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Solar and Stellar Flares

Observations, Simulations, and Synergies

Paperback Engels 2018 9789402414417
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Samenvatting

This volume is a collection of research articles on the subject of solar flares and flares on other cool stars, which are currently extensively studied using new ground- and space-based instruments, together with highly sophisticated numerical simulations. The collection memorializes the work of a pioneer in the study of solar physics, Professor Zdenek Švestka (1925 Prague – 2013 Bunschoten), a leading expert in the field of solar flares and the co-founder and Editor-in-Chief of the journal Solar Physics. The book contains many contributions to the conference “Solar and Stellar Flares: Observations, simulations and synergies”, held in Prague during 23 – 27 June 2014, organised in honor and memory of Professor Švestka.
Originally published as Topical Issue of Solar Physics, Vol. 290, Issue 12, 2015.

Specificaties

ISBN13:9789402414417
Taal:Engels
Bindwijze:paperback
Uitgever:Springer Netherlands

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Inhoudsopgave

Preface.-&nbsp;Švestka’s Research Then and Now.-&nbsp;Extreme Ultra-Violet Spectroscopy of the Lower Solar Atmosphere During Solar Flares (Invited Review).-&nbsp;From Coronal Observations to MHD Simulations, the Building Blocks for 3D Models of Solar Flares (Invited Review).-&nbsp;Flare-CME Models: An Observational Perspective (Invited Review).-&nbsp;New Insights into White-Light Flare Emission from Radiative-Hydrodynamic Modeling of a Chromospheric Condensation.-&nbsp;Mg&nbsp;ii&nbsp;Lines Observed During the X-class Flare on 29 March 2014 by the&nbsp;Interface Region Imaging Spectrograph.-&nbsp;Ionisation Equilibrium for the Non-Maxwellian Electron&nbsp;<br>l; word-wrap: normal; white-space: nowrap; float: none; direction: ltr; max-width: none; max-height: none; min-width: 0px; nn&nbsp;-Distributions in Solar Flares: Updated Calculations.-&nbsp;Particle Acceleration and Plasma Heating in the Chromosphere.-&nbsp;Impulsive Heating of Solar Flare Ribbons Above 10 MK.-&nbsp;Temperature Dependence of the Flare Fluence Scaling Exponent.- Flare Hybrids.-&nbsp;Soft X-Ray Pulsations in Solar Flares.-&nbsp;Triggering an Eruptive Flare by Emerging Flux in a Solar Active-Region Complex.-&nbsp;The Origin of Superflares on G-Type Dwarf Stars of Various Ages.-&nbsp;X-ray Flare Spectra from the DIOGENESS Spectrometer and Its Concept Applied to ChemiX on the Interhelioprobe Spacecraft.

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