Basic radiometry and SNR eq. for CCD, ICCD - UNIS

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Dynamic range (2) An approximate theoretical value for DR is obtained by dividing the maximum signal by the total noise (37) DR ≈ 20 log 10 n e − max − n e − d 〈n e − tot 〉 [dB] UNIS 2011-11-15 – p. 50
ICCD UNIS 2011-11-15 – p. 51
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Basic radiometry and SNR equations
Page 3 and 4:
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
Page 11 and 12: Photon flux: in energy units: Flux
Page 13 and 14: Spectral radiance Also known as spe
Page 15 and 16: Spectral irradiance Also known as s
Page 17 and 18: At apperture: Eγapp = Φγapp Aapp
Page 19 and 20: Photometric units scoptic—rods (K
Page 21 and 22: The foot-lambert A foot-lambert or
Page 23 and 24: The Rayleigh (1) Consider a cylindr
Page 25 and 26: The Rayleigh (3) In SI-units the Ra
Page 27 and 28: By now you should realized that. .
Page 29 and 30: . . . God said: Go to, let us go do
Page 31 and 32: and now. . . UNIS 2011-11-15 - p. 2
Page 33 and 34: The 4π confusion Therefore, we pro
Page 35 and 36: Can we agree on this? The apparent
Page 37 and 38: Still confused. . . . . . but at a
Page 39 and 40: Where are my photons? • Transmitt
Page 45 and 46: What is noise? UNIS 2011-11-15 - p.
Page 47 and 48: Notation 〈X〉 2 variance of X
Page 49 and 50: E2V TECH CCD201 UNIS 2011-11-15 - p
Page 51 and 52: CCD-noise sources UNIS 2011-11-15 -
Page 53 and 54: (20) (21) (22) 〈n e − s 〉 = =
Page 55 and 56: (23) (24) 〈n e − p 〉 = Patter
Page 57 and 58: Signal-to-noise ratio for a CCD •
Page 59 and 60: Signal-to-noise ratio for a CCD •
Page 61: Dynamic range (1) The Dynamic Range
Page 65 and 66: SNR for a CCD • Measured signal-t
Page 67 and 68: SNR for a CCD • Measured signal-t
Page 69 and 70: SNR for an ICCD • The signal-to-n
Page 71 and 72: SNR for an emCCD The signal-to-nois
Page 73 and 74: SNR vs. of integration time SNR 100
Page 79 and 80: SNR: CCD, ICCD and emCCD SNR 1000 1
Page 81 and 82: SNR Fast: ≈ 2900 photons/pixel 10
Page 83 and 84: SNR Slow: ≈ 42 photons/pixel 100
Page 85 and 86: Intercalibration UNIS 2011-11-15 -
Page 87 and 88: The European Rayleigh UNIS 2011-11-
Page 89 and 90: Intercal. procedure • Calibrators
Page 91 and 92: 25 20 15 10 5 Intercal. workshops N
Page 93 and 94: and the FMI-sphere UNIS 2011-11-15
Page 95 and 96: [Rayleighs/Angstrom] 1000 100 10 1
Page 97 and 98: Calibration issues UNIS 2011-11-15
Page 99 and 100: Abs. calibration (ALIS) UNIS 2011-1
Page 101 and 102: ALIS UNIS 2011-11-15 - p. 81
Page 103 and 104: Spectroscopic imaging 4000 4500 500
Page 105 and 106: Scientific results and capabilities
Page 107 and 108: UNIS 2011-11-15 - p. 87
Page 109 and 110: electron energy 10 2 10 1 10 0 Auro
Page 111 and 112: UNIS 2011-11-15 - p. 90
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UNIS 2011-11-15 - p. 92
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UNIS 2011-11-15 - p. 94
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Radio-induced optical emissions UNI
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Tomography of RIOE After Gustavsson
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UNIS 2011-11-15 - p. 100
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A strange meteor trail 130 120 110
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Future plans and challenges UNIS 20
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We do not understand: • Creation
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Page 131 and 132:
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ALIS 2010-2014 • Electrodynamics
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and now. . . UNIS 2011-11-15 - p. 1
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It’s The end! UNIS 2011-11-15 - p
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The end? Kiruna ASC 2007-02-05 17.3
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Enell, C.-F., Optical studies of po
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Basic radiometry and SNR eq. for CCD, ICCD - UNIS

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