Related Experiment Video
Updated: Jul 24, 2026

05:20
Characterization of Thermal Transport in One-dimensional Solid Materials
Published on: January 26, 2014
Characterization of milk properties with a radiative transfer model
Czarena L Crofcheck1, Fred A Payne, M Pinar Mengüç
1University of Kentucky, Lexington 40546-0276, USA. ccrofche@bae.uky.edu
Applied Optics
|April 9, 2002
Summary
This study used a radiative transfer model to analyze light scattering in milk. The model accurately characterized milk properties, showing high sensitivity to fat globule size and distribution.
Area of Science:
- Dairy Science
- Optical Physics
- Food Science
Background:
- Milk composition analysis is crucial for quality control.
- Light-scattering techniques offer non-invasive methods for characterizing milk.
Purpose of the Study:
- To develop and validate a semianalytical radiative transfer model for milk characterization.
- To simulate light backscatter in homogenized milk with varying fat content.
Main Methods:
- Utilized a semianalytical radiative transfer model.
- Simulated light backscatter in milk (0.05-3.2 wt.% fat).
- Input parameters included wavelength, refractive index, and particle density.
Main Results:
- Achieved reasonable model-data fit for lower fat milks by varying wavelength.
- Model sensitivity was highest for particle diameter and size distribution.
- Model showed lower sensitivity to particle number and refractive index.
Conclusions:
- The radiative transfer model effectively characterizes milk optical properties.
- Particle size and distribution are key determinants of light scattering in milk.
- This approach aids in understanding milk composition through optical measurements.
Related Concept Videos
Mechanism of heat transfer
Understanding heat transfer mechanisms is essential for understanding how our bodies maintain balance in different environmental conditions. When the environment is thermoneutral, the body is in a state of balance, neither using nor releasing energy to maintain its core temperature. However, when the environment is not thermoneutral, the body employs four heat transfer mechanisms to maintain homeostasis: conduction, convection, evaporation, and radiation. These mechanisms facilitate heat...
Radiation: Applications
The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
The average...
Absorption of Radiation
The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
Conduction, Convection and Radiation: Problem Solving
There are three methods by which heat transfer can take place: conduction, convection, and radiation. Each method has unique and interesting characteristics, but all three have two things in common: they transfer heat solely because of a temperature difference; and the greater the temperature difference, the faster the heat transfer.
In order to solve a problem related to heat transfer, first of all, the situation needs to be examined to determine the type of heat transfer involved. This could...
In order to solve a problem related to heat transfer, first of all, the situation needs to be examined to determine the type of heat transfer involved. This could...
Maxwell-Boltzmann Distribution: Problem Solving
Individual molecules in a gas move in random directions, but a gas containing numerous molecules has a predictable distribution of molecular speeds, which is known as the Maxwell-Boltzmann distribution, f(v).
This distribution function f(v) is defined by saying that the expected number N (v1,v2) of particles with speeds between v1 and v2 is given by
This distribution function f(v) is defined by saying that the expected number N (v1,v2) of particles with speeds between v1 and v2 is given by
Maxwell's Thermodynamic Relations
Maxwell's thermodynamic relations are very useful in solving problems in thermodynamics. Each of Maxwell's relations relates a partial differential between quantities that can be hard to measure experimentally to a partial differential between quantities that can be easily measured. These relations are a set of equations derivable from the symmetry of the second derivatives and the thermodynamic potentials.
All thermodynamic potentials are exact differentials. Therefore, their second-order...
All thermodynamic potentials are exact differentials. Therefore, their second-order...

