Scattering and Polarization

Total Page:16

File Type:pdf, Size:1020Kb

Scattering and Polarization Scattering and Polarization C HAP T E R 13 13.1 these two molecules interferes de­ 1 3.2 INTRODUCTION structively. as in Figure 12.4 (along RAYLEIGH SCATTERING the x-axis). and this Is so for any - sideways direction from which you - So far we have considered what look at the beam. Air. on the other When white light scatters from hap pens when light encounters ma­ hand, is a gas. so there is no guar­ some molecules. it scatters selec­ terial obstacles of a size much antee that there will be another tively because part of the light is ab ­ greater than the wavelength (geo­ molecule half a wavelength beyond sorbed at the resonant frequ encies metrical optics) or of a size so small the first-sometimes there may be a of the molecules-the scattered as to be comparable with the wave­ few extra molecules around one light Is then colored. For man y length of light (wave optics). But point, sometimes a few less. You see other molecules. however, the im­ you can also observe effects due the scattering from these pOints be­ portant resonant frequenCies are to even smaller obstacles, much cause of these fluctuations. (The significantly higher than visible fre­ smaller than the wavelength of visi­ TRY IT suggests ways to enhance quencies. White light nevertheless ble light. When light interacts with the scattering in air.) becomes colored when it scatters an isolated object that small, it Scattering is selective in several from these molecules-the higher shakes all the charges in the object, ways: light of certain wavelengths the frequency of the incident light. which th en radiate in all directions. is scattered more than light of other the more light will be scattered. This phenomenon is called scatter­ wavelengths. and light of one polar­ ThiS type of scattering is called ing. ization (Sec. 1.3B) is scattered Rayleigh scattering and occurs To scatter with appreciable inten­ more than light of another polari­ whenever the scattering particles sity, light must encounter many zation. Because our eyes are not are much smaller than the incident isolated small objects: for example, very sensitive to the polarization of wavelength and have resonances at the m olecules that constitute the light. we have not yet discussed the frequenCies higher than those of air. Indeed, it is onJy because light phenomena associated with it. visible light. Eq.uivalently, we may does scatter in air that you can Scattering provides us with the op­ write the rule for Rayleigh scatter­ see the beams of Figures 1.3, 1.4, portunity to do so, even as it ac­ ing: and 8.19b. Without scattering, the tually prOvides most of the polarized light's path through the air would light around us. Much of this chap­ The shorter the wavelength be invisible and the camera could ter will therefore deal with polarized of the incident light, the not record it. light, produced by scattering as well more light is scattered This simple explanation, offered as by other means. when these figu res were intro­ duced, now bears closer scrutiny. It This result was worked out in detail would seem that when propagating TR Y IT by the same Lord Rayleigh we met in any dense medium, such as in Sections 10.5B and 12.5C. It glass, light should be scattered by FOR SECTION 13.1 says that blue light will be scattered the many molecules that are pres­ Light beams more than red light. In fact, for in­ ent. Instead. as we know. it contin­ cident broad-band white light, the ues to propagate in a sharp beam, To see the path of light rays, you need intenSity of scattered 400-nm light as in vacuum, only with a different tiny objects in the path that will scatter Is almost ten times as great as that part of the light to your eye. To see the speed. This is because there are of 700-nm light. beam of your flashlight, put larger One consequence of Rayleigh scat­ many molecules present in glass, particles in the air, such as dust motes, and wh enever there is one molecule smoke, or chalk dust. In their presence tering is the sky's blue color. Light to scatter light, there will be an­ yo u should be able to trace the light's reaching your eyes from the sky is other one for which the light path path, including reflections from mirrors sunlight that has been scattered by to .your eye is half a wavelength and water surfaces, to test the law ofreflec­ the air molecules (Fig. 13.1 ) and is longer. The scattered light from tion (Sec. 2.4) and Snell's