Theoretical and Observational Problems Related to Solar Eclipses: Nato Science Series C:, cartea 494
Editat de Z. Mouradian, Magda Stavinschien Limba Engleză Paperback – 14 oct 2012
Din seria Nato Science Series C:
- 18%
Preț: 1182.47 lei - 24%
Preț: 863.31 lei - 18%
Preț: 920.45 lei - 18%
Preț: 919.98 lei - 18%
Preț: 1179.75 lei -
Preț: 381.34 lei -
Preț: 388.40 lei - 18%
Preț: 1191.12 lei - 18%
Preț: 1188.39 lei - 18%
Preț: 1183.84 lei - 18%
Preț: 1181.26 lei - 18%
Preț: 1763.57 lei - 24%
Preț: 1164.99 lei -
Preț: 375.65 lei -
Preț: 399.98 lei - 18%
Preț: 1184.45 lei -
Preț: 379.51 lei - 18%
Preț: 1178.53 lei - 18%
Preț: 1773.75 lei -
Preț: 384.68 lei -
Preț: 415.84 lei -
Preț: 422.98 lei -
Preț: 412.48 lei - 18%
Preț: 1776.49 lei - 18%
Preț: 914.22 lei - 18%
Preț: 1182.47 lei - 18%
Preț: 1188.39 lei -
Preț: 385.79 lei -
Preț: 390.81 lei - 18%
Preț: 1182.94 lei -
Preț: 402.42 lei - 18%
Preț: 1176.11 lei
Preț: 373.24 lei
Nou
Puncte Express: 560
Preț estimativ în valută:
66.05€ • 77.45$ • 58.00£
66.05€ • 77.45$ • 58.00£
Carte tipărită la comandă
Livrare economică 31 ianuarie-14 februarie 26
Preluare comenzi: 021 569.72.76
Specificații
ISBN-13: 9789401063111
ISBN-10: 9401063117
Pagini: 292
Ilustrații: XVIII, 270 p.
Dimensiuni: 160 x 240 x 15 mm
Greutate: 0.41 kg
Ediția:Softcover reprint of the original 1st ed. 1997
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria Nato Science Series C:
Locul publicării:Dordrecht, Netherlands
ISBN-10: 9401063117
Pagini: 292
Ilustrații: XVIII, 270 p.
Dimensiuni: 160 x 240 x 15 mm
Greutate: 0.41 kg
Ediția:Softcover reprint of the original 1st ed. 1997
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria Nato Science Series C:
Locul publicării:Dordrecht, Netherlands
Public țintă
ResearchCuprins
Session 1: Principal scientifique results from the past eclipse observations.- Results from the coronal observations of the 1994 and 1995 total solar eclipses.- Distribution on halfwidths for the green coronal line (5303 Å).- Results of polarization observations of the white-light corona.- Distribution of polarization degree for the solar corona of 03 November 1994.- Fundamental contributions of the solar eclipse observations to solar physics in the second half of the 20th century.- Polarization of the 530.3 nm coronal line as observed on July 11, 1991.- Measurement of the coronal electron temperature at the total solar eclipse on 1994, November 3.- High resolution coronal imaging.- Session 2.: Small and large scale models of coronal structures.- Coronal physics inferred from the analysis of fine structures.- Radiative transfer in atmospheres with randomly distributed inhomogeneities.- Probing the solar atmosphere through radiophysics. A review of eclipse radio observations.- Computation of nonlinear force-free coronal magnetic fields: theory face to observations.- Comparing the large-scale coronal electron density distribution of the 1991 and 1994 solar eclipses.- 2D MHD numerical model for the study of dynamic and magnetic structures in the solar atmosphere.- MHD turbulences in the solar corona.- Post -flare loops in the chromosphere and corona.- Chromospheric and coronal heating mechanisms.- Reconstruction of the large-scale distribution of coronal electrons from eclipse data.- A new understanding of the coronal shape changes during the solar cycle.- Thermal evolution of a coronal condensation.- Medium and large scale structures of the low corona from decimeter and meter wavelength observations.- Session 3.: Low temperature structures in coronal environment.-Filament channels in the corona.- Faint “chromospheric” emission in the solar corona : observational and theoretical problems.- Creation of prominences and filaments — New vista on familiar sunscapes.- Unsolved problems in prominence research.- Session 4: Specific problems of solar eclipse observations.- Eclipse E-corona recording at far distances.- Simulation method to compute accurately the Einstein effect during a total solar eclipse. New ideas.- Emission line spectrum of the solar corona.- A possibility for studying subtelescopic structures in the solar corona.- Eclipse observations relevant to the coronal heating problem.- The indication of neutral hydrogen in the solar corona.- Relevant radio observations during a total solar eclipse.- Session 5.: Tasks for total solar eclipse of 11 August 1999.- NASA bulletin for the total solar eclipse of 1999.- Romanians prepararations for the’ 99 eclipse.- JOSO Working Group 7 : A focal point for collaboration around the 1999 solar eclipse.- A radio observation project for the 1999 solar eclipse.- Romanian projects for the 1999 total solar eclipse.- Session 6.: Instrumental improvement for future observations.- EIT, the Extreme-Ultraviolet Imaging Telescope on board SOHO:first results.- Objectives of a Ukrainian solar-oriented satellite.- A project for infrared observations during the total solar eclipses from the circumterrestrial orbit.- Session 7.: Public education at eclipse and eye safety.- Eye safety during solar eclipses — Myths and realities.- Solar eclipses as a vehicle for international astronomy education.- Variations of geophysical and biological parameters observed at a solar eclipse.- List of Poster Papers.- Notes on General Discussion.- Author Index.