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

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The Rayleigh (2) Integrating along the line of sight l [m]: ∞ (3) 4πLγ = ǫ(l, t, λ)dl 0 This quantity is the column emission rate, which Hunten et al. [1956] proposed as a radiometric unit for the aurora and airglow. UNIS 2011-11-15 – p. 22
The Rayleigh (3) In SI-units the Rayleigh becomes [Baker and Romick, 1976]: (4) 1 [Rayleigh] ≡ 1 [R] 10 10 photons s m 2 (column) The word column denotes the concept of an emission-rate from a column of unspecified length, as discussed above. It should be noted that the Rayleigh is an apparent emission rate, not taking absorption or scattering into account. UNIS 2011-11-15 – p. 23
Page 1 and 2: Basic radiometry and SNR equations
Page 3 and 4: This is about taking pictures of da
Page 5 and 6: Radiometry UNIS 2011-11-15 - p. 5
Page 7 and 8: Radiometry vs. photometry Holst [19
Page 9 and 10: 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: The Rayleigh (1) Consider a cylindr
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 and 62: Dynamic range (1) The Dynamic Range
Page 63 and 64: ICCD UNIS 2011-11-15 - p. 51
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 75 and 76:
Where are my photons? • Transmitt
Page 77 and 78:
Where are my photons? • Transmitt
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
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Intercalibration UNIS 2011-11-15 -
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The European Rayleigh UNIS 2011-11-
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Intercal. procedure • Calibrators
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25 20 15 10 5 Intercal. workshops N
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and the FMI-sphere UNIS 2011-11-15
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[Rayleighs/Angstrom] 1000 100 10 1
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Calibration issues UNIS 2011-11-15
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Abs. calibration (ALIS) UNIS 2011-1
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ALIS UNIS 2011-11-15 - p. 81
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Spectroscopic imaging 4000 4500 500
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Scientific results and capabilities
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UNIS 2011-11-15 - p. 87
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electron energy 10 2 10 1 10 0 Auro
Page 111 and 112:
UNIS 2011-11-15 - p. 90
Page 113 and 114:
UNIS 2011-11-15 - p. 92
Page 115 and 116:
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
Page 129 and 130:
Page 131 and 132:
Page 133 and 134:
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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