Barr Ca K filter
Filter |
Test method |
f-ratio |
Surface measured |
FWHM |
BW at 10% peak transmission |
CWL |
Barr Ca K 0.37 nm
|
Sol'Ex spectro
(fc=fi=125 mm) |
f-115
|
10 micron × 4.5 mm |
0.26 nm |
0.48 nm
2-cavity filter |
- 0.7 A |
|
Sol'Ex spectro
(fc=fi=200 mm) |
f-115 |
10 micron × 4.5 mm |
0.26 nm |
0.44 nm
2-cavity filter |
- 0.6 A |
Temperature coefficient : 0.01 A/°C
Measurement in collimated light
# 1 : Optical set-up:
Sun => Sol'Ex spectrograph with 10 micron slit : 10
micron × 4 mm. 125 mm f.l. collimating lens (re-focused on Ca K). Grating : 2400 l/mm. 125 mm f.l. imaging lens. ASI290 camera. 12-bit acquisition. Dispersion: 0.0932 A/pixel.
Very transparent blue sky. Sun near meridian.
Estimated accuracy: +/- 0.1 A for CWL, FWHM and bandwidth at 10% transmisison.
The filter is exposed to nearly perfect collimated light
beam: converging light beam with a 0.5° cone (solar
disk),
equivalent to f-115 ratio. The surface of the filter sampled is
set by the slit size (10 micron x 4 mm)
The following two images show:
- the solar spectrum near Ca K and H,
- the spectrum transmitted by the Barr filter at normal incidence.
Transmission profile at normal incidence
The bandpass at 10% peak transmission being < 2 × FWHM, we can conclude this is a 2-cavity filter.
Measured peak transmission is in the range of 20%.
These measurements with the 125 mm f.l. collimator are in close agreement with the measurements made with the 80 mm collimator (0.1 A difference).
# 2 : Optical set-up:
Sun => Sol'Ex spectrograph with 10 micron slit : 10
micron × 4 mm. 200 mm f.l. collimating and imaging lenses (re-focused on Ca K). Grating : 2400 l/mm. ASI290 camera. 12-bit acquisition. Dispersion: 0.05822 A/pixel.
Blue sky. Sun near meridian.
Note:
The small dents in the transmission profile are artefacts due to non linearity of the camera and/or defocussing.