✦ LIBER ✦

The excitation temperature of the solar chromosphere determined from molecular spectra

✍ Scribed by D.E. Blackwell

Book ID: 111710813
Publisher: Elsevier Science
Year: 1955
Tongue: English
Weight: 380 KB
Volume: 1
Category: Article
ISSN: 0083-6656
DOI: 10.1016/0083-6656(55)90090-8

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Experiment to determine the temperature

Experiment to determine the temperature structure in the solar chromosphere and corona

✍ C. R. Negus 📂 Article 📅 1972 🏛 Springer Netherlands 🌐 English ⚖ 76 KB

Forbidden lines in spectra of the solar

Forbidden lines in spectra of the solar chromosphere and corona

✍ Carole Jordan 📂 Article 📅 1973 🏛 Elsevier Science ⚖ 519 KB

Solar chromosphere in the D3helium line

Solar chromosphere in the D3helium line from spectra of the eclipse of March 29, 2006

✍ G. P. Marchenko; L. A. Akimov; I. L. Belkina; Yu. I. Velikodsky 📂 Article 📅 2011 🏛 Allerton Press Inc 🌐 English ⚖ 670 KB

Effect of dielectronic recombination exc

Effect of dielectronic recombination excitation in the solar chromosphere-corona transition region

✍ Suresh Chandra 📂 Article 📅 1981 🏛 Elsevier Science 🌐 English ⚖ 631 KB

Determination of the rotational excitati

Determination of the rotational excitation temperature in solar type stars

✍ M. J. Fernández-Figueroa; M. Rego; A. Perea 📂 Article 📅 1982 🏛 Springer Netherlands 🌐 English ⚖ 300 KB

Inhomogeneous structure of the solar chr

Inhomogeneous structure of the solar chromosphere from Lyman-continuum data

✍ J. E. Vernazza; R. W. Noyes 📂 Article 📅 1972 🏛 Springer 🌐 English ⚖ 874 KB

We describe a new model of the chromosphere based on Lyman-continuum observations by Harvard spectrometers aboard the satellites OSO 4 and OSO 6. The model assumes (a) that a random distribution of optically thick inhomogeneities overlies a plane-parallel homogeneous atmosphere, and (b) that the Lym