CHIANTI—An Atomic Database for Emission Lines. V. Comparison with an Isothermal Spectrum Observed with SUMER

Landi, E.; Feldman, U.; P. Dere, K.

doi:10.1086/337949

Public

CHIANTI—An Atomic Database for Emission Lines. V. Comparison with an Isothermal Spectrum Observed with SUMER

Published in The Astrophysical Journal Supplement Series • Mar 1, 2002

Authors:

E. Landi

U. Feldman

K. P. Dere

Abstract

CHIANTI is a database consisting of critically evaluated atomic data and transition probabilities necessary to analyze spectral observations of optically thin plasmas. Previous papers described the content of the database and compared it to a solar active region spectrum between 170 and 450 Å. The a...

Subject

Isothermal process

Database

Spectral line

Research Assistant

AI chat, annotations, notes & similar papers

Finding related papers...

Discussions

(0)

No comments yet

Be the first to share your thoughts!