Data from 01.08.22
Using a 7x1 array to show the importance of phases when generating multitone signal.
CCD camera is positioned after 2D AOD. 
Using the new AWG code, frequency tones have 2.5MHz separation: [90,92.5,95,97.5,100,102.5,105].
Vrms scales proportionally to input power. For amp 0.227 Vrms is 103mV
crest factors:
Same	Random	Optimised 
3.7	2.5	1.9

Folders:
Each folder contains images named by the % optical power requested for each trap.
Amp_same_phase: all tones have phase of 0
Amp_random_phase: manually set phases to [331.08234304, 261.28265977, 37.20895749, 108.47695932, 269.15452107, 169.61955156, 122.15325531]
Amp_optimised_phase: individually optimise phase of each tone in turn to minimise the crest factor: [0.0, 66.93430366136724, 198.31992814428708, 9.682335024151481, 250.34879192186617, 166.33752127977093, 157.27470779218316]




Other data from 18.07.22
CCD placed in 1:1 telescope after 2D AOD in 817 tweezer path.

The array phases and individual frequency amplitudes were previously optimised,
so that the trap powers should be within 1% of each other. 
However, the powers are quite clearly unbalanced.

1_0.bmp   -- The data sent to CH0 has an rms amplitude of 107mV. 
Using the amplitudes that should balance trap powers.
0.8_0.bmp -- 94mV. scale all frequency tone amplitudes by a factor of 0.8.
1.2_0.bmp -- 121mV. scale by 1.2
1.4_0.bmp -- 135mV. scale by 1.4
1.5_0.bmp -- 140mV. scale by 1.5
