Asymptotic light field in the presence of a bubble-layer
Flatau, P.J., J. Piskozub, and J.R.V. Zaneveld. Asymptotic light field in the presence of a bubble-layer. Optics Express, 30 Aug. 1999, 5, 120-124, 1999.
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Asymptoticlightfieldinthepresenceofa
bubble-layer
Piotr J. Flatau
Scripps Institution of Oceanography, University of California, San
Diego, La Jolla, California 92093-0221
pflatau@ucsd.edu
Jacek Piskozub
Institute of Oceanology, Polish Academy of Sciences, 81712 Sopot,
Poland
piskozub@iopan.gda.pl
J. Ronald V. Zaneveld
Oregon State University, College of Ocean and Atmospheric Science,
Corvallis, OR 97331
zaneveld@oce.orst.edu
Abstract: Wereportthatthesubmergedmicrobubblesareanefficient
sourceofdiffuseradianceandmaycontributetoarapidtransitionto
thediffuseasymptoticregime.Inthisasymptoticregimeanaverage
cosineiseasilypredictableandmeasurable.
c⃝1999OpticalSocietyofAmerica
OCIS codes: (010.4450)Oceanoptics;(290.4210)MultipleScattering
References and links
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#11948 - $15.00 US Received July 23, 1999; Revised August 26, 1999
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1 Introduction
Theverticalstructureoflightintheseaisimportantinmarinebio-optics.Sunlightis
theenergysourceforthebiologicalfoodchain,andtheamountandspectrumofsolar
energyavailableatagivendepthmustbeknownifaccurateproductivitycalculations
aretobemade.Theverticalstructureofthediffuseattenuationcoefficientinthenear
surfaceregimeisimportantinunderstandingopticalremotesensing.Thebehaviorof
thelightfieldintheseaisdescribedbytheequationofradiativetransfer,whichre-
latesthelightfieldtotheinherentopticalpropertiesofwateranditsconstituents[1].
Oncethisequationissolvedcertainmomentsofthelightfieldcanbederivedandcom-
paredwithmeasurements.Ofparticularinterestistheaveragecosineofirradianceat
depthzwhichisdefinedby ¯µ(z)= E(z)/E
0(z),whereE0(z)isthescalarirradiance
andE(z)isthenet(vector)irradiance,bothwithunitsWm −2.Thedownwellingav-
eragecosineis ¯µd(z)= Ed/E0,where Ed isthedownwellingirradiance.Theaverage
cosine,whichcanvarybetween-1and1,givesdirectionalinformationabouttheradi-
ancedistribution.Theaveragecosineisalsorelatedtothediffuseattenuationcoefficient
K(z)= −1/E(z)dE(z)/dz.Integrationoftheradiativetransferequationoveralldirec-
tionsleadsto dE(z)/dz= −a(z)E
0(z)sothat¯µ(z)= a(z)/K(z),whichisknownas
Gershun’sequation.Wecannowmeasurea(z)and K(z)routinely,sothatitispossible
toverifypredictionsoftheverticaldistributionof¯µonthebasisofobservations.Anum-
berofmodelsoftheverticalstructureoftheaveragecosineofthelightfieldhavebeen
presented[1-4]buttheyhaveallbeenlimitedtohomogeneousmediawithaflatsurface.
Ontheotherhand,usingthedatafromtheGulfofCaliforniaandtheEastCoastshelf
oneofus(JRVZ,unpublished)concludedthattheaveragecosinemodelsdonotfitthe
determinationof ¯µ(z)from K(z)and a(z).Itisspeculatedthatthisdeparturefrom
theoryisduetoverticalinhomogeneitiesintheinherentopticalproperties(IOPs)and
thepossibilitythatthelightfieldinthesurfacelayeroftheoceanmaybemorediffuse
thantheoreticalmodelsassume.Thisdiffuselightfieldmaybeduetohazeandclouds
intheatmosphere,relativelylowsolarzenithangles,surfacewaves,andmicrobubbles
inthesurfacelayer.Acombinationofthesefactorscontributestothelightfieldbeing
quitediffusethroughoutthewatercolumn.Inthisstudywedemonstratethecapacity
ofairbubblestobeanefficientscatterer.
2R e s u l t s
Thereislimitedknowledge[5-7]abouttheradiativetransferpropertiesofbubbleclouds,
theirinherentopticalproperties,andtheirglobalclimatology.Recently,wereported[8]
ontheinfluenceofsubmergedbubblecloudswithinthewaterontheremotesensing
reflectance.Individualbubblecloudspersistforseveralminutesandaregeneratedby
breakingwaves.Thereisevidencethatathighwindspeeds,separatebubbleclouds
nearthesurfacecoalesce,producingastratuslayer[9,10].Themajorityofbubblesin-
jectedintothesurfacelayersofnaturalwatersareunstable,eitherdissolvingdueto
enhancedsurfacetensionandhydrostaticpressuresorrisingtotheair-waterinterface
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Wind Velocity 8 m/s
Bubble Clouds
0m
-6m
-3m
Fig. 1. Bubble-stratus layer generated by breaking waves. Bubble population is
continually replenishedbywave activity (breaking waves atthe surface)leading
eventuallytosemi-homogeneouslayer.
wheretheybreak[11].However,bubbleswithlongresidencetimes,i.e.stablemicrobub-
bleshavebeenobserved[12-14].Oneofthestabilizationmechanisms[15,11]assumes
thatthesurfactantmaterialisanaturaldegradationproductofchlorophyll,presentin
photosynthesizingalgae.
