✦ LIBER ✦

Shrinking and Cooling of Flare Loops in a Two-Ribbon Flare

✍ Scribed by Bojan Vršnak; Manuela Temmer; Astrid Veronig; Marian Karlický; Jun Lin

Publisher: Springer
Year: 2006
Tongue: English
Weight: 609 KB
Volume: 234
Category: Article
ISSN: 0038-0938
DOI: 10.1007/s11207-006-0093-6

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Study of Ribbon Separation and Magnetic

Study of Ribbon Separation and Magnetic Reconnection Rates in a Two-Ribbon Flare

✍ W. Xie; H. Zhang; H. Wang 📂 Article 📅 2008 🏛 Springer 🌐 English ⚖ 772 KB

Cooling of a coronal flare loop through

Cooling of a coronal flare loop through radiation and conduction

✍ Zdeněk Švestka 📂 Article 📅 1987 🏛 Springer 🌐 English ⚖ 431 KB

The magnetohydrodynamic development of t

The magnetohydrodynamic development of two-ribbon flares or a five-finger theory for solar flares

✍ J.S. Kaastra 📂 Article 📅 1984 🏛 Elsevier Science 🌐 English ⚖ 160 KB

Influence of magnetic field structure on

Influence of magnetic field structure on the conduction cooling of flare loops

✍ S. K. Antiochos; P. A. Sturrock 📂 Article 📅 1976 🏛 Springer 🌐 English ⚖ 388 KB

A simple model facilitates calculation of the influence of magnetic field configuration on the conduction cooling rate of a hot post-flare coronal plasma. The magnetic field is taken to be that produced by a line dipole or point dipole at an arbitrary depth below the chromosphere. For the high tempe

Radiative and conductive cooling in a so

Radiative and conductive cooling in a solar flare

✍ Zongjun Ning; Dong Li 📂 Article 📅 2011 🏛 Springer Netherlands 🌐 English ⚖ 477 KB

A numerical experiment relevant to line-

A numerical experiment relevant to line-tied reconnection in two-ribbon flares

✍ T. G. Forbes; E. R. Priest 📂 Article 📅 1983 🏛 Springer 🌐 English ⚖ 953 KB

The nonlinear evolution of a reconnecting magnetic field configuration similar to that occurring just before the onset of'post'-flare loops in two-ribbon flares is determined. The evolution, which is obtained by numerically solving the resistive MHD equations, shows two new features that have not ye