Eruptive solar flares : proceedings of Colloquium No. 133 of the International Astronomical Union held at Iguazú, Argentina, 2 6 August 1991

This is an exhaustive survey of present-day solar research including both theory and observations. It deals with eruptive flares, filament eruption in x-rays and radio waves, energy release and transport, and terrestrial response to solar flares. Details of the most recent SOLAR-A project (launched...

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Opis bibliograficzny
Korporacja: Union astronomique internationale. Colloque :Iguazú
Kolejni autorzy: Švestka, Zdeněk (Dyrektor wydawnictwa), Jackson, Bernard V. (Dyrektor wydawnictwa), Machado, Marcos E. (Dyrektor wydawnictwa)
Format: Livre numérique
Język:Anglais
Wydane: Berlin [etc.] : Springer [20..].
Cham : Springer Nature
Seria:Lecture notes in physics 399
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Edition sous un autre format:• Eruptive Solar Flares, Texte imprimé, 9783540552468
• Eruptive Solar Flares, Texte imprimé, 9783662138731
• Eruptive Solar Flares, Texte imprimé, 9783662138748
Spis treści:
  • History and basic characteristics of eruptive flares
  • Basic magnetic configuration and energy supply processes for an interacting flux model of eruptive solar flares
  • The role of cancelling magnetic fields in the buildup to erupting filaments and flares
  • Variation of the vector magnetic field in an eruptive flare
  • Intrinsically hot flares and a possible connection to deep convective magnetic fields
  • Interaction of large-scale magnetic structures in solar flares
  • The intrinsic relationship between flares and eruption of filament currents
  • Filament eruptions, flaring arches and eruptive flares
  • MHD non-equilibrium: A numerical experiment
  • Triggering of eruptive flares: Destabilization of the preflare magnetic field configuration
  • Field opening and reconnection
  • Energy release at Alfvénic fronts in a force-free magnetic flux tube
  • Energy transport in solar flares: Implications for Ca XIX emission
  • Fluid flow in a jet and the CA XIX line profiles observed during solar flares
  • Characteristics of the impulsive phase of flares
  • Comparison of UV and X-ray solar flare observations and theoretical models
  • White-light flares
  • Post flare loops
  • Plasma parameters derived from MSDP observations of cool flare loops
  • Flare evolution in the density temperature diagram
  • The Neupert Effect: What can i tell us about the impulsive and gradual phases of eruptive flares?
  • Particle acceleration in the impulsive phase of solar flares
  • Kinetic description of electron beams in the chromosphere
  • Nuclear reactions in flares
  • Radio emission of eruptive flares
  • Arcsecond determination of solar burst centers of emission simultaneous to high time resolution and high sensitivity at 48 GHz
  • Trapping and escape of the high energy particles responsible for major protonevents
  • Coronal and interplanetary transport of solar flare protons from the ground level event of 29 september 1989
  • High energetic solar proton flares of 19 to 29 October 1989
  • Large-scale quasi-stationary X-ray coronal structures associated with eruptive solar flares
  • Large scale structures associated with eruptive flares and radio waves
  • Coronal millimeter sources associated with eruptive flares
  • On the association between large scale X-ray brightenings and solar flares
  • A giant post-flare coronal arch observed by Skylab
  • Characteristics of coronal mass ejections
  • The solar sources of coronal mass ejections
  • Remote sensing observations of mass ejections and shocks in interplanetary space
  • In situ observations of coronal mass ejections in interplanetary space
  • Meter-decameter radio emission associated with a coronal mass ejection
  • Models of normal and inverse polarity filament eruptions and coronal mass ejections
  • MHD shocks and simple waves in CMES
  • Terrestrial response to eruptive solar flares: Geomagnetic storms
  • Stellar flares: Confined or eruptive events?
  • Radio flare emission from late-type stars
  • The Solar-A mission experiments and the targets
  • Nobeyama radioheliograph
  • Decimeter high resolution solar radio spectroscope
  • Considerations of a Solar Mass Ejection Imager in a low-earth orbit
  • An Observational-conceptual model of the formation of filaments
  • Dynamics in the prominence-corona transition region from HRTS spectra
  • Active region classifications, complexity, and flare rates
  • Compact sources of suprathermal microwave emission detected in quiescent active regions during lunar occulatations
  • Velocity field in the 13 June 1980 flare area
  • Deformation of magnetic null points
  • The X12 limb flare and spray of 01 June 1991
  • Analysisof X-ray flares observed by the SMM spacecraft
  • Distribution function for electron beams in the chromosphere
  • Sub-second variations of HXR and H-alpha flare emission
  • The role of protons in solar flares
  • High spectral resolution of MM-wavelength (23 18 GHz) solar bursts
  • Microwave flare characteristics in 8 and 3 mm Metsähovi measurements compared with optical and H-alpha data
  • Simultaneous H? and microwave observations of a limb flare on June 20, 1989
  • Nonresonant ion-beam turbulence in solar flares
  • Nonlinear emission mechanism of type III solar radio bursts
  • A numerical simulation of magnetically driven coronal mass ejections
  • Coronal mass ejections: The link between solar and geomagnetic activity
  • A study of geomagnetic variations with periods of four years, six months and 27 days
  • Atmospheric models of flare stars
  • The emerging picture of eruptive solar flares.