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Numerical modelling of the temporally variable lunar surficial H and OH number densityтезисы доклада
- Авторы: Wöhler C., Berezhnoy A.A., Grumpe A., Shevchenko V.V.
- Сборник: European Lunar Symposium
- Тезисы
- Год издания: 2017
- Место издания: Muenster, Germany
- Первая страница: 233
- Последняя страница: 234
- Аннотация: We have presented results of numerical modelling of the density of lunar surficial H and OH, which are qualitatively consistent with M³-based observations at low and high southern latitudes. Future work will involve the addition of H2O to the model. Further tests of the model will require observations of specific regions at many different daytimes, which are hardly available in the M³ data set. Ground-based near-infrared spectrometers such as the LIS instrument to be deployed on the upcoming Russian lunar landers will allow for a more refined comparison between observations and modelling results of daytime-dependent variations of the surficial OH abundance.
- Добавил в систему: Бережной Алексей Андреевич