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ANGEO | Articles | Volume 36, issue 6
Ann. Geophys., 36, 1537–1543, 2018
https://doi.org/10.5194/angeo-36-1537-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
Ann. Geophys., 36, 1537–1543, 2018
https://doi.org/10.5194/angeo-36-1537-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.

ANGEO Communicates 15 Nov 2018

ANGEO Communicates | 15 Nov 2018

Can an interplanetary magnetic field reach the surface of Venus?

Yasuhito Narita and Uwe Motschmann
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On the ion-inertial-range density-power spectra in solar wind turbulence
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Advanced calibration of magnetometers on spin-stabilized spacecraft based on parameter decoupling
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Subject: Terrestrial planets systems | Keywords: Magnetic field
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Cited articles  
Bagdonat, T. B.: Hybrid simulations of weak comets, PhD thesis, Tech. Univ. Braunschweig, Braunschweig, 2002. a, b
Benkhoff, J., van Casteren, J., Hayakawa, H., Fujimoto, M., Laakso, H., Novara, M., Ferri, P., Middleton, H. R., and Ziethe, R.: BepiColombo – Comprehensive exploration of Mercury: Mission overview and science goals, Planet. Space Sci., 58, 2–20, https://doi.org/10.1016/j.pss.2009.09.020, 2010. a
Bößwetter, A.: Wechselwirkung des Mars mit dem Sonnenwind: Hybrid-Simulationen mit besonderem Bezug zur Wasserbilanz, PhD thesis, Tech. Univ. Braunschweig, Braunschweig, Germany, https://publikationsserver.tu-braunschweig.de/receive/dbbs_mods_00028707 (last access: 15 November 2018), 2009. a
Bößwetter, A., Bagdonat, T., Motschmann, U., and Sauer, K.: Plasma boundaries at Mars: a 3-D simulation study, Ann. Geophys., 22, 4363–4379, https://doi.org/10.5194/angeo-22-4363-2004, 2004. a, b
Dimmock, A. P., Alho, M., Kalio, E., Pope, S. A., Zhang, T. L., Kilpua, E., Pulkkinen, T. I., Futaana, Y., and Coates, A. J.: The response of the Venusian plasma environment to the passage of an iCME: Hybrid simulation results and Venus Express observations, J. Geophys. Res.-Space, 123, 3580–3601, https://doi.org/10.1029/2017JA024852, 2018. a
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Venus has no intrinsic magnetic field. On the other hand, we discover that an interplanetary magnetic field may nevertheless penetrate the planetary ionosphere by the diffusion process and reach the planetary surface when the solar wind condition remains for a sufficiently long time, between 12 and 54 h, depending on the condition of ionosphere.
Venus has no intrinsic magnetic field. On the other hand, we discover that an interplanetary...
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