The topology and evolution of the Bastille day flare

G Aulanier, EE DeLuca, SK Antiochos… - The Astrophysical …, 2000 - iopscience.iop.org
… role of the multipolar topology created by the null point in creating EUV brightenings before,
during, and after the —are. We also present arguments that the Bastille Day —are can be …

Reevaluation of the magnetic structure and evolution associated with the Bastille day flare on 2000 July 14

H Wang, C Liu, Y Deng, H Zhang - The Astrophysical Journal, 2005 - iopscience.iop.org
flares are associated with a very interesting evolutionary pattern in sunspots: part of the outer
spot structure decays rapidly after major flares… this flare and evolution of magnetic topology

[PDF][PDF] THE TOPOLOGY AND EVOLUTION OF THE BASTILLE DAY FLARE G. AULANIER, 1 EE DELUCA, 2 SK ANTIOCHOS, 1 RA MCMULLEN, 2 AND L. GOLUB2

G AULANIER - THE ASTROPHYSICAL JOURNAL, 2000 - academia.edu
… role of the multipolar topology created by the null point in creating EUV brightenings before,
during, and after the —are. We also present arguments that the Bastille Day —are can be …

Reconnection and energetics in two-ribbon flares: a revisit of the Bastille-day flare

J Qiu, WJ Liu, N Hill… - The Astrophysical …, 2010 - iopscience.iop.org
… magnetic structures and therefore the overall topology and magnetic energy in the field. In
a … relative to the PIL and study the flare ribbon evolution to infer the reconnection pattern, …

A Simple Topological Model of the Bastille Day Flare (2000, July 14)

IV Oreshina, BV Somov - AIP Conference Proceedings, 2004 - pubs.aip.org
… Result of the numerical computation of the flare ribbons. On basis of the topological model,
we examine the evolution of the magnetic field before the flare and estimate the electric field …

A Simple Topological Model of the Bastille Day Flare (July 14, 2000)

IV Oreshina, BV Somov - Solar Magnetic Phenomena: Proceedings of the …, 2005 - Springer
… Then, we assume that the flare is caused by magnetic reconnection in a current layer (…
Based on the topological model, we examine the evolution of the magnetic field before the flare

Flare Plasma Cooling from 30 MK down to 1 MK modeled from Yohkoh, GOES, and TRACE observations during the Bastille Day Event (14 July 2000)

MJ Aschwanden, D Alexander - Solar Physics, 2001 - Springer
… of the evolution of the thermal flare plasma during the 14 July 2000, 10 UT, Bastille Day flare
… of this double-ribbon flare consists of a curved arcade with some 100 post-flare loops which …

[HTML][HTML] The" Bastille Day"; GLE 14 July, 2000 as observed by the worldwide neutron monitor network

AV Belov, JW Bieber, EA Eroshenko… - Proceedings of the …, 2001 - adsabs.harvard.edu
… illustrate development of the EUV post-eruption arcade with … Sun, which revealed itself in a
day as a exclusively geoeffective … Golub, The topology and evolution of the Bastille Day flare. …

The magnetic field topology associated with two M flares

ML Luoni, CH Mandrini, GD Cristiani… - Advances in Space …, 2007 - Elsevier
… and decay at the same place all along the flare duration; the absence of observed ejecta
at the flare location and the Hα kernel evolution indicates that the event is confined. Two of …

Modeling large solar flares

BV Somov, T Kosugi, HS Hudson, T Sakao… - Advances in Space …, 2003 - Elsevier
The basic ideas to model the large solar flares are reviewed and illustrated. Some … large
flares in terms of reconnection. We assume that in the two-ribbon flares, like the Bastille-day flare