
Proceedings Paper
Astroclimate of specialized stations of the Large Solar Vacuum Telescope: Part IFormat | Member Price | Non-Member Price |
---|---|---|
$17.00 | $21.00 |
Paper Abstract
The paper presents the results of measurements of characteristics of local astroclimate in special production areas of the
Large solar vacuum telescope (the Baikal astrophysical observatory of the Institute of Solar-Terrestrial Physics SB
RAS). It is demonstrated that the temperature gradients in the telescope rooms are the cause of the initiation of the
Benard cell and originating (incipient) turbulence in the pavilion of the astronomical spectrograph. The characteristics of
the originating turbulence were studied in detail. It has been found that the measurements date have supported the basic
scenarios of stochastization (Landau-Hopf, Ruelle-Takens, Feigenbaum, Pomeau-Menneville scenarios). The
Feigenbaum bifurcation diagram has experimentally been supported. It is shown that the basic vortex in Benard cell
breaks down into smaller vortices as the result of ten bifurcations of the period duplication. It has been found that the
originating turbulence introduced large errors in the data of spectral measurements, even at the path of small length. The
horizontal random displacements of spectral lines, appearing due to the pavilion effects, in the horizontal Ebert scheme
can reach 1 second of arc. In this case the line displacements occur slowly, at the frequency about 0.01 Hz. Because of
low frequencies of line displacements the originating turbulence by its optical characteristics approximated the regular
refraction.
Paper Details
Date Published: 22 April 2008
PDF: 11 pages
Proc. SPIE 6936, Fourteenth International Symposium on Atmospheric and Ocean Optics/Atmospheric Physics, 69360P (22 April 2008); doi: 10.1117/12.783158
Published in SPIE Proceedings Vol. 6936:
Fourteenth International Symposium on Atmospheric and Ocean Optics/Atmospheric Physics
Gennadii G. Matvienko; Victor A. Banakh, Editor(s)
PDF: 11 pages
Proc. SPIE 6936, Fourteenth International Symposium on Atmospheric and Ocean Optics/Atmospheric Physics, 69360P (22 April 2008); doi: 10.1117/12.783158
Show Author Affiliations
V. V. Nosov, Institute of Atmospheric Optics (Russia)
V. M. Grigoriev, Institute of Solar-Terrestrial Physics (Russia)
P. G. Kovadlo, Institute of Solar-Terrestrial Physics (Russia)
V. M. Grigoriev, Institute of Solar-Terrestrial Physics (Russia)
P. G. Kovadlo, Institute of Solar-Terrestrial Physics (Russia)
V. P. Lukin, Institute of Atmospheric Optics (Russia)
E. V. Nosov, Institute of Atmospheric Optics (Russia)
A. V. Torgaev, Institute of Atmospheric Optics (Russia)
E. V. Nosov, Institute of Atmospheric Optics (Russia)
A. V. Torgaev, Institute of Atmospheric Optics (Russia)
Published in SPIE Proceedings Vol. 6936:
Fourteenth International Symposium on Atmospheric and Ocean Optics/Atmospheric Physics
Gennadii G. Matvienko; Victor A. Banakh, Editor(s)
© SPIE. Terms of Use
