Abstract

We demonstrate the ability to generate ultrahigh frequency burst sequences of deep UV at 226nm by mixing the optical parametric oscillator signal output at 622nm with third harmonic at 355nm from a pulse burst laser system. We obtained 226nm burst sequences with uniform burst envelopes, and the average pulse energy is 0.5mJ. Nitric oxide planar laser-induced fluorescence image sequences at ultrahigh (100kHz) frame rates have been obtained.

© 2008 Optical Society of America

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2008 (1)

2007 (2)

C. Kittler and A. Dreizler, Appl. Phys. B 89, 163 (2007).
[CrossRef]

J. D. Smith and V. Sick, Proc. Combust. Inst. 31, 747 (2007).
[CrossRef]

2004 (1)

2003 (1)

W. Lempert, M. Boehm, N. Jiang, S. Gimelshein, and D. Levin, Exp. Fluids 34, 403 (2003).

2001 (1)

J. S. Fox, A. F. P. Houwing, P. M. Danehy, M. J. Gaston, N. R. Muidford, and S. L. Gai, J. Propul. Power 17, 284 (2001).
[CrossRef]

2000 (1)

P. Wu, W. R. Lempert, and R. B. Miles, AIAA J. 38, 672 (2000).
[CrossRef]

1999 (1)

C. F. Kaminski, J. Hult, and M. Alden, Appl. Phys. B 68, 757 (1999).
[CrossRef]

1993 (1)

1989 (1)

1985 (1)

1984 (1)

G. Kychakoff, K. Knapp, R. D. Howe, and R. K. Hanson, AIAA J. 22, 153 (1984).
[CrossRef]

1982 (2)

Alden, M.

C. F. Kaminski, J. Hult, and M. Alden, Appl. Phys. B 68, 757 (1999).
[CrossRef]

Boehm, M.

W. Lempert, M. Boehm, N. Jiang, S. Gimelshein, and D. Levin, Exp. Fluids 34, 403 (2003).

Crosley, D. R.

Danehy, P. M.

J. S. Fox, A. F. P. Houwing, P. M. Danehy, M. J. Gaston, N. R. Muidford, and S. L. Gai, J. Propul. Power 17, 284 (2001).
[CrossRef]

Dreizler, A.

C. Kittler and A. Dreizler, Appl. Phys. B 89, 163 (2007).
[CrossRef]

Dyer, M. J.

Fox, J. S.

J. S. Fox, A. F. P. Houwing, P. M. Danehy, M. J. Gaston, N. R. Muidford, and S. L. Gai, J. Propul. Power 17, 284 (2001).
[CrossRef]

Gai, S. L.

J. S. Fox, A. F. P. Houwing, P. M. Danehy, M. J. Gaston, N. R. Muidford, and S. L. Gai, J. Propul. Power 17, 284 (2001).
[CrossRef]

Gaston, M. J.

J. S. Fox, A. F. P. Houwing, P. M. Danehy, M. J. Gaston, N. R. Muidford, and S. L. Gai, J. Propul. Power 17, 284 (2001).
[CrossRef]

Gimelshein, S.

W. Lempert, M. Boehm, N. Jiang, S. Gimelshein, and D. Levin, Exp. Fluids 34, 403 (2003).

Gord, J.

Hanson, R. K.

Houwing, A. F. P.

J. S. Fox, A. F. P. Houwing, P. M. Danehy, M. J. Gaston, N. R. Muidford, and S. L. Gai, J. Propul. Power 17, 284 (2001).
[CrossRef]

Howe, R. D.

Hult, J.

C. F. Kaminski, J. Hult, and M. Alden, Appl. Phys. B 68, 757 (1999).
[CrossRef]

Jiang, N.

Kaminski, C. F.

C. F. Kaminski, J. Hult, and M. Alden, Appl. Phys. B 68, 757 (1999).
[CrossRef]

Kittler, C.

C. Kittler and A. Dreizler, Appl. Phys. B 89, 163 (2007).
[CrossRef]

Knapp, K.

