@Article{HaiderThBaAbSoGo:2022:SeTeVa,
               author = "Haider, S. A. and Thirupathaiah, P. and Batista, Inez Staciarini 
                         and Abdu, Mangalathayil Ali and Sobral, Jos{\'e} Humberto Andrade 
                         and Gobbi, Delano",
          affiliation = "{Physical Research Laboratory} and {St. John’s College} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)}",
                title = "Modeling and causative mechanism of OI 630.0 nm nightglow emission 
                         over Cachoeira Paulista (22.7oS, 45oW) – Brazil: Seasonal and 
                         temporal variability",
              journal = "Advances in Space Research",
                 year = "2022",
               volume = "69",
               number = "2",
                pages = "889--904",
                month = "Jan.",
             abstract = "The seasonal and temporal variability of the OI 630.0 nm nightglow 
                         emissions were observed over Cachoeira Paulista (22.7oS, 45oW; dip 
                         latitude \−35°) in Brazil by multichannel photometer during 
                         2014 and 2015. The temporal variation of the OI 630.0 nm nightglow 
                         intensity shows a peak during post-midnight hours (\∼25 h00 
                         LT) during the summer. During autumn, this peak is shifted towards 
                         pre-midnight at \∼ 22 h00 LT. It is noticed that this peak 
                         again shifted towards post-midnight at 26 h30 LT and 25 h30 LT 
                         during winter and spring, respectively. The intensity increases by 
                         a factor of 24 in the summer than that observed in other three 
                         seasons. The modelling of the nightglow measurements in 2015 is 
                         carried out by calculating the excitation rate, emission rate and 
                         intensity of OI 630.0 nm nightglow emission in the upper 
                         atmosphere at low latitudes. Our calculation suggests that the 
                         dissociative recombination of O2+ with electrons is the main 
                         source for the OI 630.0 nm nightglow emission. We report that the 
                         model intensities are in good agreement with the measurements at 
                         Cachoeira Paulista for all four seasons and the model reproduces 
                         all features of peak intensities very well.",
                  doi = "10.1016/j.asr.2021.10.018",
                  url = "http://dx.doi.org/10.1016/j.asr.2021.10.018",
                 issn = "0273-1177 and 1879-1948",
             language = "en",
           targetfile = "haider_2022_modeling.pdf",
        urlaccessdate = "01 maio 2024"
}