Estudo teórico de moléculas diatômicas e triatômicas em manchas solares

Abstract

In this work we study the existence of diatomic and triatomic molecules in sunspots. From experimental data of the solar spectrum in the infrared (IR) region of 473 cm-1 - 925cm-1, it was possible to identify lines due to rotovibrational transitions of the molecules: BH, CH, HF, C2, CN, MgH, CO, AlH, NO, SiH, HCl, NP, TiO, CO2, HCN, NO2, BeCl2, OCS, NNO. The purpose of this description is to identify the presence of these molecules in sunspots, based on the amount of bands calculated for each case, including the NP molecule that has not yet been reported in the literature. Study the magnetism of these molecules and thus being able to predict which molecules may be influencing the magnetic field of sunspots and the consequences of this.