EO Flashcards

1
Q

Which three parts of the EM spectrum does EO cover?

A
  1. Ultraviolet (UV): From 10 nm up to 400 nm
  2. Visible Spectrum: Between 400 and 700 nm
  3. Infrared (IR): Up to approximately 1 mm wavelength
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2
Q

Which four factors affect the general detection problem?

A
  1. Scene illumination and illuminance
  2. Target and background contrast
  3. Atmospheric conditions
  4. Detector quality
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3
Q

What can be used as visual cues in optical systems?

A

McTEC

  1. Movement
  2. Contrast
  3. Texture
  4. Edges and outlines
  5. Colour (relevant only in daylight)
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4
Q

What are the atmospheric transmission windows for IR radiation?

A
  1. Short-wavelength infrared (SWIR): 3 µm to 5 µm
  2. Mid-wavelength infrared (MWIR): 8 µm to 14 µm.
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5
Q

Explain atmospheric absorption and scattering.

A

• Atmospheric Absorption: Gases like water vapour and carbon dioxide absorb IR radiation, reducing target contrast.

• Scattering: Caused by aerosols and particles, it leads to diffraction, absorption, and reflection of radiation.

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6
Q

What was the name of the first-generation image intensifier? What were its limitations?

A

Cascade Intensifier.

Converted photons to electrons, amplifying them, and converting them back to visible light.

Its limitations included large power requirements, bulky/heavy size and low resolution.

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7
Q

What is the technology associated with modern (second/third gen) II systems? What are its major advantages?

A

Modern image intensification - To amplify light more efficiently.

Significant advantages include higher resolution, better sensitivity, and reduced size and weight.

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8
Q

Explain what is meant by blackbody, grey-body, and selective radiators.

A

• Blackbody: An idealised object that absorbs all incident radiation and re-emits it perfectly.

• Grey-body: A real object that does not absorb all incident radiation but emits a fraction of it based on its emissivity.

• Selective Radiator: Emits radiation at specific wavelengths or bands, typically gases at high temperatures emitting line spectra.

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9
Q

What type of materials are sources of the above types of radiation?

A

• Blackbody: The idealised theoretical model in which no perfect blackbody exists, but stars are close approximations.

• Grey-body: Most real-world objects, such as earth surfaces, buildings, and vehicles.

• Selective Radiator: Gases like those in jet engine exhaust or gas-discharge lamps.

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10
Q

Briefly compare thermal and photon detectors, stating the advantages and disadvantages of each. If designing a horizon surveillance system, which detector would you use and why?

A

• Thermal Detectors: Measure temperature changes, typically slower response times, and no cooling required.
Advantage: Good sensitivity over a wide range of wavelengths.
Disadvantage: Slower response.

• Photon Detectors: Measure individual photon events, faster response times, often require cooling. Advantage: Higher sensitivity and quicker response.
Disadvantage: Requires cooling. Photon detectors would be preferred for horizon surveillance due to their higher sensitivity and faster response times.

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11
Q

What are the 2 types of cooling available for photon detectors, which is most appropriate for a missile IR seeker, and why? What temperature do these coolers operate at typically?

A

• Thermoelectric Cooling: Suitable for less demanding applications.
• Cryogenic Cooling: Most appropriate for missile IR seekers due to the need for high sensitivity and low noise. These coolers typically operate at around 77 K (liquid nitrogen) or lower temperatures.

77K!!!!!!

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12
Q

Compare and contrast serial scan, parallel scan, and fully staring arrays. What is a SPRITE detector, and how does it work?

A

• Serial Scan: Sequentially scans the scene, typically slower.
• Parallel Scan: Scans multiple lines simultaneously, faster than serial.
• Fully Staring Arrays: The entire scene is imaged simultaneously, with no moving parts, the fastest.
• SPRITE Detector: (Signal PRocessing In The Element) uses a continuous strip of photodetector material to improve signal processing within each detector element, enhancing sensitivity and resolution.

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13
Q

What is spontaneous emission?

A

Spontaneous emission is when an excited electron spontaneously falls to a lower energy state, emitting a photon without external stimulation.

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14
Q

What is stimulated emission?

A

Stimulated emission occurs when an incoming photon causes an excited electron to fall to a lower energy state, emitting a photon coherent with the stimulating photon.

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