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Study of high energy cosmic rays by different components of back scattered radiation generated in the lunar regolithдоклад на конференции
- Авторы: Калмыков Н.Н., Константинов А.А., Mukhamedshin R.A., Chubenko A.P., Свешникова Л.Г., Турундаевский А.Н., Tkatchev L., Подорожный Д.М.
- Международная Конференция : 32nd International Cosmic Ray Conference
- Даты проведения конференции: 2011
- Тип доклада: не указан
- Докладчик: не указан
- Место проведения: Beijing, China, China
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Аннотация доклада:
Possible experiments aimed at studying the primary cosmic rays on the Moon’s surface are considered. Monte-Carlo simulation was used. Three components (secondary neutrons, gamma rays, and radio waves) of back scattered radiation can be simultaneously registered. These components of radiation are generated by showers developing in the lunar regolith. Primary particle parameters can be reconstructed.
- Добавил в систему: Турундаевский Андрей Николаевич