Zobrazeno 1 - 10
of 249
pro vyhledávání: '"Hadid, L."'
Autor:
Mousis, O., Bouquet, A., Langevin, Y., André, N., Boithias, H., Durry, G., Faye, F., Hartogh, P., Helbert, J., Iess, L., Kempf, S., Masters, A., Postberg, F., Renard, J. -B., Vernazza, P., Vorburger, A., Wurz, P., Atkinson, D. H., Barabash, S., Berthomier, M., Brucato, J., Cable, M., Carter, J., Cazaux, S., Coustenis, A., Danger, G., Dehant, V., Fornaro, T., Garnier, P., Gautier, T., Groussin, O., Hadid, L. Z., Ize, J. -C., Kolmasova, I., Lebreton, J. -P., Maistre, S. Le, Lellouch, E., Lunine, J. I., Mandt, K. E., Martins, Z., Mimoun, D., Nenon, Q., Caro, G. M. Munõz, Rannou, P., Rauer, H., Schmitt-Kopplin, P., Schneeberger, A., Simons, M., Stephan, K., Van Hoolst, T., Vaverka, J., Wieser, M., Wörner, L.
Enceladus, an icy moon of Saturn, possesses an internal water ocean and jets expelling ocean material into space. Cassini investigations indicated that the subsurface ocean could be a habitable environment having a complex interaction with the rocky
Externí odkaz:
http://arxiv.org/abs/2211.00721
Publikováno v:
A&A 661, A116 (2022)
Context. The presence of a magnetic guide field induces several types of anisotropy in solar wind turbulence. The energy cascade rate between scales in the inertial range depends strongly on the direction of this magnetic guide field, splitting the e
Externí odkaz:
http://arxiv.org/abs/2112.13748
Autor:
Chatain, A., Wahlund, J. -E., Shebanits, O., Hadid, L. Z., Morooka, M., Edberg, N. J. T., Guaitella, O., Carrasco, N.
Publikováno v:
Journal of Geophysical Research: Space Physics, 126, e2020JA028413 (2021)
The ionosphere of Titan hosts a complex ion chemistry leading to the formation of organic dust below 1200 km. Current models cannot fully explain the observed electron temperature in this dusty environment. To achieve new insight, we have re-analyzed
Externí odkaz:
http://arxiv.org/abs/2108.12908
Autor:
Chatain, A., Wahlund, J. -E., Shebanits, O., Hadid, L. Z., Morooka, M., Edberg, N. J. T., Guaitella, O., Carrasco, N.
Publikováno v:
Journal of Geophysical Research: Space Physics, 126, e2020JA028412 (2021)
Current models of Titan ionosphere have difficulties in explaining the observed electron density and/or temperature. In order to get new insights, we re-analyzed the data taken in the ionosphere of Titan by the Cassini Langmuir probe (LP), part of th
Externí odkaz:
http://arxiv.org/abs/2108.12907
Autor:
Huybrighs, H. L. F., Roussos, E., Blöcker, A., Krupp, N., Futaana, Y., Barabash, S., Hadid, L. Z., Holmberg, M. K. G., Witasse, O.
In Huybrighs et al., 2020 we investigated energetic proton depletions along Galileo's Europa flyby E26. Based on a particle tracing analysis we proposed that depletions are caused by perturbed electrogmagnetic fields combined with atmospheric charge
Externí odkaz:
http://arxiv.org/abs/2108.10255
Autor:
Andrés, N., Sahraoui, F., Hadid, L. Z., Huang, S. Y., Romanelli, N., Galtier, S., DiBraccio, G., Halekas, J.
The first computation of the compressible energy transfer rate from $\sim$ 0.2 AU up to $\sim$ 1.7 AU is obtained using PSP, THEMIS and MAVEN observations. The compressible energy cascade rate $\varepsilon_C$ is computed for hundred of events at diff
Externí odkaz:
http://arxiv.org/abs/2102.11781
Autor:
Huang, S. Y., Sahraoui, F., Andrés, N., Hadid, L. Z., Yuan, Z. G., He, J. S., Zhao, J. S., Galtier, S., Zhang, J., Deng, X. H., Jiang, K., Yu, L., Xu, S. B., Xiong, Q. Y., Wei, Y. Y., de Wit, T. Dudok, Bale, S. D., Kasper, J. C.
The scaling of the turbulent spectra provides a key measurement that allows to discriminate between different theoretical predictions of turbulence. In the solar wind, this has driven a large number of studies dedicated to this issue using in-situ da
Externí odkaz:
http://arxiv.org/abs/2101.09851
Autor:
Huang, S. Y., Zhang, J., Sahraoui, F., He, J. S., Yuan, Z. G., Andrés, N., Hadid, L. Z., Deng, X. H., Jiang, K., Yu, L., Xiong, Q. Y., Wei, Y. Y., Xu, S. B., Bale, S. D., Kasper, J. C.
The nature of the plasma wave modes around the ion kinetic scales in highly Alfv\'enic slow solar wind turbulence is investigated using data from the NASA's Parker Solar Probe taken in the inner heliosphere, at 0.18 Astronomical Unit (AU) from the su
Externí odkaz:
http://arxiv.org/abs/2006.04665
Autor:
Andrews, D. J., Cowley, S. W. H., Provan, G., Hunt, G. J., Hadid, L. Z., Morooka, M. W., Wahlund, J. -E.
Saturn's magnetospheric magnetic field, planetary radio emissions, plasma populations and magnetospheric structure are all known to be modulated at periods close to the assumed rotation period of the planetary interior. These oscillations are readily
Externí odkaz:
http://arxiv.org/abs/1910.12540
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