Astrophysik V: Verschiedenes / Astrophysics V: Miscellaneous by R. R. Mcmath, O. C. Mohler (auth.), S. Flügge (eds.)

By R. R. Mcmath, O. C. Mohler (auth.), S. Flügge (eds.)

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T. ·EVANS: Unpublished, Sacramento Peak Observatory. 4 A. E. WHITFORD and G. E. KRON: Rev. Sci. lnstrum. 8, 78 (1937). - H. W. BABCOCK: Astrophys. Journ. 107, 73 (1948). s W. O. ROBERTS: Electronics 19,100 (1946). - E. FOWLER and S. JOHNSON: Electronics 24,118 (1948). 6 R. R. McMATH: Pub!. Obs. Univ. Michigan 7, 42 (1937). L. P. TABOR: Pub!. Cook Obs. Univ. Pennsylvania 4, 3 (1939). Sect. 16. Auxiliary instruments: Methods of recording. 29 In some problems it is desirable to drive the solar image at a preselected rate along a line at a given position angle.

82, 26 (1935). \. DOLLFUS: L'Astronomie 73,345 (1')5')). 4 ::VI. \strophys. Joum. 130, 245 (1959). \. ABOUD, W. E. G and W. A. RENsE: Astrophys. J oum. 130, 381 (1959). 6 R. \. NIDEY and D. S. SL\CEY: Rev. Sci. lnstrum. 27, 216 (1956). - H. D. \. , ::VI. JUZA, T. ::VIAHER and F. SPECK: Rev. Sci. lnstrum. 27, 381 (1956). 1 2 38 R. R. McMATH and O. C. MOHLER: Solar Instruments. Sect. 18. Table. Solar tower teleBlank spaces in the table remain where information to fill them could not be obtained. - Only solar tower telescopes are listed.

3* 36 R. R. McMATH and O. C. MOHLER: Solar Instruments. Sect. 18. predicted, nearly ideal conditions should occur on an isolated, high mountain peak rising from an ocean, far from land, within the latitude zone ±35°. The mountain should be high enough to rise above ordinary formations of cumulus clouds. The nearest approaches to such sites are the island of Tenerife 1 and the island of Hawaii 2, but little is known of the solar observing conditions at these sites. Even if a perfect site could be found, all solar instruments so far constructed would continue to be handicapped seriously by air currents established in the neighborhood of the telescope, and even within the telescope, by the heat of the Sun.

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