|
ИСТИНА |
Войти в систему Регистрация |
Интеллектуальная Система Тематического Исследования НАукометрических данных |
||
A new method for determining particle energy in the range 10(11)-10(15) eV and results from a beam test at 180 GeV/cстатья
Информация о цитировании статьи получена из
Web of Science,
Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 18 июля 2013 г.
- Авторы: Bashindzhagyan G.L., Voronin A.G., Golubkov S.A., Grebenyuk V.M., Egorov N.N., Kalinin A.M., Karmanov D.E., Kon'kov K.A., Korotkova N.A., Kozlov Y.F., Krumshtein Z.V., Merkin M.M., Panasyuk M.I., Pakhomov A.Y., Podorozhnyi D.M., Postnikov E.B., Roganova T.M., Sadovskii A.B., Sveshnikova L.G., Sidorov A.I., Tkachev L.G., Turundaevskii A.N.
- Журнал: Instruments and Experimental Techniques
- Том: 48
- Номер: 1
- Год издания: 2005
- Издательство: Pleiades Publishing, Ltd
- Местоположение издательства: Road Town, United Kingdom
- Первая страница: 32
- Последняя страница: 36
- DOI: 10.1007/s10786-005-0004-3
- Аннотация: A method for measuring the energy of the nuclear component of cosmic rays is described. The principle of the method consists in determining the energy of a primary nucleus from the space density of secondary particles produced in a thin target in the initial event of inelastic interaction. The results from testing the method on an ejected 180-GeV pion beam are presented. Analysis of the experimental data and simulation show that, using this method, it is possible to measure the particle energy with a relative error of similar to 67%. The method is being developed for the direct detection of cosmic rays over wide ranges of energy (10(11)-10(15) eV/particle) and charge (Z = 1-30) during a cosmic experiment in near-Earth space.
- Добавил в систему: Воронина Екатерина Николаевна