Аналитические приближения характеристик ночного гидроксила на Марсе и внутригодовые вариации
- Авторы: Шапошников Д.С.1, Григалашвили М.2, Медведев А.С.2, Зоннеманн Г.Р.2, Хартог П.2
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Учреждения:
- Московский физико-технический институт (НИУ)
- Институт исследований Солнечной системы им. Макса Планка
- Выпуск: Том 57, № 1 (2023)
- Страницы: 3-16
- Раздел: Статьи
- URL: https://journals.rcsi.science/0320-930X/article/view/134962
- DOI: https://doi.org/10.31857/S0320930X23010061
- EDN: https://elibrary.ru/HEHQZV
- ID: 134962
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Аннотация
Наблюдения за эмиссиями колебательно-возбужденного гидроксила (ОН*) широко используются для получения информации о динамике и составе атмосферы. Мы представляем несколько аналитических приближений для характеристик гидроксильного слоя в марсианской атмосфере, таких как концентрация ОН* у максимума и высота максимума, а также соотношения для оценки влияния различных факторов на слой ОН* в ночных условиях. Эти характеристики определяются температурой окружающей среды, концентрацией атомарного кислорода и их вертикальными градиентами. Полученные соотношения применены к результатам численного моделирования с помощью модели глобальной циркуляции атмосферы для предсказания сезонного поведения гидроксильного слоя на Марсе. Годовые и внутригодовые вариации концентрации возбужденного гидроксила и высоты слоя по данным моделирования имеют как некоторые сходства с земными, так и существенные различия. Концентрация и высота максимума в экваториальных, северных и южных средних широтах меняются в зависимости от сезона, при этом максимальные концентрации и наименьшая высота приходятся на первую половину года. Модельные расчеты подтвердили наличие пика концентрации ОН* в полярных широтах зимой на высоте примерно 50 км со значениями объемных плотностей эмиссии 2.1, 1.4 и 0.6 × 104 фотонов см–3 с–1 для переходов колебательных уровней 1–0, 2–1, 2–0, соответственно. Полученные соотношения могут быть использованы для анализа измерений и интерпретации их вариаций.
Ключевые слова
Об авторах
Д. С. Шапошников
Московский физико-технический институт (НИУ)
Email: shaposhnikov@phystech.edu
Россия, Москва
М. Григалашвили
Институт исследований Солнечной системы им. Макса Планка
Email: shaposhnikov@phystech.edu
Германия, Гёттинген
А. С. Медведев
Институт исследований Солнечной системы им. Макса Планка
Email: shaposhnikov@phystech.edu
Германия, Гёттинген
Г. Р. Зоннеманн
Институт исследований Солнечной системы им. Макса Планка
Email: shaposhnikov@phystech.edu
Германия, Гёттинген
П. Хартог
Институт исследований Солнечной системы им. Макса Планка
Автор, ответственный за переписку.
Email: shaposhnikov@phystech.edu
Германия, Гёттинген
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