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Basic radiometry and SNR equations
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This is about taking pictures of da
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Radiometry UNIS 2011-11-15 - p. 5
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Radiometry vs. photometry Holst [19
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Radiometry “Mathematics is often
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Photon flux: in energy units: Flux
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Spectral radiance Also known as spe
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Spectral irradiance Also known as s
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At apperture: Eγapp = Φγapp Aapp
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Photometric units scoptic—rods (K
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The foot-lambert A foot-lambert or
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The Rayleigh (1) Consider a cylindr
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The Rayleigh (3) In SI-units the Ra
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By now you should realized that. .
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. . . God said: Go to, let us go do
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and now. . . UNIS 2011-11-15 - p. 2
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The 4π confusion Therefore, we pro
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Can we agree on this? The apparent
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Still confused. . . . . . but at a
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Where are my photons? • Transmitt
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Where are my photons? • Transmitt
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Where are my photons? • Transmitt
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What is noise? UNIS 2011-11-15 - p.
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Notation 〈X〉 2 variance of X
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E2V TECH CCD201 UNIS 2011-11-15 - p
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CCD-noise sources UNIS 2011-11-15 -
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(20) (21) (22) 〈n e − s 〉 = =
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(23) (24) 〈n e − p 〉 = Patter
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Signal-to-noise ratio for a CCD •
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Signal-to-noise ratio for a CCD •
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Dynamic range (1) The Dynamic Range
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ICCD UNIS 2011-11-15 - p. 51
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SNR for a CCD • Measured signal-t
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SNR for a CCD • Measured signal-t
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SNR for an ICCD • The signal-to-n
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SNR for an emCCD The signal-to-nois
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SNR vs. of integration time SNR 100
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Where are my photons? • Transmitt
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Where are my photons? • Transmitt
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SNR: CCD, ICCD and emCCD SNR 1000 1
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SNR Fast: ≈ 2900 photons/pixel 10
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SNR Slow: ≈ 42 photons/pixel 100
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Intercalibration UNIS 2011-11-15 -
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- Page 109 and 110: electron energy 10 2 10 1 10 0 Auro
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- Page 117 and 118: Radio-induced optical emissions UNI
- Page 119 and 120: Tomography of RIOE After Gustavsson
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- Page 125 and 126: Future plans and challenges UNIS 20
- Page 127 and 128: We do not understand: • Creation
- Page 129 and 130: We do not understand: • Creation
- Page 131 and 132: We do not understand: • Creation
- Page 133 and 134: ALIS 2010-2014 • Electrodynamics
- Page 135 and 136: and now. . . UNIS 2011-11-15 - p. 1
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