Impact of Heavy Ions on the Structure of Current Sheets in the Gravity Field of Exoplanets and Stars

Autor: R. A. Kislov, H. V. Malova, O. V. Khabarova, L. M. Zelenyi, U. P. Antsiferova

Publikováno v: The Astrophysical Journal, Vol 947, Iss 2, p 63 (2023)

Boundary current sheets (CSs) can be formed in collisionless space plasmas in the environment of exoplanets and cold stars. Usually they represent curved surfaces carrying the electric current analogous to the well-known planetary ionospheres, magnet

Externí odkaz: https://doaj.org/article/92bf186ce2484668bacbabc0c2d49056

Formation of Multiple Current Sheets in the Heliospheric Plasma Sheet

Autor: V. Yu. Popov, E. V. Maiewski, A. A. Petrukovich, R. A. Kislov, Olga Khabarova, Lev Zelenyi, Helmi Malova

Publikováno v: Cosmic Research. 58:411-425

When spacecraft cross the heliospheric plasma sheet (HPS) that separates large-scale magnetic sectors of opposite directions in the solar wind, multiple rapid fluctuations in the sign of the magnetic radial component are often observed. These fluctua

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::6bffe0eb25f2a77f97657775c836560a
https://doi.org/10.1134/s0010952520060076

Multi-year statistical analysis of properties of current sheets at 1 AU

Autor: Timothy Sagitov, R. A. Kislov, Gang Li, Olga Khabarova

We use the multi-year open acees database of current sheets identified at 1 AU with the one-second resolution from ACE data (https://csdb.izmiran.ru ) to study properties of current sheets in the solar wind. We find that the CS daily rate (the number

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::4ce231d50a6eac84a2570fe1549c02c5
https://doi.org/10.5194/egusphere-egu21-13510

Current Sheets, Plasmoids and Flux Ropes in the Heliosphere: Part II: Theoretical Aspects

Autor: J. A. le Roux, GuoQing Li, Lev Zelenyi, Sergio Servidio, William H. Matthaeus, Olga Malandraki, Helmi Malova, V. N. Obridko, Roberto Bruno, Antonella Greco, Oreste Pezzi, F. Pecora, N. E. Engelbrecht, V. D. Kuznetsov, R. A. Kislov, Olga Khabarova

Publikováno v: Space science reviews 217 (2021): 39-1–39-70. doi:10.1007/s11214-021-00799-7
info:cnr-pdr/source/autori:Pezzi, O.; Pecora, F.; le Roux, J.; Engelbrecht, N. E.; Greco, A.; Servidio, S.; Malova, H. V.; Khabarova, O. V.; Malandraki, O.; Bruno, R.; Matthaeus, W. H.; Li, G.; Zelenyi, L. M.; Kislov, R. A.; Obridko, V. N.; Kuznetsov, V. D./titolo:Current Sheets, Plasmoids and Flux Ropes in the Heliosphere: Part II: Theoretical Aspects/doi:10.1007%2Fs11214-021-00799-7/rivista:Space science reviews/anno:2021/pagina_da:39-1/pagina_a:39-70/intervallo_pagine:39-1–39-70/volume:217

Our understanding of processes occurring in the heliosphere historically began with reduced dimensionality - one-dimensional (1D) and two-dimensional (2D) sketches and models, which aimed to illustrate views on large-scale structures in the solar win

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::93fc7a011eb84dd4c1bf6fa880ecac9c

Model of Solar Wind in the Heliosphere at Low and High Latitudes

Autor: R. A. Kislov, E. V. Maiewski, V. Yu. Popov, A. A. Petrukovich, Helmi Malova

Publikováno v: Plasma Physics Reports. 44:80-91

The spatial distributions of the magnetic field, plasma density, and current at distances of (20–400)RS from the Sun (where RS is the solar radius) are investigated within a stationary axisymmetric MHD model of the solar wind (SW) at all latitudes

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::74b754db3b007577148ffe8295af212b
https://doi.org/10.1134/s1063780x18010099