ts of sky
2 wind-driv-
ficantiy. If
ight back-
fluctu-
of sea col-
5 Sun^s al-
30 to 40
sun glitter)
> signal is
vides us a
glitter,
il and the
the station
lr experi-
^a measured
al charac-
lard devia-
ace bright-
scover oil
/ gradients,
ı the sea
the water
jended mat-
:s opti-
the open
velling
| be found
find it,
from the
je majority
ton again.
is must have
ind the
me
seas like the
ed into the
on between
lankton is
| from shal-
ight spec-
Kf all the
| whole vis-
of spectral
represents
. Therefore,
lating the
r various
e matters
gations is
rdon et al.
77, 1980),
In the present paper the spectral curves (in the range from
400 to 700 nm) of diffuse reflectance just below the sea surface
depending on the concentrations and vertical profiles of hydrosols,
Chlorophyll and yellow substance in the water are computed. The
total absorption coefficient of the water environment under con-
sideration for the wavelength of incident radiation A is des-
Cribed by the formula:
K (A) = Eu (0) + kn (A) Cu + kc(^)& * ky@)Cy , (1)
where k,"—.spectral absorption coefficient of pure water; KH,kes
ky - spectral absorption coefficients of hydrosol, chlorophyll and
yellow substance, correspondingly; cg , Cc , Cy - concentrations
of the hydrosol, chlorophyll and yellow substance,correspondingly.
Assuming the light scattering caused by water and hydrosols
only, the total scattering coefficient may be described:
DA) = Ou O0) t 6i, (2)
where ©w and 6,4 - the Spectral scattering coefficients of pure
water and hydrosol, correspondingly. :
The numerical values of these spectral absorption and
scattering coefficients are obtained from the investigation by
Plass et al. (1978). The mathematical model based on the well-known
"two-stream approximation" is used (see Arst and Lokk (1981)). The
Sun”s zenith angle is chosen to be 60° and the corresponding
values of the relation between the direct and diffuse solar radia-
tion for clear sky are determined on the basis of the results by
Avagte et al. (1962). The diffuse reflectance (DR) of the sea’ is
computed as a relation between the values of upward and downward
solar irradiance just below the water surface.
The dependence of /C,| , €c, and €, on the depth (z) in
the water is assumed to be described by the formula:
2 -5
€ - e wxpl- pt -25)*] * exp C (0 z*). : (3)
Varying the.parameters e , (f and Có one can obtain
different from each other vertical profiles of c. Fig.l represents
the profiles of c , corresponding to various numerical values of
ol + Bp and Y . Besides, the spectra of DR are computed for
several cH , cce and cy assumed not depending on depth.
The DR spectral curves are presented both in normalized
(to A = 520 nm) and unnormalized form. As our estimations show,
normalized spectra of DR do not depend on the nonselective radia-
tive characteristics (nearly nonselective are the scattering cha-
racteristics of seawater). On the contrary, the absolute values of
the unnormalized DR spectral curves are essentially sensitive to
the scattering and backscattering coefficients of seawater. Hence,
if scattering is the main distinguishing feature for decoding, it
is better to use the absolute spectral values of DR, but if ab-
sorption is presumably the main distinguishing feature the
normalized spectral curves must be preferred. However, it must be
pointed out that in some cases the analyse by collating the
normalized and unnormalized spectral curves of DR may occur very
helpful.
In Fig.2 some results of calculations of the normalized DR
Spectral curves depending on the concentration of optically active
substances in the water are shown. Three main cases of the