. "\u0421\u043F\u0435\u043A\u0442\u0440\u043E\u0441\u043A\u043E\u043F\u0438\u044F \u0441 \u0434\u043B\u0438\u043D\u043D\u043E\u0439 \u0449\u0435\u043B\u044C\u044E"@ru . . . . "\u0421\u043F\u0435\u043A\u0442\u0440\u043E\u0441\u043A\u043E\u043F\u0438\u044F \u0441 \u0434\u043B\u0438\u043D\u043D\u043E\u0439 \u0449\u0435\u043B\u044C\u044E (\u0430\u043D\u0433\u043B. Long-slit spectroscopy) \u2014 \u043C\u0435\u0442\u043E\u0434 \u0441\u043F\u0435\u043A\u0442\u0440\u043E\u0441\u043A\u043E\u043F\u0438\u0438, \u043F\u043E\u0437\u0432\u043E\u043B\u044F\u044E\u0449\u0438\u0439 \u043F\u043E\u043B\u0443\u0447\u0430\u0442\u044C \u043E\u0434\u043D\u043E\u0432\u0440\u0435\u043C\u0435\u043D\u043D\u043E \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u0443\u044E \u0438 \u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0441\u0442\u0432\u0435\u043D\u043D\u0443\u044E \u0438\u043D\u0444\u043E\u0440\u043C\u0430\u0446\u0438\u044E \u043E\u0431 \u043E\u0431\u044A\u0435\u043A\u0442\u0435. \u041C\u0435\u0442\u043E\u0434 \u0440\u0430\u0441\u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0451\u043D \u0432 \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0438\u0438."@ru . . . . . . . . . . "4794"^^ . . . . . . . . . "In astronomy, long-slit spectroscopy involves observing a celestial object using a spectrograph in which the entrance aperture is an elongated, narrow slit. Light entering the slit is then refracted using a prism, diffraction grating, or grism. The dispersed light is typically recorded on a charge-coupled device detector."@en . . . . . "1099185263"^^ . . . . . "Long-slit spectroscopy"@en . . "\u0421\u043F\u0435\u043A\u0442\u0440\u043E\u0441\u043A\u043E\u043F\u0438\u044F \u0441 \u0434\u043B\u0438\u043D\u043D\u043E\u0439 \u0449\u0435\u043B\u044C\u044E (\u0430\u043D\u0433\u043B. Long-slit spectroscopy) \u2014 \u043C\u0435\u0442\u043E\u0434 \u0441\u043F\u0435\u043A\u0442\u0440\u043E\u0441\u043A\u043E\u043F\u0438\u0438, \u043F\u043E\u0437\u0432\u043E\u043B\u044F\u044E\u0449\u0438\u0439 \u043F\u043E\u043B\u0443\u0447\u0430\u0442\u044C \u043E\u0434\u043D\u043E\u0432\u0440\u0435\u043C\u0435\u043D\u043D\u043E \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u0443\u044E \u0438 \u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0441\u0442\u0432\u0435\u043D\u043D\u0443\u044E \u0438\u043D\u0444\u043E\u0440\u043C\u0430\u0446\u0438\u044E \u043E\u0431 \u043E\u0431\u044A\u0435\u043A\u0442\u0435. \u041C\u0435\u0442\u043E\u0434 \u0440\u0430\u0441\u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0451\u043D \u0432 \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0438\u0438."@ru . . . . . . . . . . . "32668725"^^ . . . . . . . . . . "In astronomy, long-slit spectroscopy involves observing a celestial object using a spectrograph in which the entrance aperture is an elongated, narrow slit. Light entering the slit is then refracted using a prism, diffraction grating, or grism. The dispersed light is typically recorded on a charge-coupled device detector."@en . . . . . . . . . .