Air-wedge shearing interferometer

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Figure 1. Beam path inside of air-wedge interferometer. Fig1 Air-Wedge beams.jpg
Figure 1. Beam path inside of air-wedge interferometer.

The air-wedge shearing interferometer is probably the simplest type of interferometer designed to visualize the disturbance of the wavefront after propagation through a test object. This interferometer is based on utilizing a thin wedged air-gap between two optical glass surfaces and can be used with virtually any light source even with non-coherent white light.

Contents

Setup

An air-wedge shearing interferometer is described in [1] and was employed in set of experiments described in. [2] [3] [4] [5] [6] [7] [8] This interferometer consists of two optical glass wedges (~2-5deg), pushed together and then slightly separated from one side to create a thin air-gap wedge. This air-gap wedge has a unique property: it is very thin (micrometer scale) and it has perfect flatness (~λ/10).

There are four nearly equal intensity Fresnel reflections (~4% for refraction coefficient 1.5) from the air-wedge interferometer (Fig.1):

  1. from the exterior surface of the first glass block
  2. from the interior surface of the first glass block
  3. from the interior surface of the second glass block
  4. from the exterior surface of the second glass block

The angle between beams 1-2 and 3-4 is non adjustable and depends only on the shape of the glass wedge. The angle between beams 2-3 is easily adjusted by varying the air-wedge angle. The distance between the air-wedge and an image plane should be long enough to spatially separate reflections 1 from 2 and 3 from 4.[ specify ] The overlap of beams 2 and 3 in the image plane creates an interferogram.

Alignment

To minimize image aberrations the angle plane of the glass wedges has to be placed orthogonal to the angle plane of the air-wedge. Because intensity of Fresnel reflections from a glass surface are polarization and angle dependent, it is necessary to keep the air-wedge plane nearly perpendicular to the incident beam (±5deg) to minimize instrumentally induced intensity variation. This is very important when coupling the air-wedge interferometer to imaging optics. The air-wedge interferometer has a very simple design and requiring only 2 standard BK7 glass wedges and 1 mirror holder (Fig.3).

Figure 3. Example of air-wedge interferometer. Fig2-air-wedge int.jpg
Figure 3. Example of air-wedge interferometer.

Applications

Because of its extremely thin air-gap, the air-wedge interferometer was successfully applied in experiments with femto-second high-power lasers. Figure 4 shows an interferogram of laser interactions with a He jet in a vacuum chamber. [2] The probing beam has ~500-fs duration, and ~1-μm wavelength. The air-wedge interferogram from even this very short coherence length laser beam exhibits clear, high-contrast interference lines.

Figure 4. Interferogram of laser-He jet interaction at +15ps. Fig3-HeJet Inter 0517i33 +15ps.jpg
Figure 4. Interferogram of laser-He jet interaction at +15ps.

Advantages

The air-wedge shearing interferometer is similar to the classical shearing interferometer but is micrometres thick, can operate with virtually any light source even with non-coherent white light, has an adjustable angular beam split, and uses standard inexpensive optical elements. Replacement of the second glass wedge by a plane-concave lens, will turn the lateral-shearing air-wedge interferometer to a radial-shearing interferometer, which is important for some specific applications.

The principle of interference from the air-wedge between two plane-parallel glass plates is described in a number of elementary optics textbooks. [9] But this "classical" air-wedge arrangement has never been used for interferometry with field visualization owing to the overlap of all four reflected beams in the image plane. Design described in this article eliminates this obstruction and makes the air-wedge interferometer effective for practical applications with a visualization field interferometry.

See also

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References

  1. G.S. Sarkisov, Shearing interferometer with an air wedge for electron density diagnostics in a dense plasma, Instruments and Experimental Techniques, vol.39, No.5, pp.727-731 (1996).
  2. 1 2 Sarkisov, G. S.; Bychenkov, V. Yu.; Novikov, V. N.; Tikhonchuk, V. T.; Maksimchuk, A.; et al. (1999-06-01). "Self-focusing, channel formation, and high-energy ion generation in interaction of an intense short laser pulse with a He jet". Physical Review E. American Physical Society (APS). 59 (6): 7042–7054. Bibcode:1999PhRvE..59.7042S. doi:10.1103/physreve.59.7042. ISSN   1063-651X. PMID   11969693. S2CID   13029022.
  3. Iglesias, E.J.; Elton, R.C.; Griem, H.R.; Scott, H.A. (2003). "Time resolved air-wedge shearing interferometry and spectroscopy on a picoseconds plasma" (PDF). Revista Mexicana de Fisica. 49 (S3): 126-129. Bibcode:2003RMxFS..49b.128I.
  4. S.V. Granov, V.I. Konov, A.A. Malyutin, O.G. Tsarkova, I.S. Yatskovsky, F. Dausinger, High resolution interferometric diagnostics of plasmas produced by ultrashot laser pulses, Laser Physics, 13, 3, pp.386-396 (2003).
  5. Hii, King Ung; Kwek, Kuan Hiang (2009-01-08). "Dual-prism interferometer for collimation testing". Applied Optics. The Optical Society. 48 (2): 397–400. Bibcode:2009ApOpt..48..397H. doi:10.1364/ao.48.000397. ISSN   0003-6935. PMID   19137053.
  6. Hu, Min; Kusse, Bruce R. (2004). "Optical observations of plasma formation and wire core expansion of Au, Ag, and Cu wires with 0–1 kA per wire". Physics of Plasmas. AIP Publishing. 11 (3): 1145–1150. Bibcode:2004PhPl...11.1145H. doi:10.1063/1.1644582. ISSN   1070-664X.
  7. Ivanov, V. V.; Sotnikov, V. I.; Sarkisov, G. S.; Cowan, T. E.; Bland, S. N.; et al. (2006-09-18). "Dynamics of Mass Transport and Magnetic Fields in Low-Wire-Number-ArrayZPinches". Physical Review Letters. American Physical Society (APS). 97 (12): 125001. Bibcode:2006PhRvL..97l5001I. doi:10.1103/physrevlett.97.125001. ISSN   0031-9007. PMID   17025975.
  8. Ivanov, Vladimir V; Altemara, Sara D; Astanovitskiy, Alexey A; Sarkisov, Gennady S; Haboub, Abdelmoula; Papp, Daniel; Kindel, Joseph M (2010). "Development of UV Laser Probing Diagnostics for 1-MA Z-Pinches". IEEE Transactions on Plasma Science. Institute of Electrical and Electronics Engineers (IEEE). 38 (4): 574–580. Bibcode:2010ITPS...38..574I. doi:10.1109/tps.2010.2041215. ISSN   0093-3813. S2CID   9937375.
  9. M. Born and E. Wolf, Principles of Optics (Cambridge University Press; 6 edition, 1997).