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Light Detectors

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Current through bolometer should be kept Constant. Temperature rise due to joule's heating limits the maximum current through bolometer ... – PowerPoint PPT presentation

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Title: Light Detectors


1
Title
  • Light Detectors

2
Characteristics
  • Sensitivity
  • Accuracy
  • Spectral Relative Response(R(?))
  • Absolute Sensitivity(S(?))
  • Signal-to-noise ratio
  • --Noise equivalent input power
  • http//www.electron-tubes.co.uk/pmts/pmt_select.ht
    ml

3
Characteristics
  • Intensity range
  • Response time
  • -effect of detector time constant
  • Price

4
Types of Detectors
  • Light Detectors can be classified int
  • Thermal Detectors
  • --changes the temperature dependent
    properties of detectors
  • --wavelength independent sensitivity
  • --sensitivity depends on detector parameters
  • --heat capacitance
  • --thermal losses

5
Thermal Detectors
  • Time constant of detector depends ratio of heat
    capacitance and thermal losses
  • ? H/G
  • where Hheat
    capacity

  • Gthermal losses
  • --Sensitive to small values of G
  • --time constant of detector limits the
    frequency of detector

6
Thermal Detectors
  • Calorimeter

7
Thermal Detectors
8
Thermal Detectors
  • Bolometer
  • ?consists of N thermocouples in series

9
  • Limitations
  • Input impedance of the amplifier should be larger
    than R for a change in current
  • Current through bolometer should be kept Constant
  • Temperature rise due to joules heating limits
    the maximum current through bolometer

10
Golay Cell
11
Direct Photo detectors
  • Direct Photo detectors are based on
  • ? spectral based on emission of
    photoelectrons
  • ? changes in conductivity of semiconductors
  • ? voltage generated by the internal photo
    effect
  • ?spectral response depends on work function
    or
  • band gap

12
Photodiode
  • Doped semiconductors
  • Can be either photovoltaic or photoconductive
  • P-n junction when irradiated generates
    photovoltage
  • Photoconductive elements change their internal
    resistance

13
Photodiode
14
Photodiode
15
Photodiode
  • Absorption coefficient is spectral dependent
  • Should be operated at low temperature in order to
    minimize thermal excitation of electrons
  • ?For ?lt 10 micrometers liquid nitrogen
  • For ?gt 10 micrometers liquid helium
  • add figure 4.81 and 4.82

16
Photodiode
17
Photoconductive diodes
  • When illuminated its electric resistance
    decreases
  • Time constant is dependent on diffusion time of
    electrons

18
Photovoltaic detector
  • When illuminated generates electron-hole pairs

19
Photodiode
20
Photo Emissive Detectors
  • Depend on external photoeffect
  • Photocathode is of low work function

21
Photo multiplier Tubes
  • Used in detection of low light levels
  • Overcomes noise limitation by using dynodes
  • Amplification factor depends on accelerating
    voltage U, incident angle,dynode material

22
Photo multiplier Tubes
  • Noise sources are
  • Photomultiplier dark current
  • Noise of the incoming radiation
  • Shot noise and johnson noise caused by
    fluctuations of the amplication
  • Noise of the load resistor

23
Photon Counting
24
Streak Camera
  • Definition

?The streak camera is a device which measures
ultra-fast light phenomena and delivers intensity
vs. time vs. position (or wavelength) information
25
Streak Camera
26
Streak Camera
  • Since the deflection sensitivity can be as high
    as 100 volts/cm, it can be seen that a drive
    pulse with rise time of 2000 volts/ns gives rise
    to a time base of 50 ps/cm. (The maximum
    deflection speed is approximately the speed of
    light.)
  • The readout system typically an image
    intensified CCD camera can clearly resolve 100
    microns or less, giving an overall time
    resolution of 1 ps, or less.

27
Streak Camera
  • The streak image can contain spatial information.
    In a typical application the spatial information
    could be spectra, so the image shows
    intensity/time information over a spectral range
    of interest.

28
Streak Camera
  • Time resolved spectroscopy
  • ?When used in combination with a spectroscope,
    time variation of the incident light intensity
    with respect to wavelength can be measured

29
Why do we need a Streak Camera
  • Time-resolved spectroscopy, fluorescence,
    absorption and Raman scattering are all extremely
    important techniques needed to understand many
    chemical, biological and physical processes.
  • Fundamental processes caused by excited
    molecules, such as energy transfer, proton
    transfer and vibrational relaxation, occur on an
    ultrafast time scale.

30
Why do we need a Streak Camera
  • Time-resolved spectroscopy using streak
    technology is capable of capturing spectra of
    such fast processes in their transitional states
  • studying their dynamic behavior with temporal
    resolutions ranging in the nanosecond to
    sub-picosecond domain.

31
Streak Camera
  • Parameters
  • ?Slit width and read out pixel
  • ?Tube Spatial Resolution
  • ?Magnification and Deflection Speed
  • ?Chromatic Aberration and Space Charge
  • Limitation
  • ?Scale Effects (Small is Beautiful?)

32
Streak Camera
  • Features
  • Simultaneous measurement of light intensity on
    both the temporal and spatial axis (wavelength
    axis)By positioning a multi-channel spectroscope
    in front of the slit (for the incident light) of
    the streak camera, the spatial axis is reckoned
    for the wavelength axis. This enables changes in
    the light intensity on the various wavelengths to
    be measured (time-resolved spectroscopy).

33
Streak Camera
  • Superb temporal resolution of less than 0.2
    psThe streak camera boasts a superb maximum
    temporal resolution of 0.2 ps. This value of 0.2
    ps corresponds to the time it takes for light to
    advance a mere 0.06 mm.
  • Handles anything from single event phenomena to
    high-repetition phenomena in the GHz rangeA wide
    range of phenomena can be measured simply by
    replacing the modular sweep unit.

34
Streak Camera
  • Measurement ranges from X-rays to the near
    infrared raysA streak tube (detector) can be
    selected to match any wave-length range from
    X-rays to near infrared rays.
  • Ultra-high sensitivity (single photoelectron can
    be detected)The streak tube converts light into
    electrons, and then multiply it electrically. By
    this, it can measure faint light phenomena not to
    be seen by the human eyes. This enables
    monitoring of extremely faint light even single
    photoelectron can be detected.

35
Streak Camera
  • Dedicated readout systemA dedicated readout
    system is available which allows images recorded
    by a streak camera (streak images) to be
    displayed on video monitor and analyzed in real
    time. This enables the data to be analyzed
    immediately without the delay of film processing.
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