law (Sec. 2.5). therefore predominately blue. Since 347 CHAPTER I3, SCATTERING AND POLARIZATION 3 4 8 the direct rays from the sun have There are a number of other ex­ or sugar, talcum powder, ch alk , the some of the blue part of the spec­ amples where blue coloring is due white spots of moths and butter­ trtim scattered out of them they to Rayleigh scattering. We've al­ flies, white paper, fog, snow, beaten should look slightly yellowish. When ready noted (Sec. 9.9E) that fine egg white, and beer foam all look the sun is overhead, and if the sky black pigment mixed into white white for the same reason. The is very clear, this is a small effect. paint gives it a bluish cast for just white pattern in star rubies and However , if there are lots of tiny this reason. In fact, da Vinci noted sapphires, and in tiger's-eye quartz du st and smoke particles in the air, this and attributed it to the same are Similarly due to scattering from the effect is larger. It becomes even cause that makes the sky blue. The large inclusions. Likewise, the clear larger as the sun sets; the direct writer George MacDonald correctly albumen becomes white as an egg rays from it to your eyes must pass identifies another blue with the is cooked because the protein mol­ through more and more atmo­ blue of the sky when he writes, ecules are freed of their surface wa­ sphere, so these rays are depleted of "Where did you get those eyes so ter and are then able to coagulate more and more of the shorter wave­ blue?IOut of the sky as I came into large clumps, which scatter lengths, and the sun looks redder through." Your beautiful blue eyes nonselectively. When the watery and redder. (See the TRY IT.) are due to scattering from small, whey from milk is made into cheese widely separated particles in your (such as ricottal, the cheese is IrIses. Similarly, the moonstone white because of the same coagula­ owes its blue sheen to Rayleigh tion process. scattering. Yellow lights are often u sed as fog You can see the same effect in lights or headlights on cars because fine smoke, say from a wood fire. yellow is as easily detected by your The smoke looks bluish when illu­ eyes as white but is scattered less in minated from the side and viewed a fine mist, when the droplets are against a dark background, so only very small compared to the wave­ scattered light reaches your eyes. If length of visible light. Un fortu­ instead the smoke is seen against a nately, more often the droplets are bright background, it looks red or larger, and the yellow is then scat­ brown (due to the removal of blue tered as well. by scattering). If the smoke gets too Particles may, of course, also pro­ thick, the particles become dense duce colors by selective absorption enough that all light is repeat­ and r€iflection. The smog we all edly scattered, and the light that know and love takes its brown color emerges sideways is white or gra,y. because of absorption by particles A similar effect can occur when of nitrous oxide, which has reso­ the particles become larger. For ex­ nances at visible frequencies. Not ample, the smoke rising from the all particles in the sky produce ugly end of a Cigarette is bluish, but af­ colors, however. For example, in ter you inhale and exhale it, the 1883 the volcano Krakatoa erupted smoke looks gray or white. Here you spectacularly, spewing micrometer­ have covered the smoke particles size particles into the atmosphere with mOisture, making them much in such abundance that all over the larger. They are then large enough world there were unusually colorful to scatter light of all wavelengths sunrises and sunsets for three equally-as in the reflections of geo­ years! metrical optics-and thus they look Scattering by the air or the parti­ fiGURE 13.1 white. This is also why clouds are cles in it is thus responsible for aer­ white: The water droplets in clouds ial perspective (Sec. 8.6El, wh ich When A looks at point C in the sky, only scattered light from the sun reaches her may be fifty times as large as the makes distant dark hills look blue eyes. As short-wavelength light is wavelength of visible light. With so and distant snow-clad peaks look scattered most, the sky looks blue to many droplets, and thus so many yellow (see Plate 8.4). The purer and her. Direct rays from the sun, from surfaces to reflect the light, the more transparent the air, the bluer which the blue end of the spectrum has been removed by scattering, vary from clouds scatter almost all the light those dark hills.
