Search Results - (Author, Cooperation:S. Barabash)
-
1A. S. Barabash, P. Belli, R. Bernabei, F. Cappella, V. Caracciolo, R. Cerulli, D. M. Chernyak, F. A. Danevich, S. d’Angelo, A. Incicchitti, D. V. Kasperovych, V. V. Kobychev, S. I. Konovalov, M. Laubenstein, D. V. Poda, O. G. Polischuk, V. N. Shlegel, V. I. Tretyak, V. I. Umatov, and Ya. V. Vasiliev
American Physical Society (APS)
Published 2018Staff ViewPublication Date: 2018-11-13Publisher: American Physical Society (APS)Print ISSN: 0556-2821Electronic ISSN: 1089-4918Topics: PhysicsKeywords: Particle Physics ExperimentsPublished by: -
2T. L. Zhang ; Q. M. Lu ; W. Baumjohann ; C. T. Russell ; A. Fedorov ; S. Barabash ; A. J. Coates ; A. M. Du ; J. B. Cao ; R. Nakamura ; W. L. Teh ; R. S. Wang ; X. K. Dou ; S. Wang ; K. H. Glassmeier ; H. U. Auster ; M. Balikhin
American Association for the Advancement of Science (AAAS)
Published 2012Staff ViewPublication Date: 2012-04-12Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
3H. Nilsson ; G. Stenberg Wieser ; E. Behar ; C. S. Wedlund ; H. Gunell ; M. Yamauchi ; R. Lundin ; S. Barabash ; M. Wieser ; C. Carr ; E. Cupido ; J. L. Burch ; A. Fedorov ; J. A. Sauvaud ; H. Koskinen ; E. Kallio ; J. P. Lebreton ; A. Eriksson ; N. Edberg ; R. Goldstein ; P. Henri ; C. Koenders ; P. Mokashi ; Z. Nemeth ; I. Richter ; K. Szego ; M. Volwerk ; C. Vallat ; M. Rubin
American Association for the Advancement of Science (AAAS)
Published 2015Staff ViewPublication Date: 2015-01-24Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
4Delva, M. ; Baumjohann, W. ; Auster, H.-U. ; Carr, C. ; Russell, C. T. ; Barabash, S. ; Balikhin, M. ; Kudela, K. ; Berghofer, G. ; Biernat, H. K. ; Lammer, H. ; Lichtenegger, H. ; Magnes, W. ; Nakamura, R. ; Schwingenschuh, K. ; Volwerk, M. ; Vörös, Z. ; Zambelli, W. ; Fornacon, K.-H. ; Glassmeier, K.-H. ; Richter, I. ; Balogh, A. ; Schwarzl, H. ; Pope, S. A. ; Shi, J. K.
[s.l.] : Nature Publishing Group
Published 2007Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Venus has no significant internal magnetic field, which allows the solar wind to interact directly with its atmosphere2,3. A field is induced in this interaction, which partially shields the atmosphere, but we have no knowledge of how effective that shield is at solar minimum. ...Type of Medium: Electronic ResourceURL: -
5Lundin, R. ; Zakharov, A. ; Pellinen, R. ; Borg, H. ; Hultqvist, B. ; Pissarenko, N. ; Dubinin, E. M. ; Barabash, S. W. ; Liede, I. ; Koskinen, H.
[s.l.] : Nature Publishing Group
Published 1989Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Previous missions to Mars have shown (see, for example, ref. 1) that the interaction with the solar wind forms both a bow shock and a magnetopause. There is2 a smooth transition from the shocked solar-wind plasma to the hot plasma cushion above the ionosphere, which closely resembles the solar-wind ...Type of Medium: Electronic ResourceURL: -
6Sandahl, I. ; Barabash, S. ; Borg, H. ; Budnik, E. Yu. ; Dubinin, E. M. ; Eklund, U. ; Johansson, H. ; Koskinen, H. ; Lundin, K. ; Lundin, R. ; Mostrom, A. ; Pellinen, R. ; Pissarenko, N. F. ; Pulkkinen, T. ; Toivanen, P. ; Zakharov, A. V.
Springer
Published 1997Staff ViewISSN: 0992-7689Source: Springer Online Journal Archives 1860-2000Topics: GeosciencesPhysicsNotes: Abstract PROMICS-3 is a plasma experiment flown in the Russian project Interball. It performs three-dimensional (3D) measurements of ions in the energy range 4 eV–70 keV with mass separation and of electrons in the energy range 12 eV–35 keV. The Interball project consists of two main satellites, the Tail Probe and the Auroral Probe, each with one subsatellite. The Interball Tail Probe was launched on 3 August 1995, into a 65° inclination orbit with apogee at about 30 RE. Both main satellites carry identical PROMICS-3 instruments and thus direct comparisons of the particle distributions will be possible once the Auroral Probe is launched. Furthermore, PROMICS-3-Tail is the first instrument measuring the 3D ion distribution function in the magnetospheric boundary layers at high latitudes. In this paper we describe the PROMICS-3 instrument and show initial results from the Tail probe, measurements of the mag-netosheath, plasma sheet, and ring current plasmas.Type of Medium: Electronic ResourceURL: -
7Sandahl, I. ; Barabash, S. ; Borg, H. ; Budnik, E. Y. ; Dubinin, E. M. ; Eklund, U. ; Koskinen, H. ; Lundin, K. ; Lundin, R. ; Mälkki, A. ; Pellinen, R. ; Pissarenko, N. F. ; Pulkkinen, T. ; Zakharov, A. V.
Springer
Published 1999Staff ViewISSN: 0992-7689Keywords: Magnetospheric physics (auroral phenomena; magnetotail boundary layers; instruments and techniques)Source: Springer Online Journal Archives 1860-2000Topics: GeosciencesPhysicsNotes: Abstract The PROMICS-3 instrument on Interball-2 is nominally identical to the PROMICS-3 instrument on Interball-1. It performs three-dimensional measurements of ions in the energy range 4 eV–70 keV with mass separation and of electrons in the energy range 300 eV–35 keV. Interball-2 was launched on August 29, 1996, into an orbit with the same inclination as that of Interball-1, 63°, but with apogee at 20 000 km. In this study the PROMICS-3 instrument on Interball-2 is briefly described and examples of the first results are presented. Firstly, we report observations of upward moving molecular ions with energies of up to 700 eV at the poleward edge of the auroral oval. Previous observations of outflowing molecular ions have been at lower altitudes and lower energies. Secondly, we show observations of dawnside magnetosheath plasma injections. Using conjugate data from both PROMICS-3 instruments we have found dispersion structures above the morningside auroral oval, which occurred simultaneously with isolated “pockets” of magnetosheath plasma at a distance of XGSM = −14 to −12 RE, which had been injected into the inner part of the low-latitude boundary layer. These isolated plasma structures were sites of strong field-aligned currents and are proposed to be the magnetospheric counterparts of the dispersion structures.Type of Medium: Electronic ResourceURL: