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Sea state effect on the sea surface emissivity at L-band

Abstract

In May 1999, the European Space Agency (ESA) selected the Earth Explorer Opportunity Soil Moisture and Ocean Salinity (SMOS) mission to obtain global and frequent soil moisture and ocean salinity maps. SMOS' single payload is the Microwave Imaging Radiometer by Aperture Synthesis (MIRAS), an L-band two-dimensional aperture synthesis radiometer with multiangular observation capabilities. At L-band, the brightness temperature sensitivity to the sea surface salinity (SSS) is low, approximately 0.5 K/psu at 20/spl deg/C, decreasing to 0.25 K/psu at 0/spl deg/C, comparable to that to the wind speed /spl sim/0.2 K/(m/s) at nadir. However, at a given time, the sea state does not depend only on local winds, but on the local wind history and the presence of waves traveling from far distances. The Wind and Salinity Experiment (WISE) 2000 and 2001 campaigns were sponsored by ESA to determine the impact of oceanographic and atmospheric variables on the L-band brightness temperature at vertical and horizontal polarizations. This paper presents the results of the analysis of three nonstationary sea state conditions: growing and decreasing sea, and the presence of swell. Measured sea surface spectra are compared with the theoretical ones, computed using the instantaneous wind speed. Differences can be minimized using an "effective wind speed" that makes the theoretical spectrum best match the measured one. The impact on the predicted brightness temperatures is then assessed using the small slope approximation/small perturbation method (SSA/SPM).

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Sea state effect on the sea surface emissivity at L-band

Author: Miranda, J.,Vall-Llossera Ferran, Mercedes Magdalena,Camps Carmona, Adriano José,Duffo Ubeda, Núria,Corbella Sanahuja, Ignasi,Etcheto, Jacqueline
Publisher: IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
Year: 2003
Source: https://upcommons.upc.edu/bitstream/2117/2130/4/sea%20state%20effect01237392.pdf
IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, VOL. 41, NO. 10, OCTOBER 2003 2307
Sea S a e E ec on he Sea Su ace
Emissi i y a L-Band
Jo ge José Mi anda, Me cè Vall-llosse a, Membe , IEEE, Ad iano Camps, Senio Membe , IEEE,
Nú ia Du o, Membe , IEEE, Ignasi Co bella, Membe , IEEE, and Jacqueline E che o
Abs ac —In May 1999, he Eu opean Space Agency (ESA)
selec ed he Ea h Explo e Oppo uni y Soil Mois u e and
Ocean Salini y (SMOS) mission o ob ain global and equen soil
mois u e and ocean salini y maps. SMOS single payload is he
Mic owa e Imaging Radiome e by Ape u e Syn hesis (MIRAS),
an L-band wo-dimensional ape u e syn hesis adiome e wi h
mul iangula obse a ion capabili ies. A L-band, he b igh ness
empe a u e sensi i i y o he sea su ace salini y (SSS) is low,
app oxima ely 0.5 K/psu a 20 C, dec easing o 0.25 K/psu a
0C, compa able o ha o he wind speed 0.2 K/(m/s) a
nadi . Howe e , a a gi en ime, he sea s a e does no depend only
on local winds, bu on he local wind his o y and he p esence
o wa es a eling om a dis ances. The Wnd and Salini y
Expe imen (WISE) 2000 and 2001 campaigns we e sponso ed by
ESA o de e mine he impac o oceanog aphic and a mosphe ic
a iables on he L-band b igh ness empe a u e a e ical and
ho izon al pola iza ions. This pape p esen s he esul s o he
analysis o h ee nons a iona y sea s a e condi ions: g owing and
dec easing sea, and he p esence o swell. Measu ed sea su ace
spec a a e compa ed wi h he heo e ical ones, compu ed using
he ins an aneous wind speed. Di e ences can be minimized using
an “e ec i e wind speed” ha makes he heo e ical spec um
bes ma ch he measu ed one. The impac on he p edic ed
b igh ness empe a u es is hen assessed using he small slope
app oxima ion/small pe u ba ion me hod (SSA/SPM).
Index Te ms—Nons a iona y sea condi ions, sea su ace emis-
si i y a L-band, sea su ace spec um, swell e ec .
I. INTRODUCTION
KNOWLEDGE o he dis ibu ion o sal in he ocean
and i s annual and in e annual a iabili y a e c ucial
in unde s anding he ole o he ocean in he clima e sys em.
The measu emen o he sea su ace salini y (SSS) is one
o he challenges o he Eu opean Space Agency’s (ESA)
Soil Mois u e and Ocean Salini y (SMOS) Ea h Explo e
Oppo uni y mission. SMOS single payload is he Mic owa e
Imaging Radiome e by Ape u e Syn hesis (MIRAS), a
wo-dimensional (2-D) L-band syn he ic ape u e adiome e
wi h ull-pola ime ic capabili y. Two-dimensional b igh ness
Manusc ip ecei ed Oc obe 14, 2002; e ised June 30, 2003. This wo k was
suppo ed by he Spanish Comisión In e minis e ial de Ciencia y Tecnología
(CICYT TIC99-1050-C03-01) and by G an “Dis inció de Rece ca de la Gen-
e ali a de Ca alunya,” esolu ion: UNI/2120/2002 on July 19 h, DOGC 3684,
24/07/2002. The WISE 2000 and 2001 ield campaigns ha e been sponso ed by
he Eu opean Space Agency unde ESTEC con ac 14188/00/NL/DC.
J. J. Mi anda, M. Vall-llosse a, A. Camps, N. Du o, and I. Co bella a e
wi h he Technical Uni e si y o Ca alonia (UPC), E-08034, Ba celona, Spain
(e-mail: [email p o ec ed]).
J. E che o is wi h Labo a oi e d’Océanog aphie Dynamique e Clima ologie
(LODYC), UPMC, F-75252 Pa is Cedex 05, F ance.
Digi al Objec Iden i ie 10.1109/TGRS.2003.817190
empe a u e images will p o ide looks o he same pixel unde
incidence angles om 0 o almos 65 , which equi es he
de elopmen o soil and sea emission models in he whole
ange o incidence angles, and sui able geophysical pa ame e s
e ie al algo i hms.
The dielec ic pe mi i i y o seawa e is de e mined, among
o he a iables, by salini y. The e o e, in p inciple, i is possible
o e ie e SSS om passi e mic owa e measu emen s as long
as he a iables in luencing he b igh ness empe a u e (TB)
signal (sea su ace empe a u e, oughness, and oam) can be
accoun ed o a di e en iewing angles, pola iza ions, and e-
quencies. The sensi i i y o TB o SSS is maximum a low mi-
c owa e equencies, and good condi ions o salini y e ie al
a e ound a L-band (1.4 GHz). Howe e , e en a his equency,
he sensi i i y o TB o SSS is s ill low ( 0.5 K/psu o a sea
su ace empe a u e SST 20 C, dec easing o 0.25 K/psu
o SST 0 C), which is compa able o ha o he wind speed
(0.2 K/(m/s) a nadi ). Consequen ly, i places demanding e-
qui emen s on bo h he pe o mance o he ins umen , and he
geophysical modeling o he sea su ace and i s emissi i y.
The SSS e ie al algo i hms o he SMOS mission mus
hen include: 1) he a ia ion o he local incidence angle, as a
pixel appea s in consecu i e snap-sho s, and e en ually 2) he
azimu hal a ia ion o he sea emissi i y o sea emission az-
imu hal signa u e. These wo poin s equi e an accu a e mod-
eling o he sea su ace emissi i y a L-band. Howe e , un il
ecen ly, expe imen al da a we e e y sca ce. The main goal
o he ESA-sponso ed Wind and Salini y Expe imen (WISE)
2000 and 2001 campaigns was o de e mine he TB sensi i i y
o wind speed (o sea s a e) [1], [2]. The campaigns ook place
a Repsol’s Casablanca oil ig,loca ed a 40 43.02 N 21.50 E,
40 km away om he Eb o Ri e mou h on he coas o Ta -
agona, Spain. The sea bed is 165 m, and he sea condi ions a e
ep esen a i eo heMedi e aneanshel /slope egionwi hpe i-
odic in luence o he Eb o Ri e esh wa e plume. WISE 2000
da a acquisi ion spanned om No embe 25 o Decembe 18,
2000 and om Janua y 8 o Janua y 15, 2001, and WISE 2001
om Oc obe 23 o No embe 22, 2001.
I is known ha he wind is he majo dis u bing o ce o he
sea su ace [3]. In WISE 2000 and 2001, pa o he disc epan-
cies be ween he b igh ness empe a u e da a and he b igh ness
empe a u e compu ed using ins an aneous local wind speed a e
a ibu ed owa e e lec ionsin heoil igs uc u e, hep esence
o wa es o igina ed by winds ha ha e blown a away, and sea
s a e condi ions di e en om hose o ully de eloped sea [4].
In Sec ion II, a desc ip ion o some sea su ace oughness
models and he in ol ed pa ame e s a e p esen ed. Then, in
0196-2892/03$17.00 © 2003 IEEE
2308 IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, VOL. 41, NO. 10, OCTOBER 2003
Fig. 1. Dependence o he uni ied omnidi ec ional spec um wi h he in e se-wa e-age ( he used alues o

a e 0.84, 1, 2, 3, 4, and 5). Wind speed is 15 m/s.
Sec ion III, he mos ep esen a i e clima ologic condi ions
occu ed du ing WISE campaigns a e analyzed. In ac , we
p esen an in e compa ison o measu ed spec a in WISE
campaigns wi h he ones compu ed by models when he
simul aneously measu ed wind speed is applied. Finally,
he di e ence be ween he b igh ness empe a u es o bo h
spec a (measu ed and heo e ical depending only wi h he
ins an aneous wind speed) is ob ained. I is demons a ed ha
his di e ence is compa able o he b igh ness empe a u e SSS
signa u e. The e o e, in o de o achie e he equi ed accu acy
in SSS e ie al, i is necessa y o know he ac ual sea s a e
condi ions and no only he ins an aneous wind speed.
II. MODELING THE SEA STATE
The s a is ical desc ip ion o he sea su ace is ep esen ed by
i s di ec ional spec um , de ined as he Fou ie ans-
o m o he au oco ela ion unc ion o he su ace heigh . Sea
s a e e ol es bo h in ime and space. The e olu ion o spec al
sea su ace componen s a wa enumbe , a eling in he di-
ec ion, along a dis ance , du ing a ime , ollows he ene gy
balance o anspo equa ion o deep-wa e [5]
(1)
whe e is he g oup speed. The igh -hand side o (1) adds he
wind ene gy inpu ( ), he dissipa ion ( ), and he ans e -
ence o ene gy among equency componen s due o nonlinea
in e ac ions ( ) [6].
Due o ic ional d ag in he ai –su ace in e ace, i s sho
capilla y wa es a ede eloped. Pa o he capilla y wa e ene gy
is hen ans e ed o longe wa eleng h g a i y wa es, and as
ime elapses he wa eleng h associa ed o he spec al peak and
o al ene gy inc ease. This p ocess con inues un il an equilib-
ium s a e, in which he inpu wind ene gy balances he ene gy
dissipa ion, is eached. In his s a e, he sea is said o be ully
de eloped. The ime necessa y o de elop g a i y wa es is hen
highe han ha o de elop capilla y wa es. When wind s ops,
sho wa es disappea apidly, while long wa es ake longe and
may las o se e al days, which allows hem o p opaga e o e
long dis ances and add o locally gene a ed wa es. This phe-
nomenon is usually known as swell, and i is conside ed o con-
ain wa e-pe iods highe han 10 s, app oxima ely [7].
Thedi ec ional spec um [(1)]is di idedin o heom-
nidi ec ional spec um and he angula sp eading unc ion
[(2)]
(2)
The sp eading unc ion, which is e en and eal, can be decom-
posed by a Fou ie se ies expansion
(3)
and i is usually app oxima ed wi h he wo i s e ms [8]
(4)
Many sea oughness spec um models ha e been de eloped.
A comp ehensi e desc ip ion o hem is p esen ed in [8]. How-
e e , mos o hem assume ully de eloped sea s a e condi ions,
a si ua ion ha equi es ha he wind blows a cons an speed
and di ec ion du ing a gi en ime and dis ance. Fully de eloped
sea spec a depend only on he wind measu ed a a e e ence
heigh . In his wo k, we use he wind speed measu ed a 10 m
(). The dis ance ha a cons an wind ec o co e s is called
e ch ( , in me e s), and i s dimensionless alue is ,
whe e is he wa enumbe , de ined as [9]. As
he wind speed inc eases, bo h e ch and wind ac ion ime mus
MIRANDA e al.: SEA STATE EFFECT ON THE SEA SURFACE EMISSIVITY AT L-BAND 2309
(a)
(b) (c)
Fig. 2. G owing sea case. (a) Wind speed e e ed o 10-m heigh du ing 24 h be o e he nominal measu emen ime. (b) Buoy-measu ed spec um (solid line),
uni ied spec um compu ed wi h he equi alen wind speed
U
=
6.77 m/s (do ed line), and uni ied spec um compu ed wi h he 3-h a e aged wind speed
measu ed a 10-m heigh
U
=
7.73 m/s (dashed line). (c) Di e ence o b igh ness empe a u e a e ical (do ed line) and ho izon al (dashed line) pola iza ions
compu ed wi h he SSA/SPM me hod using he heo e ical uni ied spec um calcula ed wi h
U
=
6.77 m/s minus he one ob ained wi h he measu ed wind speed
U
=
7.73 m/s. The e o is posi i e o he ho izon al pola iza ion and nega i e o he e ical pola iza ion in acco dance wi h a spec um o e es ima ion.
inc ease o each he condi ions o ully de eloped sea [3]. In
WISE expe imen s, because o he oil ig si ua ion (see he in-
oduc ion), in mos caseswhen he wind blows om hewes o
no hwes , he sea canno be conside ed ully de eloped. Dom-
inan winds in he Casablanca oil ig a e om he no h and
no hwes . Winds om he Sou h a e much a e .
F om he s udy o an ex ensi e da ase o de eloping sea
s a es, Donelan e al. [10] and Dobson [11] ob ained a depen-
dence o he long-wa e spec um wi h he dimensionless in-
e se-wa e-age pa ame e , whe e is he wa e
phase speed a he spec al peak. Taking in o accoun he ela-
ionship be ween he dimensionless ene gy wi h he e ch [12],
El ouhaily [8] de i ed he ollowing e ch o in e se-wa e-age
ela ionship:
(5)
whe e is he angle be ween he wind and he dominan wa es
a hespec alpeakandi s alueisalwaysclose oze o,and hen
. Seas a e said o be ully de eloped, ma u e and young
when has alues closed o 0.84, 1 and 2, espec i ely.
Fig. 1 shows he s ong dependence o he uni ied omnidi ec-
ional spec um, desc ibed in [8] (wind speed equal o 15 m/s)
wi h he in e se-wa e-age ( a ying om 0.84 o 5).
Sec ion III p esen s some plo s o measu ed wind speed and
spec a du ing WISE campaigns, showing ha in mos condi-
ions he sea s a e canno be conside ed ully de eloped. The
impac o sea s a e on he b igh ness empe a u es is e alua ed
using he small slope app oxima ion/small pe u ba ion me hod
(SSA/SPM) model [13], [14]. This model p o ides good ag ee-
men wi h measu ed and i s sensi i i y o wind speed.
III. SEA STATE IN NONSTATIONARY CONDITIONS:IMPACT ON
THE BRIGHTNESS TEMPERATURE AT L-BAND
Du ingWISEcampaignswindspeedsa 2.6- and69-mheigh
we e eco ded and e e ed o 10 m using he ollowing [15]:
cm/s (6)
2310 IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, VOL. 41, NO. 10, OCTOBER 2003
(a)
(b) (c)
Fig. 3. Dec easing sea case. (a) Wind speed e e ed o 10-m heigh du ing 24 h be o e he nominal measu emen ime. (b) Buoy-measu ed spec um (solid
line), uni ied spec um compu ed wi h he equi alen wind speed
U
=
7.45 m/s (do ed line) and uni ied spec um compu ed wi h he 3-h a e aged wind speed
measu ed a 10 m
U
=
5.21 m/s (dashed line). (c) Di e enceo b igh ness empe a u e a e ical (do ed line) and ho izon al (dashed line) pola iza ions compu ed
wi h he SSA/SPM me hod wi h he heo e ical uni ied spec um calcula ed wi h
U
=
7.45 m/s and
U
=
5.21 m/s. The e o is posi i e o he e ical
pola iza ion and nega i e o he ho izon al pola iza ion in acco dance wi h a spec um unde es ima ion.
whe e and a e he wind speed a heigh and he ic ion
speed, espec i ely, and is ob ained om
(7)
Fu he mo e, he sea su ace ele a ion spec a we e simul a-
neously measu ed by a wa e- ide buoy. Du ing 3 h, he buoy
measu es he sea heigh , and hen, i is Fou ie ans o med.
Ne e heless, he measu ed spec a a e de ined wi h only 14
poin s and he accu acy o he nume ical me hod depends on
he numbe o poin s used in he nume ical in eg a ion o hesea
su ace spec um.Hence, he ene gy o each measu ed spec um
has been ob ained, and hen, an equi alen wind speed ( ) has
been es ima ed in o de o compu e a uni ied wind d i en spec-
um wi h he same ene gy as he measu ed one. The com-
pu ed wi h he wind d i en spec um o he equi alen wind
speed ( ), a di e en ep esen a i e momen s du ing WISE
campaigns,we ecompa edwi h he compu edwi h hewind
d i en spec um applying he simul aneously measu ed wind
speed. In ac , in o de o be consis en wi h he 3-h measu e-
men s o he buoy, i has been used he a e age o wind speeds
eco ded du ing he3ho hebuoymeasu emen s ( ). Th ee
e en s a e p esen ed below as examples o h ee eal sea con-
di ions: g owing sea, dec easing sea and sea a ec ed by swell.
None o hei spec a is well cha ac e ized by ully de eloped
models.
The b igh ness empe a u es we e compu ed using he
second-o de SSA/SPM emissi i y model [16]. Johnson and
Zhang ecall a heo e ical de elopmen o his me hod in [13].
In ha pape , he physics o he emission p ocess p edic ed
by SSA/SPM was cla i ied. The use o he SSA/SPM up o
he second-o de ob ains an expansion in su ace slope, wi h
ze o-o de e ms ep oducing la su ace emission esul s,
i s -o de e ms iden ically ze o, and he second-o de e ms
p o iding he i s p edic ion o changes om la su ace
b igh ness. Second-o de e ms ake he o m o an in eg al
o a se o weigh ing unc ions o e he su ace di ec ional
spec um. P ope ies o a di ec ional spec um esul in no i s
ha monic a ia ion being ob ained; a hi d-o de SSA/SPM is
MIRANDA e al.: SEA STATE EFFECT ON THE SEA SURFACE EMISSIVITY AT L-BAND 2311
(a)
(b) (c)
Fig. 4. Swell case. (a) Wind speed e e ed o 10-m heigh du ing 24 h be o e he nominal measu emen ime. (b) Buoy-measu ed spec um (solid line), uni ied
spec um compu ed wi h he 3-h a e aged wind speed measu ed a 10-m heigh
U
=
11.33 m/s (do ed line) and he same spec um plus swell spec um wi h he
pa ame e sshownin hebox(dashedline).(c) Di e enceo b igh ness empe a u e a e ical(do edline)and ho izon al (dashedline)pola iza ionscompu ed wi h
he SSA/SPM me hod wi h he heo e ical uni ied spec um calcula ed wi h he equi alen wind speed and he a e aged measu ed wind speed. The swell inc eases
he oughness. The e o is posi i e o he e ical pola iza ion and nega i e o he ho izon al pola iza ion in acco dance wi h a spec um unde es ima ion.
(a) (b)
Fig. 5. (a) Signi ican wa e heigh (SWH) de ined as H1/3 he a e age o he highes hi d o he wa es [m], and (b) maximum wa e pe iod [s] om Oc obe 15
o No embe 22, 2001.

2312 IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, VOL. 41, NO. 10, OCTOBER 2003
(a) (b)
(c) (d)
(e) ( )
Fig. 6. B igh ness empe a u e di e ence be ween he uni ied heo e ical spec um wi hou swell and wi h swell. (a) and (c) Resul o he ho izon al pola iza ion.
(b) and (d) Resul o he e ical pola iza ion. In (a) and (b), he swell di ec ion ela i e o he wind di ec ion is 0 . In (c) and (d), he swell di ec ion is 45 espec
o he wind di ec ion. Plo (e) compa es he cu s a

=
30 in (a) and (c), and plo ( ) compa es he cu s a

=
30 in (b) and (d). The objec i e o (e) and ( ) is
o show he shi ing in he e o signa u e due o he angle be ween he wind and he swell di ec ions.
MIRANDA e al.: SEA STATE EFFECT ON THE SEA SURFACE EMISSIVITY AT L-BAND 2313
equi ed o ob ain he i s ha monics. Only he second-o de
expansion is conside ed in his s udy. No a i icial cu o
wa enumbe is equi ed o sepa a e small and la ge scale wa es
in his me hod.
A. G owing Sea
Fig. 2 co esponds o measu emen s held on No embe 1,
2001 a 6 A.M. (day o yea 305) and shows an example o a
g owing sea ha has no eached he ully de eloped condi ions.
The wind speed e olu ion du ing he p e ious 24 h is p esen ed
in Fig. 2(a), and shows wo wind speed jumps: he i s one 6 h
be o e he measu emen and he second one only hal an hou .
A la ge disc epancy be ween he measu ed spec um(solid line)
and he uni ied spec um o a ully de eloped sea (do ed line)
compu ed wi h he 3-h a e aged wind speed a 10 m om sea
le el, 7.73 m/s, is obse ed in Fig. 2(b). The measu ed
spec umcouldalsobeapp oxima edusinganin e se-wa e-age
la ge han 0.84 ( ully de eloped sea), which means ha he
sea has no eached ma u i y condi ions. Ne e heless, he dis-
ag eemen is s ill conside able. This is because he heo e ical
g owingspec umis he ansien s a ebe weena la seaand he
ully de eloped sea unde a cons an wind blowing o a qui e
long ime, whe eas heac ual si ua ion is hesum o noncons an
local wind e ec , plus he con ibu ion o he ene gy p opaga ed
om emo e places. An equi alen wind speed 6.27 m/s
has been ob ained. This wind speed has an associa ed uni ied
spec um [dashed line in Fig. 2(b)] wi h he same ene gy as
he measu ed one. Fig. 2(c) shows he di e ence be ween he
b igh ness empe a u es compu ed by SSA/SSPM o he ully
de eloped uni ied spec a wi h (same ene gy han measu e-
men ) and (a e age o 3-h measu ed wind speed). The e o
isnegligiblea nadi ,bu inc easeswi h ele a ionangle eaching
alues a ound 0.1 K and 0.12 K o and , espec i ely.
As compa ed o he salini y b igh ness empe a u e signa u e
(see he in oduc ion), hese alues a e no negligible a all.
B. Dec easing Sea
Fig. 3 co esponds o measu emen s on No embe 4, 2001 a
12 A.M. (day o yea 308) and ep esen s an example o a de-
c easing sea. The wind speed e olu ion du ing he p e ious 24 h
is plo ed in Fig. 3(a). The wind speed ends o dec ease om
20 h be o e he measu emen . Fig. 3(b) shows he measu ed
spec um (solid line), he uni ied spec um o a ully de eloped
sea o he 3-h a e aged wind speed a 10 m 5.21 m/s
(do ed line) and he uni ied spec um o a ully de eloped sea
conside ing he equi alen wind speed 7.45 m/s (dashed
line). As expec ed, he measu ed spec um shows a g ea e con-
ibu ion o he long wa es han he co esponding heo e ical
ully de eloped spec um. In gene al, he ine ia o he long
wa es c ea es a emnan oughness o e he sea su ace, which
p opaga es long dis ances and leads o he appea ance o swell
(example C).
Fig. 3(c) shows he di e ence be ween he b igh ness em-
pe a u es compu ed o he equi alen wind speed ( ) and he
a e aged wind speed ( ). The e o is negligible a nadi bu
inc eases wi h ele a ion angle eaching alues a ound 0.22 and
0.2 o and , espec i ely. This plo shows an opposi e
beha io wi h espec o he one in Fig. 2(c), which p esen s
he b igh ness empe a u e e o o an example o g owing sea.
Now, hee o isposi i e o heho izon alpola iza ionandneg-
a i e o he e ical one. In he p e ious case, he es ima ed
oughness was g ea e han he eal one, while o dec easing
sea he es ima ed oughness is lowe han he eal one. The en-
dency o he b igh ness empe a u e e o is consis en wi h he
emissi i y dependence o he wind, and hence, o he sea su -
ace oughness: an inc emen o he sea oughness p oduces an
inc emen o and a dec emen o .
C. Swell E ec s
The spec um is usually he esul o he local wind gene a ed
oughness and he swell p opaga ed om o he places. Plo s in
Fig. 4 co esponds o measu emen s on No embe 10, 2001 a
9P.M. day o yea 314) and show an example o he swell
e ec on he spec um and i s emissi i y. The wind speed e o-
lu ion du ing he p e ious 24 h is mo e cons an han in he
p e ious wo examples, bu in p e ious days [Fig. 5(a)] in ense
wind blew and signi ican wa e heigh s (de ined as he a e age
o one hi d o he highes wa es) o abou 1.8 m we e s ill
p esen in he a ea [Fig. 5(b)].
Swell spec um can be modeled by a na owband Gaussian
p ocess wi h a 2-D oughness spec um [17] wi h pa ame e s:
swell heigh a iance , di ec ional s anda d de ia ions
and , and swell spec al peak wa e numbe s and ,
in he di ec ions and , espec i ely, which a e no usually
coinciden wi h he up-wind and c oss-wind di ec ions
(8)
Then, he con ibu ion o he swell o he omnidi ec ional
spec um can be ob ained using he ollowing ela ion:
(9)
Fig. 4(b) shows he omnidi ec ional sea su ace spec um
measu ed by he wa e ide buoy (solid line), he uni ied
ully de eloped spec um o 3-h a e aged wind speed
11.33 m/s (dashed line), and his spec um plus a swell
spec um . The swell con ibu ion o he spec um has
been ob ained wi h he ollowing pa ame e s: 0.28 m,
0.011 m , and 0.043 ad/m
(do ed line). These alues ha e been chosen in o de o
minimize he di e ence be ween he measu ed spec um and
he wind-d i en ully de eloped uni ied spec um. I is clea
ha he combined model (do ed line) shows a be e ag eemen
wi h he measu ed spec um han jus he ully de eloped sea
spec um.
Fig. 4(c) shows he di e ence be ween he compu ed b igh -
ness empe a u es a e ical and ho izon al pola iza ions (
and ) when adding he swell e ec o no . As in he p e-
iouscase, he o al oughness(swellandwinde ec s)isg ea e
han he heo e ical one. The e o e, he e o o he e ical po-
la iza ion is posi i e, whe eas i is nega i e o he ho izon al
pola iza ion.
2314 IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, VOL. 41, NO. 10, OCTOBER 2003
Finally, since he swell has a e y di ec ional beha io ,
in Fig. 6 he same di e ence (emissi i y o a sea su ace
oughened by swell and wind and he one oughened only by
wind) is plo ed espec o azimu h angle as well. The azimu hal
signa u e is qui e small and dec eases wi h he ele a ion angle.
Fig. 6(a) and (b) shows he dependence o he e o when he
swell e ec is neglec ed o he e ical and he ho izon al
pola iza ions, espec i ely. In hose plo s he swell and wind
di ec ions a e he same. I he angle be ween he swell and he
wind di ec ions is 45 , his e o is only shi ed [see Fig. 6(c)
and (d)]. In o de o be e app ecia e his shi ing, Fig. 6(e)
and ( ) plo s he 30 cu in hose igu es. A shi o 45
is app ecia ed be ween do ed lines (swell and wind wi h he
same di ec ion) and solid line (45 be ween he swell and he
wind di ec ions).
IV. CONCLUSION
This pape demons a es ha i is impo an o know he ac-
ual sea s a e in he p edic ion o he L-band adiome ic emis-
sion. Fi s o all, ully de eloped wind-d i en uni ied spec a
compu ed wi h he 3-h a e aged measu ed wind a 10 m
ha e been compa ed wi h he measu ed spec a du ing WISE
campaigns, and a g ea disag eemen has been app ecia ed. The
measu ed spec a a e de ined wi h only 14 poin s and he accu-
acy o he emissi i y me hod depends on he numbe o poin s
used in he nume ical in eg al. Hence, he ene gy o each mea-
su ed spec um has been calcula ed, and hen, an equi alen
wind speed a 10 m ( ) has been es ima ed in o de o ob-
ain a ully de eloped wind-d i en uni ied spec um wi h he
same ene gy as he measu ed one. Finally, he di e ence o he
emissi i y using he spec um and he spec um, o
he ho izon al and he e ical pola iza ions has been compu ed
and plo ed wi h espec o he incidence angle. Th ee di e en
si ua ions ha e been analyzed: g owing sea, dec easing sea and
sea a ec ed by swell. In all o hem, he modulus o he di e -
ence ends o inc ease wi h he ele a ion angle. Di e ences o
a ac ion o a kel in a e ound, which a e no negligible when
e ie ing salini y om TB. These di e ences a e in he same
o de o magni ude as he dependence o TB wi h espec o he
sea su ace salini y. In addi ion i has been obse ed ha hese
di e ences ha e opposi e sign o he e ical and he ho izon al
pola iza ions: when he oughness is o e es ima ed is pos-
i i e and is nega i e, whe eas, when he oughness is un-
de es ima ed he beha io is jus he con a y. This is consis en
wi h he emissi i y dependence o he wind speed, and hence o
he sea su ace oughness: i he sea su ace oughness inc eases
he inc easesand he dec eases.The e o e,becauseo his
con a y beha io , his e o can be minimized by using he i s
S okes pa ame e in he SSS e ie al algo i hm [18].
The azimu hal dependence o he b igh ness empe a u e
e o when he swell e ec in he spec um is neglec ed has
also been s udied. This azimu hal dependence is always e y
small and dec eases wi h he ele a ion angle. Azimu h angles
wi h maximum e o a e shi ed, i he angle be ween he wind
and he swell di ec ions changes.
ACKNOWLEDGMENT
The au ho s app ecia e he coope a ion p o ided by he pe -
sonnel o Repsol In es igaciones Pe olí e as-Base Ta agona-
Pla a o ma Casablanca du ing WISE 2000 and 2001 cam-
paigns. The wa e- ide buoy measu emen s we e p o ided by
he Labo a oi e d’Océanog aphie Dynamique e Clima ologie
(LODYC).
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Vall-llosse a, N. Du o, F. To es, R. Villa ino, L. En ique, A. Julià, C.
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Julià, C. Gaba ó, J. Bou in, R. Niclós, P. Wu s eisen, M. Be ge , and M.
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MIRANDA e al.: SEA STATE EFFECT ON THE SEA SURFACE EMISSIVITY AT L-BAND 2315
Jo geJoséMi andawasbo n inLas PalmasdeG an
Cana ia, Cana y Islands, Spain, in 1973. He ecei ed
he Telecommunica ion Technical Enginee ing
deg ee om Las Palmas de G an Cana ia Uni e si y
(ULPGC), Spain, and he Senio Telecommunica ion
Enginee ing deg ee om he Poly echnic Uni e si y
o Ca alonia (UPC), Ba celona, Spain, in 1996 and
2001, espec i ely. He is cu en ly pu suing he
Ph.D. deg ee in elecommunica ion enginee ing
om UPC.
F om 1996 o 1999, he was wi h he Remo e
Sensing and Rada Labo a o y (EUITT-ULPGC), whe e collabo a ed
in sa elli e image p ocessing. In 1999, he joined he Signal Theo y and
Communica ions Depa men , UPC. His Ph.D. hesis is ocused on he sea
su ace emissi i y a L-band. I includes he de elopmen o new models o
de e mining he sea su ace oughness and he compa ison and imp o emen
o exis ing emissi i y models. Since 2002, he has been an Assis an P o esso
a he UPC.
Me cè Vall-llosse a (M’99) ecei ed he Senio Telecommunica ion Enginee
and he Doc o Telecommunica ion Enginee ing deg ees in 1990 and 1994, e-
spec i ely, bo h om he Poly echnicUni e si yo Ca alonia(UPC), Ba celona,
Spain.
Shehas been lec u ing and doing esea cha he Depa men o SignalTheo y
and Communica ions, UPC om 1990 un il 1997 as an Assis an P o esso and
om 1997 un il p esen as an Associa e P o esso . She spen a sabba ical yea
in Mon eal wi h he schola ship o he “P og amme Québécois de Bou ses
d’excellence”(1996-1997):“S agesdeFo ma ionpos doc o aleauQuébecpou
jeunes diplômés é ange s.” He esea ch in e es s include nume ical me hods
in elec omagne ism, mic owa e adiome y, an enna analysis, and design. Cu -
en ly, he esea ch is mainly ela ed o he s udy o nume ical me hods ap-
plied o he sea su ace emissi i y and hei cha ac e iza ion a L-band and he
MIRAS/SMOS p ojec .
D . Vall-llosse a, along wi h he o he membe o he adiome y g oup a
UPC, was awa ded he “P ime P emio Du an Fa ell de In es igación Tec-
nológica” in 2002, and he “P ime P emio Ciu a de Ba celona d’In es igació
Tecnològica” in 2001.
Ad iano Camps (S’91–A’97–M’00–SM’02) was
bo n in Ba celona, Spain, in 1969. He ecei ed he
Telecommunica ions Enginee ing deg ee and he
Ph.D. deg ee in elecommunica ions enginee ing in
1992 and 1996, espec i ely, bo h om he Poly-
echnic Uni e si y o Ca alonia (UPC), Ba celona,
Spain.
F om 1991 o 1992, he was wi h he ENS des Télé-
communica ions de B e agne, B e agne, F ance, wi h
an E asmus Fellowship. In 1993, he joined he Elec-
omagne icsandPho onicsEnginee ingg oup,a he
Depa men o Signal Theo y and Communica ions, UPC, as an Assis an P o-
esso , and since 1997 as an Associa e P o esso . In 1999, he was on sabba ical
lea e a he Mic owa e Remo e Sensing Labo a o y, Uni e si y o Massachu-
se s, Amhe s . His esea ch in e es s a e mic owa e emo e sensing, wi h spe-
cial emphasis in mic owa e adiome y by ape u e syn hesis echniques. He
has pe o med nume ous s udies wi hin he ame o Eu opean Space Agency
SMOS Ea h Explo e Mission. He is an Associa e Edi o o Radio Science.
D . Camps ecei ed he second na ional awa d o uni e si y s udies in
1993, he INDRA awa d o he Spanish Associa ion o Telecommunica ion
Enginee ing o he bes Ph.D. in 1997, he ex ao dina y Ph.D. awa d a he
Uni e si a Poli ècnica de Ca alunya in 1999, he Fi s Du an Fa ell Awa d
and he Ciudad de Ba celona Awa d, in 2000 and 2001, espec i ely, bo h o
Technology T ans e ; and in 2002, he Resea ch Dis inc ion o he Gene ali a
de Ca alunya o con ibu ions o mic owa e passi e emo e sensing. He was
Chai o Cal ’01. He is edi o o he IEEE Geoscience and Remo e Sensing
Newsle e and P esiden -Founde o he IEEE Geoscience and Remo e Sensing
Socie y Chap e a Spain.
Nú ia Du o (S’91–M’99) ecei ed he Telecom-
munica ion Enginee deg ee om he Poly echnic
Uni e si y o Ca alonia (UPC), Ba celona, Spain,
and he Doc o in Telecommunica ion Enginee ing
om UPC, in 1990 and 1996, espec i ely.
Since 1997, she has been an Associa e P o esso
a UPC. He cu en esea ch in e es s a e nume ical
me hods in elec omagne ics, mic owa e adiome y,
an enna analysis, and design.
Ignasi Co bella (M’99) ecei ed he Telecom-
munica ions Enginee ing and Doc o Enginee ing
deg ees, bo h om Uni e si a Poli ècnica de
Ca alunya (UPC), Ba celona, Spain, in 1977 and
1983, espec i ely.
In 1976, he joined he School o Telecommuni-
ca ion Enginee ing in UPC as a Resea ch Assis an
in he Mic owa e Labo a o y, we e he wo ked
on passi e mic owa e in eg a ed ci cui design
and cha ac e iza ion. Du ing 1979, he wo ked
a Thomson-CSF, Pa is, F ance, on mic owa e
oscilla o s design. In 1982, he became an Assis an P o esso a UPC, an
Associa e P o esso in 1986, and a Full P o esso in 1993. He is cu en ly
eaching mic owa es a he unde g adua e le el in UPC and has designed and
augh g adua e cou ses on nonlinea mic owa e ci cui s. Du ing he school
yea 1998–1999, he wo ked a NOAA/En i onmen al Technology Labo a o y,
Boulde , CO, as a Gues Resea che , de eloping me hods o adiome e
calib a ion and da a analysis. His esea ch wo k in he Depa men o Signal
Theo y and Communica ions, UPC includes mic owa e ai bo ne and sa elli e
adiome y and mic owa e sys em design.
Jacqueline E che o was bo n in Meknes, Mo occo,
in 1943. She ecei ed he Ag ega ion de Physique de-
g ee and he Doc eu es Sciences Physiques deg ee
o he hesis in space plasma physics in 1965 and
1972, espec i ely, bo h om he Ecole No male Su-
pe ieu e de Jeunes Filles, Pa is, F ance.
She became a Full-Time Scien is in Cen e Na-
ional de la Reche che Scien i ique in 1965. She is
p esen ly appoin ed o Labo a oi e d’Oceanog aphie
Dynamique e de Clima ologie, Pa is, F ance, as
Di ec eu de Reche ches. F om 1965 o 1987, she has
been wo king on space plasma physics, ocusing on s udies o p opaga ion and
gene a ion o wa es in he magne osphe e. She was esponsible o elaxa ion
sounde s onboa d GEOS1 (ESA, 1977), GEOS2 (ESA, 1978), and ISEE1
(ESA/NASA, 1977), including ins umen de ini ion, p o ision o ha dwa e,
da a handling, and scien i ic use o da a. In 1988, she became in e es ed in
oceanog aphy, using he syne gy be ween emo ely sensed measu emen s and
in si u da a o s udy he ai –sea CO2 exchange a la ge scale. He esea ch
ac i i y is mul iyea es ima ion o ai –sea CO2 lux a egional scale using
bo h sa elli e (wind speed, SST, ocean colo ) and in si u (PCO2 and ela ed
pa ame e s, including launching CARIOCA buoys) da a. Since 1999, she is
in ol ed in he p epa a ion o he SMOS sa elli e (ESA, 2007) in ended a
de e mining sea su ace salini y using L-band adiome y. She is in e es ed in
he de elopmen and alida ion o sea su ace emissi i y models a L-band,
including alida ion campaigns. She is coo dina ing he g oup o F ench
scien is s in ol ed in he ocean pa o he SMOS p ojec . She has published
77 pape s in he open li e a u e.