✦ LIBER ✦

On the stability of the solar chromosphere-corona transition region

✍ Scribed by O. V. Ptitsyna; B. V. Somov

Book ID: 111495585
Publisher: Allerton Press, Inc.
Year: 2011
Tongue: English
Weight: 207 KB
Volume: 66
Category: Article
ISSN: 0027-1349
DOI: 10.3103/s0027134911050122

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

The Solar Quiet Chromosphere—Corona Tran

The Solar Quiet Chromosphere—Corona Transition Region

✍ L. S. Anderson-Huang 📂 Article 📅 1998 🏛 Springer Netherlands 🌐 English ⚖ 527 KB

On the nature of the transition region b

On the nature of the transition region between the solar corona and chromosphere

✍ O. V. Ptitsyna, B. V. Somov 📂 Article 📅 2012 🏛 Springer 🌐 English ⚖ 722 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

Temperature structure of the chromospher

Temperature structure of the chromosphere-corona transition region

✍ G. Elwert; P. K. Raju 📂 Article 📅 1972 🏛 Springer Netherlands 🌐 English ⚖ 69 KB

On the classic heat conduction in the ch

On the classic heat conduction in the chromosphere-corona transition region of the solar atmosphere

✍ O. V. Ptitsyna; B. V. Somov 📂 Article 📅 2010 🏛 Allerton Press, Inc. 🌐 English ⚖ 194 KB

On the origin of spicules in the chromos

On the origin of spicules in the chromosphere-corona transition region

✍ Max Kuperus; R. Grant Athay 📂 Article 📅 1967 🏛 Springer 🌐 English ⚖ 610 KB

Qualitative arguments are presented to show that in the chromosphere-corona transition region the energy which is transported downwards by heat conduction cannot be disposed of by radiative losses only. The region therefore is unstable and forced to be in motion, which may give rise to spicule-like