Zobrazeno 1 - 10
of 77
pro vyhledávání: '"Mikhail Malkov"'
Publikováno v:
The Astrophysical Journal, Vol 973, Iss 1, p 27 (2024)
The observed energy spectra of accelerated particles at interplanetary shocks often do not match the diffusive shock acceleration (DSA) theory predictions. In some cases, the particle flux forms a plateau over a wide range of energies, extending upst
Externí odkaz:
https://doaj.org/article/b89b0286020e47e3be2d0ced6593cba0
Publikováno v:
SCIENCE AND SPORT: current trends. 8:72-81
The aim is to determine the ratio of low physical activity (PA) to a high sedentary behavior (SB) and to change it in the experiment. Methods and organization of the research. We carried out descriptive (n = 425) and cross-sectional (n = 36) experime
Publikováno v:
Environmental Economics and Sustainable Development. :6-13
The article focuses on the results of a new analysis conducted by the World Bank, according to which the COVID-19 pandemic threatens not only economic development, but also the achievements of the last decade in the fields of health and education, en
Autor:
Mikhail Malkov, Martin Lemoine
A shock wave propagating perpendicularly to an ambient magnetic field accelerates particles considerably faster than in the parallel propagation regime. However, the perpendicular acceleration stops after the shock overruns a circular particle orbit.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4aab90fe399b2c15ec45281f728b85df
Autor:
Igor V. Moskalenko, Mikhail Malkov
Publikováno v:
Astrophys J
A recently observed bump in the cosmic ray (CR) spectrum from 0.3--30 TV is likely caused by a stellar bow shock that reaccelerates \emph{preexisting} CRs, which further propagate to the Sun along the magnetic field lines. Along their way, these part
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c4cb53eb995e688832364e5da0c0afd
http://arxiv.org/abs/2010.02826
http://arxiv.org/abs/2010.02826
Autor:
Mikhail Malkov, Martin Lemoine
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 499 (4), pp.4972-4983. ⟨10.1093/mnras/staa3131⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 499 (4), pp.4972-4983. ⟨10.1093/mnras/staa3131⟩
Numerical simulations of particle acceleration in magnetized turbulence have recently observed powerlaw spectra where pile-up distributions are rather expected. We interpret this as evidence for particle segregation based on acceleration rate, which
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b16d3859aaa722ddd2f91fb9a7b3cba7
https://hal.archives-ouvertes.fr/hal-02939997
https://hal.archives-ouvertes.fr/hal-02939997
In situ observations of energetic particles at the Earth's bow-shock that are attainable by the satellite missions have long created the opinion that electrons are most efficiently accelerated in a quasi-perpendicular shock geometry. However, shocks
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::63dc79a0dd9674a41493dc4214415fd3
http://arxiv.org/abs/2007.06478
http://arxiv.org/abs/2007.06478
Chemistry of Ion Injection in SNR Shocks: Hybrid Simulations in the Light of He/C/O Data from AMS-02
Publikováno v:
Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019).
The Chemical composition of cosmic rays is a powerful tool for identifying the mechanisms of their acceleration. In addition to protons and He ions, recent AMS-02 observations also provide the high-precision rigidity spectra of C and O. They widen th
Publikováno v:
Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019).
In situ observations of energetic particles at the Earth's bow-shock have long created an opinion that electrons are most efficiently accelerated (injected) in a quasi-perpendicular, while protons in quasi-parallel shock geometry. Shocks that deemed
Publikováno v:
Physics of Plasmas. 27:122113
The collision of two expanding plasma flows is investigated with an emphasis on the mixing flow. The study adheres to laboratory experiments where two Ohmically exploding parallel wires launch hot plasma coronas toward each other. The interpenetratio