Magnetic Topology Before a 3b/X1.2 Flare and the Associated CME

Proceedings of the International Astronomical Union - United Kingdom
doi 10.1017/s1743921306002328
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Cambridge University Press (CUP)

Related search

Correlations Between CME Associated Flare Magnitude and in Situ Quantities

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2004English

Flare-Associated Magnetic Activity in the Sun.

Astronomical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1959English

The Stellar CME–Flare Relation: What Do Historic Observations Reveal?

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Simulations of Shock Structures of a Flare/Cme Event in the Low Corona

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2008English

Refinements to Flare Energy Estimates: A Followup to “Energy Partition in Two Solar Flare/Cme Events” by A. G. Emslie Et Al.

Journal of Geophysical Research
GeochemistrySpacePlanetary SciencesOceanographyPaleontologyPetrologySoil ScienceForestryAtmospheric ScienceEcologyGeophysicsAquatic ScienceEarthEarth-Surface ProcessesPlanetary ScienceTechnologyWater Science
2005English

Model of Cme With a Helical Magnetic Field

2019English

Variation of Coronal Magnetic Field and Solar Flare Eruption

2019English

Solar Atmospheric Oscillations and the Chromospheric Magnetic Topology

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

Magnetic Topology and the Heating of Extended Chromospheres

Symposium - International Astronomical Union
1983English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy