Time-resolved X-ray diffraction

Contemporary Physics Taylor & Francis 37:3 (1996) 205-218

Characteristics of rapidly recombining plasmas suitable for high-gain X-ray laser action

Laser and Particle Beams Cambridge University Press (CUP) 14:1 (1996) 71-79

Authors:

J Zhang, MH Key, PA Norreys, C Danson, D Neely, SJ Rose, F Walsh, GJ Tallents, L Dwivedi, M Holden, PB Holden, GJ Pert, SA Ramsden, CLS Lewis, AG Macphee, YL You

Development of XUV lasers at the RAL Central Laser Facility

Optical and Quantum Electronics Springer Nature 28:3 (1996) 201-208

Authors:

MH Key, WJ Blyth, AE Dangor, P Dhez, A Djoui, L Dwivedi, M Holden, PB Holden, P Jaegle, CLS Lewis, AG McPhee, A Modena, M Nakai, D Neely, PA Norreys, AA Offenberger, GJ Pert, JA Ploues, SG Preston, SA Ramsden, SJ Rose, B Russ, CG Smith, A Sureau, GJ Tallents, F Walsh, JS Wark, YL You, J Zhang

Efficient extreme UV harmonics generated from picosecond laser pulse interactions with solid targets.

Physical review letters 76:11 (1996) 1832-1835

Authors:

PA Norreys, M Zepf, S Moustaizis, AP Fews, J Zhang, P Lee, M Bakarezos, CN Danson, A Dyson, P Gibbon, P Loukakos, D Neely, FN Walsh, JS Wark, AE Dangor

Using low and high prepulses to enhance the J=0-1 transition at 19.6 nm in the Ne-like germanium XUV laser

Optics Communications 123:4-6 (1996) 777-789

Authors:

GF Cairns, CLS Lewis, MJ Lamb, AG MacPhee, D Neely, P Norreys, MH Key, SB Healy, PB Holden, GJ Pert, JA Plowes, GJ Tallents, A Demir

Abstract:

We report a study of the effect of prepulses on XUV lasing of Ne-like germanium for an irradiation geometry where ≈20 mm long germanium slab targets were irradiated at ≈1.6 × 1013 W cm-2 using ≈0.7 ns (1.06 μm) pulses from the VULCAN glass laser. Prepulses were generated at fractional power levels of ≈2 × 10-4 (low) and ≈2 × 10-2 (high) and arrived on target 5 and 3.2 ns respectively in advance of the main heating pulse. For both the low and high prepulses the output of the 3p-3s, J=0-1, line at 19.6 nm was enhanced such that the peak radiant density (J/st) for this line became greater than that for the normally stronger J=2-1 lines at 23.2 and 23.6 nm. The 7=0-1 line, whose FWHM duration was reduced from ≈450 ps to ≈100 ps, delivered ≈6X more power (W) than the average for the combined J=2-1 lines, whose FWHM duration was ≈500 ps for both levels of prepulse. The higher prepulse was more effective, yielding ≈2X more radiant density and ≈7X more power on both the J=0-1 and J=2-1 transitions compared to the low prepulse case. The most dramatic observation overall was the ≈40X increase of power in the J=0-1 line for the high prepulse (≈2%) case compared with the zero prepulse case. These observations, coupled with measurements of beam divergence and beam deviation through refractive bending, as well as general agreement with modelling, lead us to conclude that, for germanium, the main influence of the prepulse is (a) to increase the energy absorbed from the main pulse, (b) to increase the volume of the gain zone and (c) to relax the plasma density gradients, particularly in the J=0-1 gain zone.