Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Igor Ognev"'
Publikováno v:
Geophysical Journal International. 232:322-342
SUMMARY Volgo–Uralia is the easternmost segment of the East European Craton. It accommodates the Volga–Ural petroleum province where the maturity of source rocks is tightly related to the temperature distribution in the crust. Numerous heat flow
Autor:
Igor Ognev
Publikováno v:
SOCAR Proceedings. :135-140
In the last two decades in conjunction with the development of satellite gravimetry, the techniques of regional-scale inverse and forward gravity modeling started to be more actively incorporated in the construction of crustal and lithospheric scale
Autor:
Alexey Stepanov, Igor Ognev
Publikováno v:
Georesursy, Vol 23, Iss 4, Pp 51-57 (2021)
The relationship between the various human activities and seismic activity has become more evident in the last several decades. One of the important domains where such a relationship manifests itself is hydrocarbon fields’ development. South East T
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 517(3), 4022-4033
Geometry and dynamical structure of emission regions in accreting pulsars are shaped by the interplay between gravity, radiation, and strong magnetic field, which significantly affects the opacities of a plasma and radiative pressure under such extre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::247bbaab2c6714777896dbdc01419b47
http://arxiv.org/abs/2210.09995
http://arxiv.org/abs/2210.09995
Publikováno v:
Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021).
Autor:
Alexandra Dobrynina, Igor Ognev
Publikováno v:
Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021).
Volgo–Uralia is a Neoarchaean easternmost part of the East European craton. Recent seismic studies of the Volgo–Uralian region provided new insights into the crustal structure of this area. In this study, we combine satellite gravity and seismic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cf4e41e4ce22c508cecfb5cd5febdc23
https://se.copernicus.org/articles/13/431/2022/
https://se.copernicus.org/articles/13/431/2022/
One of the models explaining the high luminosity of pulsing ultra-luminous X-ray sources (pULXs) was suggested by Mushtukov et al. (2015). They showed that the accretion columns on the surfaces of highly magnetized neutron stars can be very luminous
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79b80f1f5283b7d1c8c67fc78806d32c
Publikováno v:
13TH INTERNATIONAL SCIENTIFIC CONFERENCE ON AERONAUTICS, AUTOMOTIVE AND RAILWAY ENGINEERING AND TECHNOLOGIES (BulTrans-2021).