Recommended publications
  • 12 Light Scattering AQ1
    12 Light Scattering AQ1 Lev T. Perelman CONTENTS 12.1 Introduction ......................................................................................................................... 321 12.2 Basic Principles of Light Scattering ....................................................................................323 12.3 Light Scattering Spectroscopy ............................................................................................325 12.4 Early Cancer Detection with Light Scattering Spectroscopy .............................................326 12.5 Confocal Light Absorption and Scattering Spectroscopic Microscopy ............................. 329 12.6 Light Scattering Spectroscopy of Single Nanoparticles ..................................................... 333 12.7 Conclusions ......................................................................................................................... 335 Acknowledgment ........................................................................................................................... 335 References ...................................................................................................................................... 335 12.1 INTRODUCTION Light scattering in biological tissues originates from the tissue inhomogeneities such as cellular organelles, extracellular matrix, blood vessels, etc. This often translates into unique angular, polari- zation, and spectroscopic features of scattered light emerging from tissue and therefore information about tissue
    [Show full text]
  • Arxiv:2008.11688V1 [Astro-Ph.CO] 26 Aug 2020
    APS/123-QED Cosmology with Rayleigh Scattering of the Cosmic Microwave Background Benjamin Beringue,1 P. Daniel Meerburg,2 Joel Meyers,3 and Nicholas Battaglia4 1DAMTP, Centre for Mathematical Sciences, Wilberforce Road, Cambridge, UK, CB3 0WA 2Van Swinderen Institute for Particle Physics and Gravity, University of Groningen, Nijenborgh 4, 9747 AG Groningen, The Netherlands 3Department of Physics, Southern Methodist University, 3215 Daniel Ave, Dallas, Texas 75275, USA 4Department of Astronomy, Cornell University, Ithaca, New York, USA (Dated: August 27, 2020) The cosmic microwave background (CMB) has been a treasure trove for cosmology. Over the next decade, current and planned CMB experiments are expected to exhaust nearly all primary CMB information. To further constrain cosmological models, there is a great benefit to measuring signals beyond the primary modes. Rayleigh scattering of the CMB is one source of additional cosmological information. It is caused by the additional scattering of CMB photons by neutral species formed during recombination and exhibits a strong and unique frequency scaling ( ν4). We will show that with sufficient sensitivity across frequency channels, the Rayleigh scattering/ signal should not only be detectable but can significantly improve constraining power for cosmological parameters, with limited or no additional modifications to planned experiments. We will provide heuristic explanations for why certain cosmological parameters benefit from measurement of the Rayleigh scattering signal, and confirm these intuitions using the Fisher formalism. In particular, observation of Rayleigh scattering P allows significant improvements on measurements of Neff and mν . PACS numbers: Valid PACS appear here I. INTRODUCTION direction of propagation of the (primary) CMB photons. There are various distinguishable ways that cosmic In the current era of precision cosmology, the Cosmic structures can alter the properties of CMB photons [10].
    [Show full text]
  • Rayleigh Scattering by Gas Molecules: Why Is the Sky Blue?
    Please do not remove this manual from from the lab. It is available via Canvas DEMO NOTES: This manual contains demonstrator notes in blue italics Optics Rayleigh Scattering: 12 hrs Rayleigh scattering by gas molecules: why is the sky blue? Objectives After completing this experiment: • You will be familiar with using a photomultiplier tube) as a means of measuring low intensities of light; • You will have had experience of working safely with a medium power laser producing visible wavelength radiation; • You will have had an opportunity to use the concept of solid angle in connection with scattering experiments; • You will have had the opportunity to experimentally examine the phenomenon of polarization; • You should understand how the scattering of light from molecules varies accord- ing to the direction of polarization of the light and the scattering angle relative to it; • You should have a good understanding of what is meant by cross-section and differential cross section. • You should be able to describe why the daytime sky appears to be blue and why light from the sky is polarized. Note the total time for data-taking in this experiment is about one hour. There are a lot of useful physics concepts to absorb in the background material. You should read the manual bearing in mind that you need to thoroughly understand how you will calculate your results from you measurements BEFORE your final lab session. This is an exercise in time management. Safety A medium power Argon ion laser is used in this experiment. The light from it is potentially dangerous to you and other people in the room.
