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MOG performance
There are many performance data that specify a complex unit like
MOG. We have concentrated on ergonomics, but always with the
ultimate laser linewidth in mind. Our lasers are limited by
the optical characteristics of the external cavity; MOG noise is inconsequential. Our normal
cavities are short (20mm), the grating feedback is small (10%), and
the diodes are not AR coated; the linewidth is typically around 300kHz (FWHM).
We have demonstrated linewidths of 160kHz fwhm (full width at half max), below 70kHz rms, measured over tens of seconds.
Current noise
The curve above shows the diode injection current noise (or lack thereof). Measured at 100mA into four 1N4148 diodes (effective resistance about 3.5 ohms). Black trace is short-circuit, blue is with current on. Unfortunately we cannot distinguish the traces; the current noise level is below -140dBm (at 10Hz RBW).
Frequency noise Here we show typical feedback error signal noise spectra with a MOGunit.
Linewidth The figure below shows a self-heterodyne beatnote for a single diode laser, locked to a rubidium transition. The beatnote width was roughly 80kHz (FWHM; 35kHz rms). Our linewidth measurements are described in Linewidths below 100 kHz with external cavity diode lasers, Appl. Opt. 48 6961-6966 (2009). The self-heterodyne technique is described in Electron. Lett. 16 630-631 (1980).
Scan range The scan range available depends very much on the mechanical and optical design of your laser. Using a standard laser diode for cd-rom writing applications (Sharp GH0781JA2C or Roithner Lasertechnik ADL-78901TX), without special coatings, and a low-efficiency 1800l/mm grating, scans of about 1GHz are typical in a Littrow configuration. Increased scan range is possible by careful design of the pivot point of the grating, so that the frequency change due to the change in cavity length closely matches the frequency change due to the change in grating angle. See for example our recent paper Appl. Opt., 48 6692-6700 (2010). We can instead ramp the diode injection current and cavity length (piezo) together. With standard uncoated diode, low-feedback grating and Littrow configuration, we can scan the entire 780nm rubidium hyperfine structure for both naturally occurring isotopes, nearly 10GHz. The figure below shows the saturated absorption and MOG error signal with a standard MOGbox.
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