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Nikolai V. Erkaev

Researcher at Siberian Federal University

Publications -  200
Citations -  5498

Nikolai V. Erkaev is an academic researcher from Siberian Federal University. The author has contributed to research in topics: Magnetohydrodynamics & Solar wind. The author has an hindex of 38, co-authored 197 publications receiving 4872 citations. Previous affiliations of Nikolai V. Erkaev include Saint Petersburg State University & Russian Academy of Sciences.

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Roche lobe effects on the atmospheric loss from "Hot Jupiters"

TL;DR: In this article, the effect of the Roche lobe on the atmospheric loss from short-periodic gas giants was investigated and reasonably accurate approximate formulas to estimate atmospheric loss enhancement due to the action of tidal forces on a hot Jupiter and to calculate the critical temperature for the onset of geometrical blow-off.
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Determining the mass loss limit for close-in exoplanets: what can we learn from transit observations?

TL;DR: In this paper, the authors estimate the position of the pressure balance boundary between Coronal Mass Ejection (CME) and stellar wind ram pressures and the planetary ionosphere pressure for non- or weakly magnetized gas giants at close orbits.
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Origin and loss of nebula-captured hydrogen envelopes from ‘sub’- to ‘super-Earths’ in the habitable zone of Sun-like stars

TL;DR: In this paper, the authors investigated the origin and loss of captured hydrogen envelopes from protoplanets having masses in a range between sub-Earth-like bodies of 0.1 M and super-Earths with 5 M in the habitable zone at 1 au of a Sun-like G star.
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Probing the blow-off criteria of hydrogen-rich 'super-Earths'

TL;DR: In this article, a time-dependent numerical algorithm was applied to solve the system of 1-D fluid equations for mass, momentum, and energy conservation to investigate the criteria under which super-Earths with hydrogen-dominated upper atmospheres can experience hydrodynamic expansion by heating of the stellar XUV (soft X-rays and extreme ultraviolet) radiation and thermal escape via blow-off.