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Dynamics of Quiescent Prominences: Proceedings of the No. 117 Colloquium of the International Astronomical Union, Hvar, SR Croatia, Yugoslavia 1989 [Kõva köide]

  • Formaat: Hardback, 315 pages, kõrgus x laius: 242x170 mm, kaal: 720 g, 105 black & white illustrations, biography
  • Sari: Lecture Notes in Physics Vol 363
  • Ilmumisaeg: 21-Sep-1990
  • Kirjastus: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 354052973X
  • ISBN-13: 9783540529736
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Dynamics of Quiescent Prominences: Proceedings of the No. 117 Colloquium of the International Astronomical  Union, Hvar, SR Croatia, Yugoslavia 1989
  • Formaat: Hardback, 315 pages, kõrgus x laius: 242x170 mm, kaal: 720 g, 105 black & white illustrations, biography
  • Sari: Lecture Notes in Physics Vol 363
  • Ilmumisaeg: 21-Sep-1990
  • Kirjastus: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 354052973X
  • ISBN-13: 9783540529736
Teised raamatud teemal:
For some time to come, this book should be the main source for research in prominences. It surveys the results of the past years, including the "Hvar Reference Atmosphere", which was developed by a panel as a model for quiescent prominences. The reader will find papers on the formation of and physical conditions in prominences, on magnetic fields, on mass motion and energy flow, and on the prominence-corona interface.
Conditions for the formation of prominences as inferred from optical
observations.- Prominence magnetic field observations.- Radio observations of
prominences.- Mass motion in and around prominences.- The prominence-corona
Interface.- Mass and energy flow in prominences.- Support of quiescent
prominences.- Magnetic structure of prominences.- Physical conditions in
prominences.- Diagnostic of prominence magnetic fields.- Formation of a
filament around a magnetic region.- Vector magnetic field and currents at the
footpoint of a loop prominence.- Photospheric field gradient in the
neighbourhood of quiescent prominences.- Evolution of fine structures in a
filament.- Magnetic 'pole-antipole' configuration as an alternative model for
solar plasma loops and sunspots' nature.- On the spatial distribution of
prominence threads.- Micro- and macroinhomogeneities of density in a
quiescent prominence.- High resolution analysis of quiescent prominences at
NSO / Sacramento Peak observatory.- A movie of small-scale Doppler velocities
in a quiescent prominence.- Fibril structure of solar prominences.-
Estimation of the line of sight amplitude of the magnetic field on threads of
an active region prominence.- High resolution observations of motions and
structure of prominence threads.- Observational aspects of a prominence from
HeI 10830 data analysis.- Some observations of the coronal environment of
prominences.- Corona-prominence interface as seen in H-alpha.- Diagnostic
study of prominence- corona interface.- The prominence-corona transition
region analyzed from SL-2 HRTS.- Radio emission from quiescent filaments.-
Dynamical structure of a quiescent prominence.- Dynamics of solar prominence
on December 7, 1978.- Post - flare loops on August 15 - 16, 1989.- Doppler
velocity oscillations in quiescent prominences.- Oscillatory relaxation of an
eruptive prominence.- On oscillations in prominences.- Matter flow velocities
in active region emission loop observed in H- alpha.- Quantitative research
on the velocity field of a loop prominence system.- On the probable
double-loop structure of the flare-like disc object.- An analysis or surges
triggered by a small flare.- Vertical flows in a quiescent filament.-
Distribution of velocities in the pre-eruptive phase of a quiescent
prominence.- Mass motions in a quiescent prominence and an active one.-
Radial velocities of active and quiescent prominences.- Spectral lines
structural features of the active prominence.- An automated procedure for
measurement of prominence transverse velocities.- A three-dimensional model
for solar prominences.- How to form a dip in a magnetic field before the
formation of a solar prominence.- MHD stability of line-tied prominence
magnetic fields.- A model for quiescent solar prominences with normal
polarity.- The nonlinear evolution of magnetized filaments.- Thermal
equilibrium of coronal loops and prominence formation.- Thermal instability
in planar solar coronal structures.- TO The problem of instability of the
solar atmosphere caused by absorption of radiation energy.- Radiative
transfer in cylindrical prominence threads.- HYdrogen line formation in
filamentary prominences.- Toward hydrogen emission in structurally
inhomogeneous prominences.- Linear polarization of hydrogen H? line in
filaments: Method and results of computation.- Multithread structure as a
possible solution for the L? problem in solar prominences.- On the Balmer and
Paschen energy decrements in different brightness prominences.-
Semi-empirical models at different heights of a quiescent prominence.-
Analysis of HeI 10830 a line in a quiescent prominence.- Quiescent filament
"appearances and disappearances".- Numerical simulation of a catastrophe
model for prominence eruptions.- Laws of evolution and destruction of solar
prominences.- Proto-elements of dark solar filaments.- On the behaviour of
the long-living solar filaments.- On some statistical and morphological
characteristics of the quiescent prominences of solar activity cycle N 21.-
Motion of high latitude solar microwave sources and comparison with polar
prominences.- Polar crown filaments and solar differential rotation at high
latitudes.- Hvar reference atmosphere of quiescent prominences.- Plasma
parameters in quiescent prominences.- Summary of IAU colloquium 117, dynamics
of prominences.