    [Show full text]
  • A Study on Numerical Integration Methods for Rendering Atmospheric
    Open Phys. 2019; 17:241–249 Research Article Tomasz Gałaj and Adam Wojciechowski A study on numerical integration methods for rendering atmospheric scattering phenomenon https://doi.org/10.1515/phys-2019-0025 In this paper, a qualitative comparison of three, pop- Received Jan 29, 2019; accepted Mar 07, 2019 ular numerical integration methods to compute the sin- gle scattering integral is presented. In provided research, Abstract: A qualitative comparison of three, popular and three methods have been chosen, namely Midpoint, Trape- most widely known numerical integration methods in zoidal and Simpson’s Rules. These three methods are fairly terms of atmospheric single scattering calculations is pre- popular in Computer Graphics field. Atmospheric scatter- sented. A comparison of Midpoint, Trapezoidal and Simp- ing is calculated using backward ray tracing algorithm tak- son’s Rules taking into account quality of a clear sky gener- ing into account variable light conditions [5]. Then, these ated images is performed. Methods that compute the atmo- methods are compared with each other taking into account spheric scattering integrals use Trapezoidal Rule. Authors quality of the generated images of the sky. As a subproduct try to determine which numerical integration method is of this research, the fidelity of the framework presented the best for determining the colors of the sky and check by Bruneton in [3] is being checked. Authors try to deter- if Trapezoidal Rule is in fact the best choice. The research mine which numerical integration method is the best for does not only conduct experiments with Bruneton’s frame- calculating the colors of the sky and check if Trapezoidal work but also checks which of the selected numerical inte- Rule is in fact the best choice.
    [Show full text]
  • An Attempt to Detect Rayleigh Scattering in the Atmospheres of Extrasolar Planets Using a Ground-Based Telescope
    Wesleyan University Blue Skies Through a Blue Sky: An Attempt To Detect Rayleigh Scattering in the Atmospheres of Extrasolar Planets Using a Ground-Based Telescope by Kristen Luchsinger A thesis submitted to the faculty of Wesleyan University in partial fulfillment of the requirements for the Degree of Master of Arts in Astronomy with a Planetary Science Concentration Middletown, Connecticut April, 2017 Acknowledgements I would like to thank the Astronomy department at Wesleyan University, which has been incredibly supportive during my time here. Both the faculty and the stu- dent community have been both welcoming and encouraging, and always pushed me to learn more than I thought possible. I would especially like to thank Avi Stein and Hannah Fritze, who first made me feel welcome in the department, and Girish Duvurri and Rachel Aranow, who made the department a joyful place to be. They, along with Wilson Cauley, were always willing to talk through any issues I encountered with me, and I am sure I would not have produced nearly as polished a product without their help. I would also like to thank the telescope operators, staff, and fellow observers from the time I spent at Kitt Peak National Observatory. Through their support and friendliness, they turned what could have been an overwhelming and fright- ening experience into a successful and enjoyable first ever solo observing run. I would like to thank my advisor, Seth Redfield, for his constant support and encouragement. Despite leading three undergraduate and one graduate student through four theses on three different topics, Seth kept us all moving forward, usually even with a smile and constant, genuine enthusiasm for the science.