G. Kychakoff, K. Knapp, R. D. Howe, and R. K. Hanson, AIAA J. 22, 153 (1984).
[CrossRef]

Kychakoff, G.

Lee, M. P.

Lempert, W.

Lempert, W. R.

P. Wu, W. R. Lempert, and R. B. Miles, AIAA J. 38, 672 (2000).
[CrossRef]

Levin, D.

W. Lempert, M. Boehm, N. Jiang, S. Gimelshein, and D. Levin, Exp. Fluids 34, 403 (2003).

McDaniel, J. C.

McMillin, B. K.

Meyer, T.

Miles, R. B.

P. Wu, W. R. Lempert, and R. B. Miles, AIAA J. 38, 672 (2000).
[CrossRef]

Muidford, N. R.

J. S. Fox, A. F. P. Houwing, P. M. Danehy, M. J. Gaston, N. R. Muidford, and S. L. Gai, J. Propul. Power 17, 284 (2001).
[CrossRef]

Opalski, A. B.

M. Wernet and A. B. Opalski, presented at the 24th American Institute of Aeronautics and Astronautics Aerodynamic Measurement Technology and Ground Testing Conference, Portland, Ore., June 28-July 1, 2004, paper 2004-2184.

Palmer, J. L.

Paul, P. H.

Samimy, M.

Seitzman, J. M.

Sick, V.

J. D. Smith and V. Sick, Proc. Combust. Inst. 31, 747 (2007).
[CrossRef]

Smith, J. D.

J. D. Smith and V. Sick, Proc. Combust. Inst. 31, 747 (2007).
[CrossRef]

Switzer, G.

Thurow, B.

Wernet, M.

M. Wernet and A. B. Opalski, presented at the 24th American Institute of Aeronautics and Astronautics Aerodynamic Measurement Technology and Ground Testing Conference, Portland, Ore., June 28-July 1, 2004, paper 2004-2184.

Wu, P.

P. Wu, W. R. Lempert, and R. B. Miles, AIAA J. 38, 672 (2000).
[CrossRef]

AIAA J. (2)

G. Kychakoff, K. Knapp, R. D. Howe, and R. K. Hanson, AIAA J. 22, 153 (1984).
[CrossRef]

P. Wu, W. R. Lempert, and R. B. Miles, AIAA J. 38, 672 (2000).
[CrossRef]

Appl. Opt. (4)

Appl. Phys. B (2)

C. F. Kaminski, J. Hult, and M. Alden, Appl. Phys. B 68, 757 (1999).
[CrossRef]

C. Kittler and A. Dreizler, Appl. Phys. B 89, 163 (2007).
[CrossRef]

Exp. Fluids (1)

W. Lempert, M. Boehm, N. Jiang, S. Gimelshein, and D. Levin, Exp. Fluids 34, 403 (2003).

J. Propul. Power (1)

J. S. Fox, A. F. P. Houwing, P. M. Danehy, M. J. Gaston, N. R. Muidford, and S. L. Gai, J. Propul. Power 17, 284 (2001).
[CrossRef]

Opt. Lett. (3)

Proc. Combust. Inst. (1)

J. D. Smith and V. Sick, Proc. Combust. Inst. 31, 747 (2007).
[CrossRef]

Other (1)

M. Wernet and A. B. Opalski, presented at the 24th American Institute of Aeronautics and Astronautics Aerodynamic Measurement Technology and Ground Testing Conference, Portland, Ore., June 28-July 1, 2004, paper 2004-2184.

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Figures (3)

Fig. 1
Fig. 1

Typical 1064 nm burst trains with interpulse separations of 10, 20, and 50 μ s .

Fig. 2
Fig. 2

Typical 20-pulse 10 μ s spacing burst sequence of 226 nm .

Fig. 3
Fig. 3

NO PLIF image sequence obtained from a 226 nm burst sequence similar to that shown in Fig. 2. Flow is from left to right, Mach 2 micronozzle with 7 × 14 mm field-of-view.

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