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Atomic and ionic spectrum lines below 2000 angstroms : hydrogen through krypton

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This article is published in Journal of Physical and Chemical Reference Data.The article was published on 1987-01-01 and is currently open access. It has received 99 citations till now. The article focuses on the topics: Krypton & Hydrogen.

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Interaction of intense laser pulses with atomic clusters.

TL;DR: In this article, the interaction of intense, femtosecond laser radiation with the large (50{endash}200 A) clusters produced in pulsed gas jets was examined.
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CHIANTI-An Atomic Database for Emission Lines. VII. New Data for X-Rays and Other Improvements

TL;DR: The CHIANTI atomic database as mentioned in this paper contains atomic energy levels, wavelengths, radiative transition probabilities, and collisional excitation data for a large number of ions of astrophysical interest.
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Ultraviolet spectroscopy and remote sensing of the upper atmosphere

TL;DR: A review of the field of airglow analysis can be found in this article, where the basic processes leading to excitation of atomic and molecular energy states are discussed and the current status of knowledge of individual emission features seen in the air glow is examined for the purpose of selecting those species most useful as diagnostics of the state of the upper atmosphere and ionosphere.
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Validation of the UARS solar ultraviolet irradiances: Comparison with the ATLAS 1 and 2 measurements

TL;DR: In this article, the same-day measurements of the solar ultraviolet spectral irradiance made by the two Upper Atmosphere Research Satellite (UARS) solar instruments, SUSIM and SOLAR STellar Irradiance Comparison Experiment (SOLSTICE), are compared with same day measurements by two solar instruments on the shuttle ATmospheric Laboratory for Applications and Science (ATLAS) missions.
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Solar UV and X-ray spectral diagnostics

TL;DR: In this article, a review of the diagnostic methods used to measure electron densities, electron temperatures, differential emission measure (DEM), and relative chemical abundances is presented, focusing on the optically thin emission from the solar atmosphere, mostly found at UV and X-ray (XUV) wavelengths.
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