Abstract:The solar wind-comet interaction, one of the basic processes investigated in the cometary physics, may be judged by the ion's behavior. CO is one of the most abundant cometary atmosphere species. A synthetic spectrum of CO was created to analyze Halley's comet spectra. The values of some molecular constants were specified in order to improve the accuracy of the computations. It was established that the more appropriate value of the spin-rotational interaction parameter y for the B2 state is 0.0192. The use of … Show more
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