Quark (chromosphere version) #3

(Sept 2023)



This Quark was bought in late 2022. It was measured using the following approach:
- Sol'Ex spectrometer in a f/31.4 telecentric beam (TOA 150 f/7.3 => Quark with its 4.3× telecentric => Sol'Ex),

Filter Test method f-ratio Surface  measured FSR FWHM Bandwith at 10% peak transmission
Quark #3 Sol'Ex spectro
(fc =fi = 200 mm, ASI 462, 0.0471 A/px dispersion)
f/31.4 telecentric 10 micron x 4.5 mm 23.0 A 0.45 A 1.3 A
(consistent with a FWHM of 0.45 A)





Sol'Ex spectrometer: measurement in a f/31.4 telecentric beam

Optical setup: Sun =>
Takahashi TOA 150  => Quark with its 4.3× telecentric beam => Sol'Ex spectrograph

10 microns slit, 200 mm collimating lens, 200 mm imaging lens, ASI 462 camera, 12-bit acquisition.
Measured dispersion = 0.0471 A/pixel
Conditions :  blue sky
6 September 2023





Three succesive images :
- Solar spectrum (= no filter).
- Solar spectrum transmitted by the Quark at ambiant temperature (about 30°C). This spectrum is registered to the solar spectrum.
- Same as above, but different vizualisation thresholds for the measurement of the FSR.




The FSR is equal to 23.0 A
 

The transmission profile of the etalon is given by the ratio "transmitted solar spectrum/solar spectrum". 

  

The direct measurement on the graph at 50 % and 10% peak transmission are given on the graphs.

Estimation of the FWHM with curve-fitted of the transmisison curve with a Lorentzian function gives a similar value, FWHM = 0.46 A

The bandwidth at 10% transmission is consistent with a FWHM = 1.33/3 = 0.44 A


Given the broadening of the FWHM at f/31.5, we can deduce a nominal FWHM < 0.45 A





 
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