    [Show full text]
  • EMR's Interaction with the Earth & Atmosphere ∝ ∝ ∝
    EMR’s interaction with the earth & atmosphere HANDOUT’s OBJECTIVES: • familiarize student with EMR scattering basics in environment • develop basic principles of radiative transfer in environment • develop Lambert’s law & Schwarzschild equation, plus introduce remote-sensing applications of same Lord Rayleigh & sky blueness “Why is the sky blue?” is a good (and hardly trivial) starting point for studying EMR’s interactions with the earth’s atmosphere and oceans. Water (whether vapor or liquid) is often invoked to explain sky blueness. After all, if ocean water is blue, shouldn’t that explain the sky’s color? Unfortunately, several meters of liquid water are required for water’s blue-green absorption minimum to be visible. If we condensed all atmospheric water vapor into a uniform shell around the earth, the shell would only be a few centimeters thick. Visible scattering by water molecules differs little from that of other atmospheric gases. (At the molecular level, we distinguish between the scattering, or redirecting, of EMR and its absorption, or conversion to other wavelengths (or kinds) of energy.) We retrace the ideas of 19th-century British scientist Lord Rayleigh, who showed that atmospheric molecules themselves are responsible for clear-sky color. Rayleigh Rp reasoned that if a spherical particle’s radius Rp << than that of λlight ( < 0.1, the λlight Rayleigh scattering criterion) its total scattering is ∝ its volume V. So when an EMR wave “illuminates” a molecule, scattering by its atoms is in phase because they are within λlight of each other. Thus the amplitude of the scattered electric field Es ∝ V. Clearly Es also depends on the strength of the incident electric field Ei.
    [Show full text]
  • Lecture 7: Propagation, Dispersion and Scattering
    Satellite Remote Sensing SIO 135/SIO 236 Lecture 7: Propagation, Dispersion and Scattering Helen Amanda Fricker Energy-matter interactions • atmosphere • study region • detector Interactions under consideration • Interaction of EMR with the atmosphere scattering absorption • Interaction of EMR with matter Interaction of EMR with the atmosphere • EMR is attenuated by its passage through the atmosphere via scattering and absorption • Scattering -- differs from reflection in that the direction associated with scattering is unpredictable, whereas the direction of reflection is predictable. • Wavelength dependent • Decreases with increase in radiation wavelength • Three types: Rayleigh, Mie & non selective scattering Atmospheric Layers and Constituents JeJnesnesne n2 020505 Major subdivisions of the atmosphere and the types of molecules and aerosols found in each layer. Atmospheric Scattering Type of scattering is function of: 1) the wavelength of the incident radiant energy, and 2) the size of the gas molecule, dust particle, and/or water vapor droplet encountered. JJeennsseenn 22000055 Rayleigh scattering • Rayleigh scattering is molecular scattering and occurs when the diameter of the molecules and particles are many times smaller than the wavelength of the incident EMR • Primarily caused by air particles i.e. O2 and N2 molecules • All scattering is accomplished through absorption and re-emission of radiation by atoms or molecules in the manner described in the discussion on radiation from atomic structures. It is impossible to predict the direction in which a specific atom or molecule will emit a photon, hence scattering. • The energy required to excite an atom is associated with short- wavelength, high frequency radiation. The amount of scattering is inversely related to the fourth power of the radiation's wavelength (!-4).
    [Show full text]
  • 11. Light Scattering
    11. Light Scattering Coherent vs. incoherent scattering Radiation from an accelerated charge Larmor formula Why the sky is blue Rayleigh scattering Reflected and refracted beams from water droplets Rainbows Coherent vs. Incoherent light scattering Coherent light scattering: scattered wavelets have nonrandom relative phases in the direction of interest. Incoherent light scattering: scattered wavelets have random relative phases in the direction of interest. Example: Randomly spaced scatterers in a plane Incident Incident wave wave Forward scattering is coherent— Off-axis scattering is incoherent even if the scatterers are randomly when the scatterers are randomly arranged in the plane. arranged in the plane. Path lengths are equal. Path lengths are random. Coherent vs. Incoherent Scattering N Incoherent scattering: Total complex amplitude, Aincoh exp(j m ) (paying attention only to the phase m1 of the scattered wavelets) The irradiance: NNN2 2 IAincoh incohexp( j m ) exp( j m ) exp( j n ) mmn111 NN NN exp[jjN (mn )] exp[ ( mn )] mn11mn mn 11 mn m = n mn Coherent scattering: N 2 2 Total complex amplitude, A coh 1 N . Irradiance, I A . So: Icoh N m1 So incoherent scattering is weaker than coherent scattering, but not zero. Incoherent scattering: Reflection from a rough surface A rough surface scatters light into all directions with lots of different phases. As a result, what we see is light reflected from many different directions. We’ll see no glare, and also no reflections. Most of what you see around you is light that has been incoherently scattered. Coherent scattering: Reflection from a smooth surface A smooth surface scatters light all into the same direction, thereby preserving the phase of the incident wave.
