Zobrazeno 1 - 10
of 11
pro vyhledávání: '"O. S. Shalygina"'
Autor:
Alexander T. Basilevsky, E. V. Shalygin, O. S. Shalygina, Wojciech J. Markiewicz, Nataliya V. Bondarenko
Publikováno v:
Icarus. 330:103-122
This work presents a comparative study of microwave properties and 1-μm emissivity for five Venus crater-associated radar-dark parabolas along with neighboring plains and some other geologic units. Craters of interest are Adivar, Bassi, Bathsheba, S
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c3a5735f31e010f4933dc95ffd31dd4e
https://doi.org/10.1016/j.icarus.2019.01.009
https://doi.org/10.1016/j.icarus.2019.01.009
Publikováno v:
Icarus. 299:272-293
From the angular positions of the glory features observed on the upper cloud deck of Venus in three VMC channels (at 0.365, 0.513, and 0.965 µm), the dominating sizes of cloud particles and their refractive indices have been retrieved, and their spa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::eb03c797dcacc3b9303c067a1167f250
https://doi.org/10.1016/j.icarus.2017.08.011
https://doi.org/10.1016/j.icarus.2017.08.011
Publikováno v:
Icarus. 260:190-204
The nature of UV contrasts observed on the upper cloud deck of Venus is still not known. To constrain better the properties of particles that may cause the UV contrasts, the phase dependences of brightness of the venusian clouds measured by the ultra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::27c3b2a4e804c69ce8ededa8c2609777
https://doi.org/10.1016/j.icarus.2015.07.015
https://doi.org/10.1016/j.icarus.2015.07.015
Publikováno v:
Planetary and Space Science. :135-158
During more than 6 years of the Venus Express (VEx) mission, the Venus Monitoring Camera (VMC) took around 300 000 images in four channels covering almost all the latitudes, including night and day sides. Here we give an overview of the VMC data and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d4fc06ec2065079f22f609b6a06ebcd4
https://doi.org/10.1016/j.pss.2014.11.012
https://doi.org/10.1016/j.pss.2014.11.012
Publikováno v:
Planetary and Space Science. :120-134
With the Venus Monitoring Camera onboard the Venus Express orbiter, for the first time full glory on the upper cloud layer of Venus has been imaged. Images were acquired in three wavelengths of 0.365, 0.513, and 0.965 μm. Glory is an optical phenome
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8798e10a513459af833748472c3b8518
https://doi.org/10.1016/j.pss.2014.11.013
https://doi.org/10.1016/j.pss.2014.11.013
Publikováno v:
Research Notes of the AAS. 3:168
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fe0ce4e22bcddfe43ca97027005f088f
https://doi.org/10.3847/2515-5172/ab552b
https://doi.org/10.3847/2515-5172/ab552b
Publikováno v:
Kinematics and Physics of Celestial Bodies. 24:201-208
Peculiarities in the use of CCD matrices for photopolarimetric observations are considered. Algorithms for processing the CCD photopolarimetric and polarimetric observations of Jupiter and other bright extended objects are described with an emphasis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8a63929a91ff81426ae61e34f4b22307
https://doi.org/10.3103/s088459130804003x
https://doi.org/10.3103/s088459130804003x
Autor:
Yu. I. Velikodsky, O. S. Shalygina, L. V. Starukhina, O. M. Starodubtseva, Viktor Korokhin, G. P. Marchenko, E. V. Shalygin, L. A. Akimov
Publikováno v:
Scopus-Elsevier
We present new results obtained from the analysis of the seasonal variations in the asymmetry of polarization of light reflected by Jupiter. From the 23-year set of observations, the anticorrelation between the asymmetries of polarization and insolat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0e6b172d641fca8314401959e370c671
https://doi.org/10.1134/s0038094608010024
https://doi.org/10.1134/s0038094608010024
Autor:
Sanjay S. Limaye, Elean Petrova, Klaus-Dieter Matz, Miguel Almeida, Wojciech J. Markiewicz, Nikolay Ignatiev, D. V. Titov, O. S. Shalygina, Thomas Roatsch
We report on the implications of the observations of the glory phenomenon made recently by Venus Express orbiter. Glory is an optical phenomenon that poses stringent constraints on the cloud properties. These observations thus enable us to constrain
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ba042650f0a0dd1d49701d4efc65d09
https://doi.org/10.1016/j.icarus.2014.01.030
https://doi.org/10.1016/j.icarus.2014.01.030
Autor:
Dmitrij V. Titov, Arianna Piccialli, Wojciech J. Markiewicz, Javier Peralta, Håkan Svedhem, Agustín Sánchez-Lavega, O. S. Shalygina
Publikováno v:
Icarus
Icarus, Elsevier, 2014, 227 (1), pp.94-111. ⟨10.1016/j.icarus.2013.09.012⟩
Icarus, 2014, 227 (1), pp.94-111. ⟨10.1016/j.icarus.2013.09.012⟩
Icarus, Elsevier, 2014, 227 (1), pp.94-111. ⟨10.1016/j.icarus.2013.09.012⟩
Icarus, 2014, 227 (1), pp.94-111. ⟨10.1016/j.icarus.2013.09.012⟩
International audience; High resolution images of Venus Northern hemisphere obtained with the Venus Monitoring Camera (VMC/VEx) allow studying small-scale dynamical phenomena at the cloud tops (∼62-70 km altitude) including features like wave train
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f05a0b6149779d593f7ef27d3410b39e
https://hal.archives-ouvertes.fr/hal-00876202
https://hal.archives-ouvertes.fr/hal-00876202