High spectral resolution line profiles and images of comet Halley
High-spectral-resolution line profiles and images of comet Halley were obtained in 1986 at the National Solar Observatory McMath telescope, using a dual-etalon Fabry-Perot spectrometer. The spectrometer was designed to obtain data in four distinct modes: (1) high-resolution (R = 200,000) scanning, (...
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| Veröffentlicht in: | Advances in space research 1985, Vol.5 (12), p.279-282 |
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| container_title | Advances in space research |
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| creator | Roesler, F.L. Scherb, F. Magee, K. Harlander, J. Reynolds, R.J. Yelle, R.V. Broadfoot, A.L. Oliversen, R.J. |
| description | High-spectral-resolution line profiles and images of comet Halley were obtained in 1986 at the National Solar Observatory McMath telescope, using a dual-etalon Fabry-Perot spectrometer. The spectrometer was designed to obtain data in four distinct modes: (1) high-resolution (R = 200,000) scanning, (2) high-resolution imaging, (3) moderate resolution (R = 30,000) scanning, and (4) moderate resolution imaging. This paper describes the instrument and some examples of data obtained in the high-resolution scanning mode. |
| doi_str_mv | 10.1016/0273-1177(85)90097-3 |
| format | Article |
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The spectrometer was designed to obtain data in four distinct modes: (1) high-resolution (R = 200,000) scanning, (2) high-resolution imaging, (3) moderate resolution (R = 30,000) scanning, and (4) moderate resolution imaging. 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| ispartof | Advances in space research, 1985, Vol.5 (12), p.279-282 |
| issn | 0273-1177 1879-1948 |
| language | eng |
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| source | Elsevier ScienceDirect Journals |
| title | High spectral resolution line profiles and images of comet Halley |
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