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Influence of the Aerosol-Size Spread on Dissipative Instability of Aerosol Flows in the Planetary Atmospheres. II. Atmospheres of Mars and Titan

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Radiophysics and Quantum Electronics Aims and scope

The results on the aerosol-size spread influence on dissipative instability of aerosol flow in a cold weakly ionized collisional plasma, which were obtained in the first part of this paper [1], are used for the Mars (altitudes 70–100 km) and Titan (altitudes 900–1200 km) atmospheric conditions. The threshold charges and characteristic space–time instability scales are quantitatively estimated.

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Authors and Affiliations

  1. Institute of Applied Physics of the Russian Academy of Sciences, Nizhny Novgorod, Russia

    V. S. Grach

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  1. V. S. Grach
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Correspondence to V. S. Grach.

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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 56, No. 7, pp. 468–479, July 2013.

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Grach, V.S. Influence of the Aerosol-Size Spread on Dissipative Instability of Aerosol Flows in the Planetary Atmospheres. II. Atmospheres of Mars and Titan. Radiophys Quantum El 56, 422–432 (2013). https://doi.org/10.1007/s11141-013-9445-x

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  • DOI: https://doi.org/10.1007/s11141-013-9445-x

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