Abstract

No abstract available.

Full Article  |  PDF Article

References

  • View by:
  • |
  • |
  • |

  1. H. D. Babcock and H. W. Babcock, J. Opt. Soc. Am. 41, 776 (1951).
    [CrossRef]
  2. R. W. Wood, Physical Optics (Macmillan Company, New York, 1934), pp. 262, 626.
  3. Arthur Shuster, Astrophys. J. 21, 197 (1905).
    [CrossRef]

1951 (1)

1905 (1)

Arthur Shuster, Astrophys. J. 21, 197 (1905).
[CrossRef]

Babcock, H. D.

Babcock, H. W.

Shuster, Arthur

Arthur Shuster, Astrophys. J. 21, 197 (1905).
[CrossRef]

Wood, R. W.

R. W. Wood, Physical Optics (Macmillan Company, New York, 1934), pp. 262, 626.

Astrophys. J. (1)

Arthur Shuster, Astrophys. J. 21, 197 (1905).
[CrossRef]

J. Opt. Soc. Am. (1)

Other (1)

R. W. Wood, Physical Optics (Macmillan Company, New York, 1934), pp. 262, 626.

Cited By

OSA participates in CrossRef's Cited-By Linking service. Citing articles from OSA journals and other participating publishers are listed here.

Alert me when this article is cited.


Figures (1)

Fig. 1
Fig. 1

Departure of focus of grating due to error of run. Curve A calculated from Eq. (1). Curve B calculated from Eq. (3). The constants used were α′=3.83 × 10−10, F=975 cm, R=975 cm. dF is expressed in mm. The triangles represent experimentally determined points for the plane grating.

Equations (5)

Equations on this page are rendered with MathJax. Learn more.

N λ = a ( sin i ± sin θ ) ,
d F = ( 2 F 2 α ) / a · sin i / cos 2 i .
r = a / α · ( cos 2 θ ) / ( sin i ± sin θ ) .
d F = [ ( R 2 α ) / a ] ( sin i ± sin θ ) .
d F = ( F 2 α ) / a · ( sin i ± sin θ ) / ( cos 2 θ ) .