    [Show full text]
  • CMB Polarization from Rayleigh Scattering
    Polarization from Rayleigh scattering Blue sky thinking for future CMB observations Previous work: Takahara et al. 91, Yu, et al. astro-ph/0103149 http://en.wikipedia.org/wiki/Rayleigh_scattering Antony Lewis http://cosmologist.info/ Classical dipole scattering 4 2 2 Oscillating dipole 풑 = 푝0 sin(휔푡) 풛 ⇒ radiated power ∝ 휔 푝0 sin 휃 dΩ Thomson Scattering Rayleigh Scattering 푚푒푧 = −푒퐸푧 sin 휔푡 푚푒푧 = −푒퐸푧 sin 휔푡 − 푚푒휔0z −푒2퐸 2 ⇒ 풑 = 푧 sin 휔푡 풛 −푒 퐸푧 2 푚푒휔 ⇒ 풑 = 2 2 sin 휔푡 풛 푚푒(휔 −휔0) (푚nucleus ≫ 푚푒) 푝+ 푒− 푒− Frequency independent Frequency dependent Given by fundamental constants: Depends on natural frequency 휔0 of target 2 8휋 푒2 휔4 휎 ≈ 휎 (휔 ≪ 휔0) 휎푇 = 2 푅 4 푇 3 4휋휖0푚푒푐 휔0 Both dipole scattering: same angular and polarization dependence (Boltzmann equations nearly the same) http://farside.ph.utexas.edu/teaching/em/lectures/node95.html Rayleigh scattering details Early universe ⇒ Neutral hydrogen (+small amount of Helium) After recombination, mainly neutral hydrogen in ground state: (Lee 2005: Non-relativistic quantum calculation, for energies well below Lyman-alpha) 8 휈 ≡ c R ≈ 3.1 × 106GHz eff 9 A 1+푧 휈 4 Only negligible compared to Thomson for 푛 obs ≪ 푛 퐻 3×106GHz 푒 Scattering rate Total cross section ≈ (푅퐻푒 ≈ 0.1) Visibility In principle Rayleigh scattering could do tomography of last scattering and beyond Expected signal as function of frequency Zero order: uniform blackbody not affected by Rayleigh scattering (elastic scattering, photons conserved) 1st order: anisotropies modified, no longer frequency independent May be detectable signal
    [Show full text]
  • Electromagnetic Scattering
    5 Electromagnetic Scattering Scattering is the process by which a particle in the path of an electromagnetic wave continuously removes energy from the incident wave and re-radiates the energy into the total solid angle centred at the particle. We only consider the far field solution for a single homogeneous sphere. The full formal solution called Mie theory is required for a particle that has a similar radius relative to the wavelength of the incident light. This is generally the case for cloud and aerosol particles at visible and near infrared wavelengths. This theory is the basis for describing the rainbow, glory and other atmospheric optical phenomena. When the wavelength of light is large compared to the particle size, Mie theory is well approximated by Rayleigh scattering. In the atmosphere molecules act as Rayleigh scatters — this phenomenon explains why the sky is blue. Scattering properties vary rapidly with wavelength so that broadband approxima- tions are inapplicable. Scattering is always considered as a monochromatic process, and calculations over a bandwidth involve wavelength integration. Variation in scat- tering properties for particle distributions is often slow enough that a single calcula- tion can suffice for a range of wavelengths. 5.1 Rayleigh Scattering 5.1.1 The Hertzian Dipole A Hertzian dipole consists of two small spherical conductors carrying equal and opposite charge q separated by a distance l. A thin wire connects the two spheres as shown in Figure 5.1. An alternating current is set up in the wire such that the charge oscillates at an angular frequency ω i.e.
