This 1990 paper says “The main and expected result is that both 1.4 mm lasers give a ‘double hump’ or Bactrian P(φ) curve…Clearly, if a tilted (dispersed) wavelength offers more power than the Littrow-selected one, the implications for grating-tuned line selection are amusing”.
This was lighthearted but serious. We had predicted and demonstrated why some grating-tuned waveguide lasers show a reduced (or even zero) range of operation at wavelengths for which the cavity has been built and aligned with all possible care. It is well aligned – but it does not obey single-mode theory.
We now had a combination of understanding and computer codes that offered a chance to design – with far less trial and error – lasers that were stable against modest perturbations. I made the point to colleagues in RSRE/DRA/DERA, UK industry, and the NATO RSG-13 panel on laser technology (see insert below). Already in the 1980s and into the 1990s much time and money had been spent on badly behaved lasers before their perturbation behaviour was appreciated and corrected. I do not say that UK lasers in the programmes to which I had access were particularly poor, or worse than those made elsewhere.
In the specific area of this article, one of our 1990s lidar technical demonstrators called for two CO2 waveguide lasers, one large and one small. The proposed large laser had been developed through some years of “VX” contract work, initially aimed at a 20 W upgrade for RSRE’s FINDER lidar. It had a folded cavity with an electro-optic crystal modulator; it was intended to run quasi-TEM00 in pulsed and CW modes, but suffered from power loss and mode distortion.
In 1990, alarmed, I was not always right or tactful, but time was short and I felt bound to speak up. The memo on TEM matrix modelling says “even resonators with EH11-favouring Case III reflectors are prone to mode/alignment problems if N is chosen incorrectly”. Then at the end of October 1990 “Recent work on waveguide resonator theory suggests that the Case III reflector is no guarantee of good mode quality, contrary to generally accepted opinion. There are ranges of guide Fresnel number…where the resonator mode losses and profiles are highly sensitive to misalignment…With this in mind I inspected [the currently proposed design] and found, as expected, that the resonator lay in a region of some risk…During September and October 1990, a detailed resonator model was run by Dr Banerji of Royal Holloway’s Computer Science Department, and his work confirmed my suspicion. If, as seems reasonable but is unproved, the crystal distortion effects are dominated by misalignment (or any process coupling the guide modes of odd and even parity), our [redesign] should raise the threshold at which the fundamental mode is seriously threatened”.
(I was the RSRE technical authority, from late 1987, for this Royal Holloway contract on laser modelling. I make no attempt here at a history of the wider SERL/Baldock/RSRE/DRA/DERA programmes, including Mike’s dedicated work as Hollow Waveguide Optics leader. He and others are far more qualified).
The problems were addressed (to the point of allowing successful flight tests) through a perturbation-insensitive resonator design and, later, an understanding of the polarisation behaviour of lasers with multiple Brewster-angled surfaces [Hill et al. 1996]. The powers obtained in a reasonable low-distortion mode were increased by perhaps 50-70 %. In general, laser weak points tended to be power supplies and cooling systems rather than optics. Obviously I remember the nervous time-pressured decisions about this mid-90s ceramic guide geometry, betting our project funds and future results on my resonator modelling, but it may have been just as important that the thermal sinks were upgraded.
The second laser, used as a local oscillator when the first was in pulsed mode, was designed for reliable near-TEM00 output (as previously demonstrated, in 1988, for a beamrider laser design); it gave very little trouble.
Many will recall this as another period of reorganisation, changing priorities, Severe Restraint in funding, and long delays in contract approval and financing, before “agreed” technical tasks could start. We and UK industry and universities muddled through. In its more commercial guise, DRA showed confidence in my work and won a small contract for my redesign of another beamrider laser. Andrew Scott led our group at the time and helped to negotiate the redesign payment. Also, during the 1990 RSG-13 meeting in Québec / Valcartier I had promised that 1991 would see a UK talk in French, in Paris. This was bold, but Andrew approved some French conversation classes, and soon there were benefits in the MLRS trials and other collaborations with ONERA and French government scientists.
And colleagues will agree that sometimes in the 1990s, as we increased our proportion of bidding and collaborating, issues of etiquette and good practice arose – what should one do? I was now working on Doppler lidar systems for UK and international trials, as well as (with intermittent support) the resonator modelling legacy. Our partners (from the UK and at least two other countries) had, I thought, gone wrong. For instance, the frequency-stabilisation method for an important technical demonstrator lidar source (from one company) was incompatible with its Doppler algorithms (from another); the latter were faulty in any case; nobody noticed until I read manuals for both. Later there was annoyance when I said that the impressively low frequency noise of an expensive lidar source was being swamped by other real-life noises and was irrelevant in practice.
So our large collaborative projects ran bumpily through various administrative and technical challenges, but I must add my appreciation of the managers who allowed essential time and resource for concentrated thinking and calculating: Jayne Ackroyd, Richard Fletcher, Norm Geddes, Kevin Welford and others as well as those mentioned in Section 1.