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Interference and Diffraction02:18

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Interference is a characteristic phenomenon exhibited by waves. When two electromagnetic waves interact with their peaks and troughs coinciding, a resulting wave with enhanced amplitude is produced. This is known as constructive interference. In this case, the two waves interacting are in phase with each other.
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The dipole moment of a bond is the product of the partial charge on either atom and the distance between them. Dipole moments influence the efficiency of IR absorption and the peak intensity. When a bond with a dipole moment is placed in an electric field, the direction of the field determines if the bond is compressed or stretched. Electromagnetic radiation consists of an electric field component that rapidly reverses direction. It follows that polar bonds are alternately stretched and...
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In atomic emission spectroscopy (AES), high-temperature atomizers excite a broad range of elements and molecules that generate complex emissions from sources such as oxides, hydroxides, and flame combustion products in the flame or plasma. Several strategies can be employed to minimize spectral interferences caused by overlapping emission lines or bands. These include increasing instrument resolution, choosing alternative emission lines, optimally placing the detector in low-background regions,...
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Measurement of Quantum Interference in a Silicon Ring Resonator Photon Source
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Cramer-Rao bounds for intensity interferometry measurements.

Richard Holmes1, Brandoch Calef, D Gerwe

  • 1Boeing Laser Technical Services, 535 Lipoa Parkway, Suite 200, Kihei, Hawaii 96753, USA. richard.b.holmes@boeing.com

Applied Optics
|July 23, 2013
PubMed
Summary
This summary is machine-generated.

Innovations in signal processing can improve signal-to-noise ratio (SNR) in intensity interferometry. Using object shape knowledge offers potential gains, but constraints can introduce biases that impact overall error.

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Area of Science:

  • Astronomy and Astrophysics
  • Signal Processing
  • Statistical Inference

Background:

  • Signal-to-noise ratio (SNR) in intensity interferometry is crucial for astronomical observations.
  • Recent advancements in signal processing offer potential improvements to SNR.

Purpose of the Study:

  • To investigate the potential SNR gains from using positivity and object shape knowledge in intensity interferometry.
  • To analyze these gains using Cramer-Rao lower bounds (CRLB).

Main Methods:

  • Application of Cramer-Rao lower bounds (CRLB) to evaluate estimators.
  • Analysis of positivity-constrained maximum likelihood (ML) estimators.
  • Investigation of the impact of prior knowledge on estimator variance.

Main Results:

  • Positivity constraints can reduce estimator variance by up to 75% compared to unconstrained estimators.
  • Positivity-constrained ML estimators offer a best-case variance reduction of 34.1%.
  • Prior knowledge gains are dependent on information quality; biases can offset variance reduction.

Conclusions:

  • Positivity and object shape knowledge can enhance SNR in intensity interferometry.
  • CRLB provides a framework to quantify gains and understand limitations, including induced biases.
  • Careful consideration of constraints and prior information is necessary to optimize total error reduction.