| Автор | Rumsey, N.J. |
| Дата выпуска | 1961 |
| dc.description | A ‘sky lens’ images a strip of sky on the entrance slit of a spectrograph. Then the intensity distribution of each spectral emission from the strip of sky is mapped along the corresponding spectral line. In order to reduce light losses to a minimum a single lens component may be used for this purpose (in place of the usual two components), but one surface should be aspherized. If this surface is made an hyperboloid the lens performs very well over a 20° field. |
| Формат | application.pdf |
| Издатель | Taylor & Francis Group |
| Копирайт | Copyright Taylor and Francis Group, LLC |
| Название | A 'Sky Lens' for an Auroral Spectrograph |
| Тип | research-article |
| DOI | 10.1080/713826363 |
| Print ISSN | 0030-3909 |
| Журнал | Optica Acta: International Journal of Optics |
| Том | 8 |
| Первая страница | 17 |
| Последняя страница | 19 |
| Аффилиация | Rumsey, N.J.; Dominion Physical Laboratory, Lower Hutt, New Zealand |
| Выпуск | 1 |
| Библиографическая ссылка | BURCH, C. R. 1942. Mon. Not. R. astr. Soc., 102: 159 |
| Библиографическая ссылка | BORCH, C. R. 1956. Observatory, 76: 173 |
| Библиографическая ссылка | LINFOOT, E. H. 1955. Recent Advances in Optics, Oxford Clarendon Press. Ch. IV |
| Библиографическая ссылка | STEWARD, G. C. 1928. The Symmetrical Optical System, Cambridge: University Press. |
