✦ LIBER ✦

The fine structure of the velocity field in a 2B/M2.3 importance flare

✍ Scribed by A. N. Babin; A. N. Koval’

Book ID: 111498147
Publisher: Allerton Press Inc
Year: 2010
Tongue: English
Weight: 382 KB
Volume: 26
Category: Article
ISSN: 0884-5913
DOI: 10.3103/s0884591310030049

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

A strong flare of the H2O maser in Sagit

A strong flare of the H2O maser in Sagittarius B2(M)

✍ O. Ramírez Hernández; E. E. Lekht; A. M. Tolmachev 📂 Article 📅 2005 🏛 Springer 🌐 English ⚖ 349 KB

The fine structure of O2(B 3Σ−u)

✍ T.H. Bergeman; S.C. Wofsy 📂 Article 📅 1972 🏛 Elsevier Science 🌐 English ⚖ 546 KB

The fine-scale structure of the turbulen

The fine-scale structure of the turbulent velocity field

✍ Champagne, F. H. 📂 Article 📅 1978 🏛 Cambridge University Press 🌐 English ⚖ 794 KB

The Magnetic Topological Structure and E

The Magnetic Topological Structure and Energy of the 2B/X2 Flare in NOAA 8100

✍ Yihua Yan; Yang Liu; Maki Akioka; Fengsi Wei 📂 Article 📅 2001 🏛 Springer 🌐 English ⚖ 777 KB

Fine structure of the repolarization cur

Fine structure of the repolarization current in the B 2 phase of a banana compound

✍ Barnik, M. I.; Blinov, L. M.; Shtykov, N. M.; Palto, S. P.; Pelzl, G.; Weissflog 📂 Article 📅 2002 🏛 Taylor and Francis Group 🌐 English ⚖ 296 KB

Dependence of the flare stream velocity

Dependence of the flare stream velocity on magnetic field orientation

✍ M. I. Pudovkin; S. A. Zaitseva; S. P. Puchenkina 📂 Article 📅 1985 🏛 Springer 🌐 English ⚖ 429 KB

The main parameters of a flare stream -its velocity, magnetic field intensity, plasma density, and temperature -are shown to depend on the mutual orientation of magnetic fields in the main body of the stream and within its compressed solar wind region. In particular, the plasma velocity and frozen-i