Performance of new infrared beamline U12IR at the National Synchrotron Light Source
1.G. P. Williams, Surf. Sci. 368, 1 (1996).
2.J. Yarwood, T. Shuttleworth, J. B. Hasted, and T. Nanba, Nature (London) 312, 742 (1984).
3.G. P. Williams, Nucl. Instrum. Methods Phys. Res. A 291, 8 (1990).
4.P. Roy, Y. L. Mathis, A. Gerschel, J. P. Marx, J. Michaut, B. Lagarde, and P. Calvani, Nucl. Instrum. Methods Phys. Res. A 325, 568 (1993).
5.A. Marcelli, E. Burattini, C. Mencuccini, A. Nucara, P. Calvani, S. Lupi, and M. Sanchez del Rio, Proc. SPIE 3153, 21 (1997).
6.C. J. Hirshmugl, G. P. Williams, F. M. Hoffmann, and Y. J. Chabal, Phys. Rev. Lett. 65, 480 (1990).
7.G. L. Carr, J. A. Reffner, and G. P. Williams, Rev. Sci. Instrum. 66, 1490 (1995).
8.A. F. Goncharov, V. V. Struzhkin, M. S. Somayazulu, R. J. Hemley, and H. K. Mao, Science 273, 218 (1996).
9.J. Kircher, R. Henn, M. Cardona, P. L. Richards, and G. P. Williams, J. Opt. Soc. Am. B 14, 705 (1997).
10.R. W. Whatmore, P. A. Goddard, B. K. Tanner, and G. F. Clarke, Nature (London) 299, 44 (1982).
11.G. P. Williams, P. Z. Takacs, R. W. Klaffky, and M. Shleifer, Nucl. Instrum. Methods Phys. Res. A 246, 165 (1986).
12.D. L. Ederer et al., Nucl. Instrum. Methods Phys. Res. A 319, 250 (1992).
13.G. L. Carr, R. P. S. M. Lobo, C. J. Hirschmugl, J. LaVeigne, D. H. Reitze, and D. B. Tanner, Proc. SPIE 3153, 80 (1997).
14.R. P. S. M. Lobo, G. L. Carr, J. LaVeigne, D. H. Reitze, and D. B. Tanner (unpublished).
15.J. Schwinger, Phys. Rev. 75, 1912 (1949).
16.J. D. Jackson, Classical Electrodynamics, 2nd ed. (Wiley, New York, 1975), p. 676.
17.G. L. Carr, D. Lynch, S. Pjerov, and G. P. Williams, J. Synchrotron Radiat. (submitted).
18.As the electrons travel in a horizontal orbit the natural emission angle is important only in the vertical direction. Along the orbit plane, light emitted by electrons in their curved trajectory fully spans the mirror for all wavelengths. The amount of light collected at long wavelengths is therefore proportional only to the ratio between the collection angle and the natural emission angle, not its square.
19.R. L. Henry and D. B. Tanner, Infrared Phys. 19, 163 (1979).
20.As each electron in the bunches is independent, in most cases the emitted power depends linearly on the ring current. Few exceptions happen when the electron density in bunches is very high (very high current per bunch or very short bunch). In this case interactions between the electrons cause them to emit coherently. For most of our applications coherent emission can be neglected.
21.W. D. Duncan and G. P. Williams, Appl. Opt. 22, 2914 (1983).
22.G. P. Williams, C. J. Hirschmugl, E. M. Kneedler, P. Z. Takaca, M. Shleifer, Y. J. Chabal, and F. M. Hoffmann, Phys. Rev. Lett. 62, 261 (1989).
23.This is only true in the horizontal direction. In the vertical direction the parabolic mirror filling varies as a slow function of the wavelength. With our setup this mirror is fully filled along the vertical direction by light below 30 At 150 it is about 70% filled.
24.R. Biscardi, G. Ramirez, G. P. Williams, and C. Zimba, Rev. Sci. Instrum. 66, 1856 (1995).
No metrics data to plot.
The attempt to load metrics for this article has failed.
The attempt to plot a graph for these metrics has failed.
Article metrics loading...
Full text loading...
Most read this month
Most cited this month