    [Show full text]
  • 15A.2 1 Dual-Frequency Simulations of Radar Observations of Tornadoes
    15A.2 1 DUAL-FREQUENCY SIMULATIONS OF RADAR OBSERVATIONS OF TORNADOES David J. Bodine1 ;2 ;3 ;,∗ Robert D. Palmer2 ;3 , Takashi Maruyama4 , Caleb J. Fulton3 ;5 , and Boon Leng Cheong3 ;5 1 Advanced Study Program, National Center for Atmospheric Research, Boulder, CO, USA 2 School of Meteorology, University of Oklahoma, Norman, OK, USA 3 Advanced Radar Research Center, University of Oklahoma, Norman, OK, USA 4 Disaster Prevention Research Institute, Kyoto University, Kyoto, Japan 5 School of Electrical and Computer Engineering, University of Oklahoma, Norman, OK, USA 1. INTRODUCTION based on radar reflectivity factor. A limitation to this technique is that the dominant scatterers must be rain Radars measure reflectivity-weighted particle velocities drops or small objects with similar electromagnetic and rather than air velocities, resulting in measurement errors aerodynamic characteristics, otherwise the correction is when Doppler velocities are used to estimate tornado wind underestimated. Polarimetric radar observations frequently speeds. Snow (1984) and Dowell et al. (2005) show that reveal areas of low co-polar cross-correlation coefficient debris is centrifuged outward relative to the air, and the radial (ρHV ) at S (Ryzhkov et al. 2005; Kumjian and Ryzhkov 2008; Bodine et al. 2013), C (Palmer et al. 2011; Schultz et al. difference between air and particle velocities (ur) depends on vortex dynamics and particle characteristics. Moreover, 2012a,b), and X bands (Bluestein et al. 2007; Snyder and Dowell et al. (2005) also showed that the tangential and Bluestein 2014), even in rural areas where perhaps larger vertical velocities of debris are reduced relative to the air scatterers are less common.
    [Show full text]
  • Multiple Rayleigh Scattering of Electromagnetic Waves E
    Multiple Rayleigh Scattering of Electromagnetic Waves E. Amic, J. Luck, Th. Nieuwenhuizen To cite this version: E. Amic, J. Luck, Th. Nieuwenhuizen. Multiple Rayleigh Scattering of Electromagnetic Waves. Journal de Physique I, EDP Sciences, 1997, 7 (3), pp.445-483. 10.1051/jp1:1997170. jpa-00247338 HAL Id: jpa-00247338 https://hal.archives-ouvertes.fr/jpa-00247338 Submitted on 1 Jan 1997 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. (1997) Phys. FFance J. I 7 445-483 1997, 445 MARCH PAGE Multiple Scattering Rayleigh Electromagnetic of Waves Antic J.M. Luck E. (~), Nieuwenhuizen and Th.M. (~i*) (~) Saclay, CEA Physique Thdorique, Service de Cedex, (~) Gif-sur~Yvette 91191 France Laboratorium, Waals-Zeeman Van der Valckenierstraat 65, (~) Amsterdam, XE The Netherlands 1018 (Recei>'ed August 1996) final form 1996, 22 accepted 1996, recei>'ed November in November 19 7 PACS.42.68.Ay Propagation, transmission, attenuation, and radiative transfer propagation, PACS.42.25.Bs ivave absorption transmission and PACS.42.68.Mj Scattering, polarization Multiple scattering polarized electromagnetic diffusive of Abstract. media is in in- waves by vestigated approach theory. of radiative transfer summing ladder This the to amounts means diagrams diffuse reflected for intensity, cyclical transmitted for the the the of or ones or cone backscattering.
    [Show full text]