𝔖 Bobbio Scriptorium
✦   LIBER   ✦

The Misnomer of “Post-Flare Loops”

✍ Scribed by Zdeněk Švestka


Book ID
106532633
Publisher
Springer
Year
2007
Tongue
English
Weight
256 KB
Volume
246
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


📜 SIMILAR VOLUMES


Mass upflows in ‘post’-flare loops
✍ T. G. Forbes; E. R. Priest 📂 Article 📅 1983 🏛 Springer 🌐 English ⚖ 416 KB

A self-consistent numerical model of a reconnecting magnetic field configuration similar to that occurring during the main-phase of two-ribbon flares is used to estimate the upflow caused by the fast-mode expansion of the magnetic field moving into the ~econnection region. Such an expansion creates

X-ray observations of limb flare loops a
✍ Zdenék Švestka; Kermit L. Smith; Keith T. Strong 📂 Article 📅 1992 🏛 Springer 🌐 English ⚖ 374 KB

We present observations of another post-flare arch following an eruptive flare, detected in X-ray lines above the western solar limb on 2 May 1985.

Study of the post-flare loops on 29 July
✍ R. D. Petrasso; J. T. Nolte; M. Gerassimenko; A. S. Krieger; R. Krogstad; F. H. 📂 Article 📅 1979 🏛 Springer 🌐 English ⚖ 931 KB

We use the filter ratio method of analysis to determine spatially resolved values of plasma parameters in the X-ray emitting post-flare loop system which developed on 29 and 30 July 1973. We find that the loops were hotter and had higher plasma pressure at their tops than near their footpoints. The

Study of the post-flare loops on 29 July
✍ Z. Švestka; H. W. Dodson-Prince; S. F. Martin; O. C. Mohler; R. L. Moore; J. T. 📂 Article 📅 1982 🏛 Springer 🌐 English ⚖ 753 KB

We present revised values of temperature and density for the flare loops of 29 July 1973 and compare the revised parameters with those obtained aboard the SMM for the two-ribbon flare of 21 May 1980. The 21 May flare occurred in a developed sunspot group; the 29 July event was a spotless two-ribbon