Posters NP6.6/AS4.17/ST1.11
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Attendance Time: Friday, 13 April 2018, 17:30–19:00 Hall X4 Chairperson: Giovanni Lapenta |
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X4.286
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EGU2018-2118
Magnetohydrodynamic discontinuities and expansion waves in the outflow region of asymmetric reconnection Boryau Hsupeng, Kun-Han Lee, Lou-Chuang Lee, and Jih-Kwin Chao |
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X4.287
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EGU2018-3485
Multi-spacecraft analysis of the structure of low Mach number, low beta, quasi-perpendicular shocks Oleksandr Goncharov, Jana Safrankova, Zdenek Nemecek, Andriy Koval, Michael Stevens, Adam Szabo, Lubomir Prech, and Maria O. Riazantseva |
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X4.288
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EGU2018-3929
Modeling scale coupling in space turbulence Highlight Giovanni Lapenta, Kirit Makwana, Francesco Pucci, Maria Elena Innocenti, and Diego Gonzalez-Herrero |
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X4.289
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EGU2018-5492
Meteroid collisions as a cause of turbulence in the solar wind Hairong Lai and Christopher T. Russell |
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X4.290
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EGU2018-6597
Arbitrary-order Hilbert spectral analysis and intermittency in solar wind density fluctuations Luca Sorriso-Valvo, Francesco Carbone, Tommaso Alberti, Fabio Lepreti, Christopher H. K. Chen, Zdenek Nemecek, and Jana Safrankova |
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X4.291
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EGU2018-9213
Investigation of interplanetary shock front structure with plasma spectrometer BMSW onboard the SPEKTR-R Natalia Borodkova, Victor Eselevich, Olga Sapunova, Georgy Zastenker, Jana Safrankova, Zdenek Nemecek, and Lubomir Prech |
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EGU2018-14196
Evolution of the magnetic field in quasi-two-dimensional chaotic flow (withdrawn after no-show) Leon Ogorodnikov, Igor Kolokolov, and Vladimir Lebedev |
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X4.293
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EGU2018-18672
Fully kinetic simulations of tangential discontinuities at the Earth magnetopause using the new energy conserving semi-implicit method (solicited) Alfredo Micera, Elisabetta Boella, Diego Gonzalez-Herrero, Andrei Zhukov, and Giovanni Lapenta |
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X4.294
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EGU2018-18870
Properties of relaxing turbulence at sub-proton scales Vyacheslav Olshevsky, Sergio Servidio, Leonardo Primavera, Francesco Pucci, and Giovanni Lapenta |
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X4.295
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EGU2018-18399
Magnetic reconnection driven via forced fluctuations in stable, sheared magnetic configurations Peera Pongkitiwanichakul, Kirit Makwana, and David Ruffolo |