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Atomic Iron and Nickel in the Coma of C/1996 B2 (Hyakutake): Production Rates, Emission Mechanisms, and Possible Parents

  • Authors: S. J. Bromley, B. Neff, S. D. Loch, J. P. Marler, J. Országh, K. Venkataramani, D. Bodewits

S. J. Bromley et al 2021 The Planetary Science Journal 2 .

  • Provider: AAS Journals

Caption: Figure 2.

Ratio of line intensity standard deviation to line intensity (in percentage) for 213 Ni I lines spanning 300–500 nm as a function of iteration number (see text). Spectra were generated at the orbital conditions of the closest approach of C/1996 Hyakutake and are plotted at 10, 102, 103, 104, 105, and 106 iterations. Each colored line shows the convergence of an individual transition.

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