Zobrazeno 1 - 10
of 1 554
pro vyhledávání: '"H, Cowley"'
Autor:
J. D. Nichols, F. Allegrini, F. Bagenal, B. Bonfond, G. B. Clark, J. T. Clarke, J. E. P. Connerney, S. W. H. Cowley, R. W. Ebert, G. R. Gladstone, D. Grodent, D. K. Haggerty, B. Mauk, G. S. Orton, G. Provan, R. J. Wilson
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 20, Pp n/a-n/a (2023)
Abstract We compare Hubble Space Telescope observations of Jupiter's FUV auroras with contemporaneous conjugate Juno in situ observations in the equatorial middle magnetosphere of Jupiter. We show that bright patches on and equatorward of the main em
Externí odkaz:
https://doaj.org/article/f6dba4af42674a78b729ed9ff26a7d26
Autor:
C. J. Farrugia, N. Lugaz, S. Wing, L. B. Wilson, D. J. Sibeck, S. W. H. Cowley, R. B. Torbert, B. J. Vasquez, J. Berchem
Publikováno v:
Frontiers in Physics, Vol 10 (2022)
Global magnetospheric effects resulting from the passage at Earth of large-scale structures have been well studied. The effects of common and short-term features, such as discontinuities and current sheets (CSs), have not been studied in the same dep
Externí odkaz:
https://doaj.org/article/16c1d93e55684c6bb2563ff65fd02b6d
Autor:
Mike Lockwood, Stan W. H. Cowley
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
The response times of the coupled magnetosphere-ionosphere-thermosphere system are, on average, greater than the autocorrelation timescales of solar wind forcing. This means that the system is rarely, if ever, in equilibrium. Departures from equilibr
Externí odkaz:
https://doaj.org/article/110500ee41064dae8c0b4a61da65fe50
Autor:
I. A. Pensionerov, E. S. Belenkaya, S. W. H. Cowley, I. I. Alexeev, V. V. Kalegaev, D. A. Parunakian
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://doaj.org/article/4739c42383e5460faff6255be5f33854
Autor:
E. S. Belenkaya, S. W. H. Cowley, I. I. Alexeev, V. V. Kalegaev, I. A. Pensionerov, M. S. Blokhina, D. A. 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 o
Externí odkaz:
https://doaj.org/article/d2b3a140bc4c4c7d87116d117f444851
Autor:
Konstantin A. Marichev, Nikolai I. Korotkikh, Alan H. Cowley, Vagiz Sh. Saberov, Nataliya V. Glinyanaya, Gennady F. Rayenko, Oles P. Shvaika
Publikováno v:
ARKIVOC, Vol 2017, Iss 4, Pp 365-376 (2017)
Externí odkaz:
https://doaj.org/article/0545ea6f50d54f729c263282a8c74e6d
Publikováno v:
Annales Geophysicae, Vol 35, Pp 505-524 (2017)
We use remote sensing of the proton aurora with the IMAGE-FUV SI12 (Imager for Magnetopause to Aurora Global Exploration–Far Ultraviolet–Spectrographic Imaging at 121.8 nm) instrument and radar measurements of the ionospheric convection from th
Externí odkaz:
https://doaj.org/article/30cee02efab642f29f64063f865230f7
Autor:
E. S. Belenkaya, V. V. Kalegaev, S. W. H. Cowley, G. Provan, M. S. Blokhina, O. G. Barinov, A. A. Kirillov, M. S. Grigoryan
Publikováno v:
Annales Geophysicae, Vol 34, Pp 641-656 (2016)
The paraboloid model of Saturn's magnetosphere describes the magnetic field as being due to the sum of contributions from the internal field of the planet, the ring current, and the tail current, all contained by surface currents inside a magnetop
Externí odkaz:
https://doaj.org/article/1f8833624b21419e8aaadd19c19a6450
Autor:
Owen M. Williams, Alan H. Cowley
Publikováno v:
Acta Crystallographica Section E: Crystallographic Communications, Vol 72, Iss 4, Pp 538-542 (2016)
A trinuclear nickel complex of phenanthrene-9,10-dione dioxime (H2pqd), namely bis[μ2-9,10-bis(oxidoimino)phenanthrene]bis[μ2-10-(oxidoimino)phenanthrene-9-one oxime](phenanthrene-9,10-dione dioxime)trinickel(II) toluene disolvate, [Ni3(C14H8N2O2)2
Externí odkaz:
https://doaj.org/article/9ea9f33f238e4a3e8eed0ed2b4199b95
Publikováno v:
Space Science Reviews. 219
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::51df151dd8268d390269e5c10efd6859
https://doi.org/10.1007/s11214-023-00961-3
https://doi.org/10.1007/s11214-023-00961-3