Book contents
- Frontmatter
- Dedication
- Contents
- Preface
- Acknowledgments
- Acronyms
- 1 Introduction
- 2 The macroscopic Maxwell equations and monochromatic fields
- 3 Fundamental homogeneous-medium solutions of the macroscopic Maxwell equations
- 4 Basic theory of frequency-domain electromagnetic scattering by a fixed finite object
- 5 Far-field scattering
- 6 The Foldy equations
- 7 The Stokes parameters
- 8 Poynting–Stokes tensor
- 9 Polychromatic electromagnetic fields
- 10 Polychromatic scattering by fixed and randomly changing objects
- 11 Measurement of electromagnetic energy flow
- 12 Measurement of the Stokes parameters
- 13 Description of far-field scattering in terms of actual optical observables
- 14 Electromagnetic scattering by a small random group of sparsely distributed particles
- 15 Statistically isotropic and mirror-symmetric random particles
- 16 Numerical computations and laboratory measurements of electromagnetic scattering
- 17 Far-field observables: qualitative and quantitative traits
- 18 Electromagnetic scattering by discrete random media: far field
- 19 Near-field scattering by a sparse discrete random medium: microphysical radiative transfer theory
- 20 Radiative transfer in plane-parallel particulate media
- 21 Weak localization
- 22 Epilogue
- Appendix A Dyads and dyadics
- Appendix B Free-space dyadic Green's function
- Appendix C Euler rotation angles
- Appendix D Spherical-wave decomposition of a plane wave in the far zone
- Appendix E Integration quadrature formulas
- Appendix F Wigner d-functions
- Appendix G Stationary phase evaluation of a double integral
- Appendix H Hints and answers to selected problems
- References
- Index
- Plate Section
11 - Measurement of electromagnetic energy flow
Published online by Cambridge University Press: 05 July 2014
- Frontmatter
- Dedication
- Contents
- Preface
- Acknowledgments
- Acronyms
- 1 Introduction
- 2 The macroscopic Maxwell equations and monochromatic fields
- 3 Fundamental homogeneous-medium solutions of the macroscopic Maxwell equations
- 4 Basic theory of frequency-domain electromagnetic scattering by a fixed finite object
- 5 Far-field scattering
- 6 The Foldy equations
- 7 The Stokes parameters
- 8 Poynting–Stokes tensor
- 9 Polychromatic electromagnetic fields
- 10 Polychromatic scattering by fixed and randomly changing objects
- 11 Measurement of electromagnetic energy flow
- 12 Measurement of the Stokes parameters
- 13 Description of far-field scattering in terms of actual optical observables
- 14 Electromagnetic scattering by a small random group of sparsely distributed particles
- 15 Statistically isotropic and mirror-symmetric random particles
- 16 Numerical computations and laboratory measurements of electromagnetic scattering
- 17 Far-field observables: qualitative and quantitative traits
- 18 Electromagnetic scattering by discrete random media: far field
- 19 Near-field scattering by a sparse discrete random medium: microphysical radiative transfer theory
- 20 Radiative transfer in plane-parallel particulate media
- 21 Weak localization
- 22 Epilogue
- Appendix A Dyads and dyadics
- Appendix B Free-space dyadic Green's function
- Appendix C Euler rotation angles
- Appendix D Spherical-wave decomposition of a plane wave in the far zone
- Appendix E Integration quadrature formulas
- Appendix F Wigner d-functions
- Appendix G Stationary phase evaluation of a double integral
- Appendix H Hints and answers to selected problems
- References
- Index
- Plate Section
Summary
Measurements of electromagnetic energy flow are an integral part of solving various energy-budget and optical-characterization problems. For example, the physical state of a cloud of water droplets or ice crystals in the terrestrial atmosphere can be affected by an imbalance between the incoming and outgoing electromagnetic energy, while measurements of specific manifestations of electromagnetic energy flow with a suitable device can potentially be analyzed to infer useful information about the cloud. Conceptually similar problems are encountered in many other areas of science and engineering. It is therefore very important to understand clearly what specific measurement is afforded by an optical instrument and how to model this measurement theoretically.
Let us recall, for example, the energy-budget problem for a macroscopic volume element of an idealized liquid-water cloud discussed in Section 1.4. Suppose that we have at our disposal a Poynting-meter, i.e., a device that can determine both the direction and the absolute value of the time-averaged local Poynting vector. Then measuring ≪S(r,t≫ at a sufficiently representative number of points densely distributed over the boundary ΔS would enable one to evaluate the integral in Eq. (1.12) numerically and thereby quantify the degree of electromagnetic energy imbalance of the volume element ΔV.
Unfortunately, none of the existing photometers can, strictly speaking, be considered a Poynting-meter.
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- Electromagnetic Scattering by Particles and Particle GroupsAn Introduction, pp. 111 - 130Publisher: Cambridge University PressPrint publication year: 2014