Zobrazeno 1 - 10
of 13
pro vyhledávání: '"David Parunakian"'
Publikováno v:
Universe, Vol 7, Iss 10, p 355 (2021)
In this paper we consider an unusual structure, twice observed at the magnetopause of Mercury, and called the “Double Magnetopause”. Presumably, it is associated with a current sheet created by Na+ ions. Two alternative scenarios are considered.
Externí odkaz:
https://doaj.org/article/a0b60c697e5e459faf34dc14542f51d0
The goal of this work is to improve our understanding of Mercury's magnetosphere and its dynamics. The magnetosphere of Mercury is rather small and highly dynamic due to its weak internal magnetic field and its close proximity to the Sun. The changin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bec0e78838701ea38926cc8cf3be1de0
https://doi.org/10.5194/egusphere-egu22-12762
https://doi.org/10.5194/egusphere-egu22-12762
Publikováno v:
Universe, Vol 7, Iss 355, p 355 (2021)
In this paper we consider an unusual structure, twice observed at the magnetopause of Mercury, and called the “Double Magnetopause”. Presumably, it is associated with a current sheet created by Na+ ions. Two alternative scenarios are considered.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4f86b15a220b67e97e9c09f53cfb33bb
https://www.mdpi.com/2218-1997/7/10/355
https://www.mdpi.com/2218-1997/7/10/355
Autor:
Alexander Lavrukhin, David Parunakian, Dmitry Nevsky, Sahib Julka, Michael Granitzer, Andreas Windisch, Ute Amerstorfer
Publikováno v:
European Planetary Science Congress 2021
The magnetosphere of Mercury is relatively small and highly dynamic, mostly due to the weak planetary magnetic field. Varying solar wind conditions principally determine the location of both the Hermean bow shock and magnetopause. In 2011 – 2015 ME
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::49882875b7f09653a13ee677d01cb758
https://doi.org/10.5194/epsc2021-651
https://doi.org/10.5194/epsc2021-651
Autor:
Elena Belenkaya, Stanley W. H. Cowley, Ivan Pensionerov, David Parunakian, Igor Alexeev, Vladimir Kalegaev
Publikováno v:
Annales Geophysicae, Vol 37, Pp 101-109 (2019)
One of the main features of Jupiter's magnetosphere is its equatorial magnetodisc, which significantly increases the field strength and size of the magnetosphere. Analysis of Juno measurements of the magnetic field during the first 10 orbits covering
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77ac4da77cf3e6ad01432a22b8bcf676
https://doi.org/10.5194/angeo-37-101-2019
https://doi.org/10.5194/angeo-37-101-2019
Autor:
Rachel L. Bailey, Christian Möstl, Ute Amerstorfer, Andreas Windisch, Alexander Lavrukhin, Sahib Julka, Dmitry Nevskiy, Michael Granitzer, Martin A. Reiss, David Parunakian
Publikováno v:
EGU General Assembly 2021
During its 2011-2015 lifetime the MESSENGER spacecraft completed more than 4000 orbits around Mercury, producing vast amounts of information regarding the planetary magnetic field and magnetospheric processes. During each orbit the spacecraft left an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d97ffd06bb910182373c2eb71c6c7e6
Jovian magnetosphere has a huge equatorial plasma disk, which is also known as the current sheet or magnetodisk. This current sheet enlarges the subsolar magnetosphere size more than twice compare to purely planetary dipole magnetosphere. Near to the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4383d24f29d7d6bc1eeb7ad4794627a1
https://doi.org/10.5194/epsc2020-615
https://doi.org/10.5194/epsc2020-615
Automatic detection of magnetopause and bow shock crossing signatures in MESSENGER magnetometer data
Autor:
Alexander Lavrukhin, David Parunakian, Dmitry Nevskiy, Ute Amerstorfer, Andreas Windisch, Sahib Julka, Christian Möstl, Martin Reiss, Rachel Bailey
Publikováno v:
Europlanet Science Congress 2020
The magnetosphere of Mercury is rather small and highly dynamic, due to its weak internal magnetic field and its close proximity to the Sun. The changing solar wind conditions principally determine the locations of both the Hermean bow shock and magn
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cdf6c4272c03cb9688069b61700459b4
https://doi.org/10.5194/epsc2020-826
https://doi.org/10.5194/epsc2020-826
Autor:
Markku Alho, Maxim L. Khodachenko, Elena Belenkaya, S. Dyadechkin, Igor Alexeev, Esa Kallio, David Parunakian
Publikováno v:
Cosmic Research. 56:108-114
Several types of numerical models are used to analyze the interactions of the solar wind flow with Mercury’s magnetosphere, including kinetic models that determine magnetic and electric fields based on the spatial distribution of charges and curren
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a42ba7e98f219a442353fccf7d226f65
https://doi.org/10.1134/s0010952518020028
https://doi.org/10.1134/s0010952518020028
Autor:
M. S. Blokhina, Ivan Pensionerov, Igor Alexeev, Vladimir Kalegaev, Elena Belenkaya, Stanley W. H. Cowley, David Parunakian
Publikováno v:
Annales Geophysicae, Vol 35, Pp 1293-1308 (2017)
A wide variety of interactions take place between the magnetized solar wind plasma outflow from the Sun and celestial bodies within the solar system. Magnetized planets form magnetospheres in the solar wind, with the planetary field creating an obsta
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::27ed2d5def42d525dad0d1db9c912039
https://doi.org/10.5194/angeo-35-1293-2017
https://doi.org/10.5194/angeo-35-1293-2017