SST-Sea
temperature
Satellit observations
Satellit observations of SST
At the time of
writing, several satellites are in orbit carrying instruments that
observe SST.
Most of these observations are being collected by the Satellite Eye
project and
are combined to daily high-resolution images of satellite sea surface
temperature (SST). The spatial resolution and the temporal resolution
from the
satellite observations vary among instruments.
In
the table below, an overview of the major
sources of satellite SST is given. Please note that observations from
TMI and
SEVIRI only can be used for the regions between latitude 40 degrees
south and
40 degrees north.
Instrument
|
Satellite
|
Spatial
resolution
|
Temporal
resolution
|
Observing
techniques
|
Expected
error, in std. dev. i C
|
AATSR
|
ENVISAT
|
1 km
|
~1 time
each 2-3 days
|
IR
|
0.3
|
AVHRR
|
NOAA
polar orbit
|
2 km
|
twice
daily
|
IR
|
0.5
|
AMSR-E
|
Aqua
|
25
km
|
Daily
|
MB
|
0.7
|
TMI
|
TRMM
|
25
km
|
Twice
daily
|
MB
|
0.7
|
MODIS
|
Aqua
|
2 km
|
Daily
|
IR
|
0.7
|
SEVIRI
|
Meteosat-8
|
5 km
|
Every hour
|
IR
|
0.8
|
Table 1: Overview of the sources
for high-resolution satellite SST observations is listed. IR is
infrared and MB
is microwave.
The data are collected by use of
the Sea and Sea-ice SAF (Satellite Application Facility) belonging to
EUMETSAT
(Satellite operator for the European Meteorological Institute).
As the infrared observations are
limited by cloud cover and the microwave observations are of rather low
spatial
resolution, an interpolation scheme for the data has been applied in
order to
obtain high-resolution SST maps without gaps.
Observations listed in the table
therefore have been collected by DMI and a method called objective
analysis has
been applied. This method uses statistics to fill out gaps and provide
and
interpolated SST map each data with a spatial resolution at around 5
km.
The infrared radiation and the microwave radiation originates from the
upper
millimeter or less of the sea surface, but the sea surface temperatures
presented are corrected such that they represent the temperature of the
upper
one meter. This has been done by inter-comparing vast amounts of
observations
from ships with satellite observations.
Two maps of satellite SST are
shown from 24 February 2007. The first map covers the Indian Ocean. It is clear that the ocean is
warm near the Equator and cool near Antarctica. The other map covers the ocean along
the west coast
of South
America.
It can be noted that the ocean is rather cool along the coastline
compared to
further offshore. The cool water stems from upwelling of cold water
from the
bottom to the surface layer. The Galathea 3 expedition is doing
investigations
in the cool water masses. The upwelling is associated with input of
nutrients
from the bottom to the ocean surface layer that feed phytoplankton and
the rest
of the marine food web (fishes etc.).
Animations of satellite SST can
be viewed in Google Earth from http://galathea.oersted.dtu.dk/GE_animation.html
and regionally at http://galathea.oersted.dtu.dk/SST_e.html
|