acknowledge CHIANTI.

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