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Growth and Damping of Oxygen Ion Cyclotron Harmonics in the Plasma Regions of Venus

  • Authors: Amrutha, S. V. Singh, K. C. Barik, G. S. Lakhina

Amrutha et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 5.

Normalized growth rate of perpendicularly propagating O+ cyclotron harmonics plotted against normalized real frequency for varying ambient plasma parameters. Wave propagation angle: θ = 89﹩\mathop{.}\limits^{\unicode{x000b0}}﹩99. (a) Plasma density varied from 100 to 400 cm−3 for IMB parameters. (b) Ambient magnetic field strength varied from 50 to 20 nT for IMB parameters. (c) Plasma density varied from 1000 to 700 cm−3 for upper ionosphere parameters. Only the fifth harmonic (n = 5) is displayed. (d) Ambient magnetic field strength varied from 10 to 40 nT for upper ionosphere plasma parameters.

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