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Thermal Radiation (Rosseland)

Mathematical Modelling — Fluid Dynamics & Heat TransferContinuum mechanics; boundary-layer similarity theory

T⁻¹Θ

Symbol

Radiative flux by the Rosseland diffusion approximation, linearised about the ambient temperature.

Main equation
Level 0 of 6
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Dimension:T⁻¹Θ (s⁻¹ K)Maths:ℝ scalar(·, ·, ·) — A single number (real numbers), depending on another quantity, another quantity, another quantityDimensionally verifiedMathematically verifiedFully reduced to base quantities

In words:times.

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Domain Analysis

Unit status, dimensional trails, per-step checks, and custom unit expressions.

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Reads as: q_r

“q_r” is analysed by expanding its full defining equation (its children and their relations), not as a bare symbol. Use Check this concept’s units above for the same result.

Mathematical Analysis

Object type, lawful operations, conditions, comparisons, and derivation-step checks.

Also known as:qr

Equation

Dimension I

Definition

What it is — and what it is not

What it is
  • S1Thermal radiation modelled by the Rosseland diffusion approximation.
Boundary of meaning
  • S2The optically thick (Rosseland) assumption holds only for a strongly absorbing/emitting medium.
Attributes
  • S3Linearised about the ambient temperature, contributing a radiative flux divergence. [1.1]

Dimension II

In practice

How to deal with it

Warnings
  • S4Linearised Rosseland radiation is mathematically equivalent to an effective Prandtl number (Magyari & Pantokratoras, 2011): Rd adds no physics independent of conduction in this form. Nonlinear (full T⁴) radiation is required for radiation to act as genuine separate physics. [3.1]

Sub-topics 2

Related

References

  1. Aziz et al. (2021), DOI 10.1007/s10973-020-10210-2.

    • 1.1

      Radiation closure — The article supports use of linear thermal radiation, not the proposalʼs chapter equation numbering.

      AmbiguityCorroborated

      Rosseland diffusion requires an optically thick medium; linearising T⁴ about T∞ additionally requires a modest temperature ratio.

  2. Rosseland (1936), Theoretical Astrophysics.

    • 2.1

      Diffusion approximation — q_r = −(4σ*/3k*)∂T⁴/∂y — valid for an optically thick medium.

      Established
  3. Magyari & Pantokratoras (2011), ICHMT 38, 554–556.

    • 3.1

      ICHMT 38, 554–556 — With T⁴ linearised about T∞, the "radiation parameter" only rescales conduction: results at (Pr, Rd) coincide with pure conduction at Pr_eff = Pr/(1 + 4Rd/3). Rd sweeps must be interpreted as effective-Prandtl sweeps.

      Established
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