A. Principle of LE-1800 Pr:YLF Laser PL4000
The emission of a blue (444 nm) diode laser is collimated with a short focal lens (CO). The lens (FL) focuses the pump light through the mirror M1 into the Pr:YLF crystal. The mirrors M1 and M2 are forming a hemispherical cavity for the Pr:YLFlaser. The mirror M2 is mounted onto a translation mechanism to extend or shorten the cavity length by 5 mm. This is useful to verify the optical stability range and different transversal modes. The filter (FI) blocks not absorbed pump light and SC serves as visualization screen for fluorescence spots as well as transversal modes.
B. Pr:YLF Laser PL4000 with attached lateral photodetector (PD)
C. Measuring the lifetime of the excited state
To measure only the fluorescence radiation without disturbing strong pump light, the photodetector (PD) is mounted perpendicular to the optical axis near the Ruby crystal. The photodetector is connected to the controller and operates in bias mode with software selectable shunt resistors and the output is connected to an oscilloscope. The injection current of the laser diode (VLD) is periodically switched on and off by the controller. The provided reference signal of the injection current is also connected to the oscilloscope and serves as trigger source on falling edge.
The corresponding oscilloscope track is shown in Fig. C. From the decay curve of the fluorescence signal the lifetime of the excited state is determined. The inverse value of it is related to Einstein coefficient for spontaneous emission.
D. Photodetector to measure the the dynamic properties of the Pr:YLF laser
To measure the Ruby laser output a detector with a filter to block the violet pump radiation is used. The signal of the photodetector and the reference signal of the injection current is displayed on the oscilloscope.
E. Selection of Laser Lines with Mirrors
The curved mirror M2 is highly reflective (99%) in the 500–700 nm range. To select the wavelengths of 523, 607, and 638, we use three differently coated mirrors. The reflectivity of each mirror is >99% only for the desired wavelength and < 50% for the undesired wavelengths. In a hemispherical laser resonator, the alignment of the plane mirror is not as critical. Therefore, we swap it out for the desired wavelength. The mirror holders are held in a defined position by magnets, so that the resonator remains aligned even after a mirror change. The mount for the laser mirror holder features a magnetic sensor that is monitored by the microprocessor. If no mirror is inserted, the processor turns off the pump laser diode; as soon as a mirror is detected, the pump laser diode can be turned back on.
F. Rayleigh Scattering
View into the cavity. Operating the green (523 nm) line
Because the output power from mirror M2 is low, the laser radiation inside the resonator has a high intensity. This leads to a unique phenomenon known as Rayleigh scattering. The dipoles of the air molecules are aligned by the high field strength and emit scattered radiation perpendicular to it. The polarization of the scattered radiation can be visually detected using a polarization analyzer.
G. CCD camera to measure the laser intensity distribution
The filter and camera modules are inserted into their respective slots. The camera's CCD chip is illuminated directly by the laser beam. Gray filters (ND) with optical densities of OD2, OD3, and OD4 are inserted into the filter module; these reduce the intensity enough to prevent the camera from being overdriven. The camera is connected to a Raspberry Pi with a 7-inch screen.

Green TEM
0 0

Green TEM
2 0

Red TEM
1 1

Red TEM
11 0
Display and measuring the intensity distribution of a TEM00 Pr:YLF laser mode
The CCD image can be obtained from the Raspberry PI as real time image file (jpg) or as XY array data (csv.