Weconsiderthreesimplesituations:(1)“infinitely”deephomogeneousoceancom-
posedofCDOM,water,andparticulates;(2)“infinitely”deephomogeneousoceancom-
posedofthesameCDOM,water,andparticulatesbutalsowithbubbles;(3)twometer
layerofbubblesand“background”CDOM,water,andparticulates.InFig.1thetwo-
layercaseispresented.(basedon[10]).
Thebackgroundwater,CDOM,andparticulatesarecharacterizedbyabsorption
andscatteringcoefficientsa=0.1801m
−1 andb=1.2525m−1 (thusweincludewater
aandb).Itcorrespondstoachlorophyllconcentrationof10mgm −3 atawavelength
λ=550nm.TheparticulatephasefunctionisthatofPetzoldforturbidwater[7].The
phasefunctionforbubbleswascalculatedbyaveragingfromsizeparameter x=10 −350,
wherex=2πr/λ,risradius.Thesizedistributionfollowsa r−4 law.Aphasefunc-
tionwasderivedusingtheexactmethodforspheresandweassumearefractiveindex
n=3/4.Thescatteringcoefficientforbubblesisassumedtobe b
bubble=0.6181m−1.In
ourrecentpaper[8]wediscussindetailtheclimatologyofbubblelayerdepth,vertical
distribution,anddependenceofdepthonthewindspeed.Assumptionsmadehereare
typicalfor10m /swindsinbubble-stratusregime.Theradiativetransfercalculations
wereperformedusingtheMonte-Carlotechnique[16].Themainresultsofthisnote
arepresentedinFigs.2-3.Fig.2showstheaveragecosineforthedownwellingradia-
tionforthethreecasesdiscussedabove.Inthisfigure“circles”areforthetwo-layer
system.Atfirstthereaisrapiddecreaseinthevalueoftheaveragecosineasinitially
collimatedphotonsareefficientlyscattered.Afterexitingthe“bubble”layerthelightis
alreadydiffuseandonlyasmalladjustmentisneededtoattainanasymptoticregime
forthe“nobubbles”situation.Thisdouble-exponentialtransitionmechanismseemsto
beparticularlyefficientinestablishingthenear-surfacediffuselightfield.Clearly,the
depthofthebubblelayerandtheinherentopticalpropertieswillfurtherdeterminethis
efficiency.Fig3shows¯µ(z),whichcontainscontributionfromtheupwellingradiation
aswell.Theupwellingradiancefieldadjustsgraduallywhenphotonsinteractwiththe
“bubble”layer.Thereispreferentiallossofphotonstravelinginthehorizontaldirection.
Thisleadstomorecollimatedlightandincreasedaveragecosineclosetothesurface.In
reference[8]wediscussinmoredetailtheclimatologyofbubbleclouds,whichstrongly
dependsonwindspeed.Theimportanceofbubblesonanasymptoticlightfielddepends
onwindspeed,windgustiness,andmicrophysicalpropertiesofbubbles.Incomingfield
projectsandlaboratorystudiesshouldgiveacleareranswerontheinfluenceofbubbles
onmarinelightfields. Insummaryweshowthatthesubmergedmicrobubblesarean
efficientsourceofdiffuseradianceand,ifpresent,contributetorapidtransitiontothe
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0.70 0.75 0.80 0.85 0.9
z [m]
0
2
4
6
8
No bubbles
2m bubble layer
Inf. bubble layer
average cosine (down)
Fig. 2. Average cosine for downwelling radiation ¯µd(z) for (1) “infinitely” deep
homogeneousoceancomposedofCDOM,purewater,andparticulatescorrespond-
ingto chl= 10mgm
−3 (triangles); (2) “infinitely” deep homogeneous ocean with
bubbles(cubes);(3)two-layersystemcomposedofbackgroundCDOM,water,and
particulatesand2mlayerofsubmergedbubblesclosetothesurface(circles).
average cosine
0.60 0.65 0.70 0.75 0.80
z [m]
0
2
4
6
No bubbles
2m bubble layer
Inf. bubble layer
Fig.3.Sameas2butfortheaveragecosine¯ µ(z).
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diffuseasymptoticregime.
Acknowledgements
P.J.FlatauwassupportedinpartbytheOfficeofNavalResearchYoungInvestigator
Program.J.PiskozubhasbeensupportedinpartbytheInstituteofOceanologyPAS
andbyOfficeofNavalResearchEuropeVisitingScientistProgram(VSP).J.Ronald
V.ZaneveldacknowledgessupportoftheEnvironmentalOpticsprogramoftheOffice
ofNavalResearchandtheBiogeochemistryprogramofNASA.
(C) 1999 OSA 30 August 1999 / Vol. 5, No. 5 / OPTICS EXPRESS 124
#11948 - $15.00 US Received July 23, 1999; Revised August 26, 1999