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Remote Sensing Satellite Characteristics: Remote
sensing instruments can be placed on a variety of platforms to view and image
targets on the earth’s surface. Although ground-based and aircraft platforms
may also be used, satellites provide a great deal of the remote sensing
imagery commonly used today. Satellites have several unique characteristics
which make them particularly useful for remote sensing of the Earth's
surface. Satellite Orbits The path followed by a
satellite is referred to as its orbit. Satellite orbits are matched to
the objectives of the mission and the capability of sensor(s) they carry.
Orbit selection can vary in terms of: 1. Altitude
(their height above the Earth's surface) 2. Orientation (relative
to earth’s equatorial plane) 3. Rotation
relative to the Earth. Satellites at very high
altitudes, which view the same portion of the Earth's surface at all times
have geostationary orbits. These geostationary satellites revolve at
speeds which match the rotation of the Earth so they seem stationary,
relative to the Earth's surface. This allows the satellites to observe and
collect information continuously over specific areas. Altitudes of geoststionary orbits are at 35,786 kilometres
(radius: 42,164
km). At this altitude satellites are required to move at a velocity of 11,300
km/h. Weather and communications satellites commonly have these types of
orbits. Due to their high altitude, some geostationary weather satellites can
monitor weather and cloud patterns covering an entire hemisphere of the
Earth. Understandably, thousands of satellites share this orbit.
Many remote sensing platforms are designed to follow an
orbit (basically north-south) which, in conjunction with the Earth's rotation
(west to east), allows them to cover most of the Earth's surface over a
certain period of time. These are near-polar orbits, so named for the
inclination of the orbit relative to a line running between the North and
South poles. Many of these satellite orbits are also sun-synchronous
such that they cover each area of the world at a constant local time of day
called local sun time. At any given latitude, the position of the sun
in the sky as the satellite passes overhead will be the same within the same
season. This ensures consistent illumination conditions when acquiring images
in a specific season over successive years, or over a particular area over a
series of days. This is an important factor for monitoring changes between
images or for mosaicking adjacent images together, as they do not have to be
corrected for different illumination conditions.
Most of the remote sensing satellite platforms
today are in near-polar orbits, which means that the satellite travels northwards
on one side of the Earth and then southwards on the second half of its orbit.
These are called ascending and descending passes, respectively. If the orbit
is also sun-synchronous, the ascending pass is most likely on the shadowed
side of the Earth while the descending pass is on the sunlit side. Sensors recording reflected
solar energy only image the surface on a descending pass, when solar
illumination is available. Active sensors which provide their own
illumination or passive sensors that record emitted (e.g. thermal) radiation
can also image the surface on ascending passes.
Swaths As a satellite revolves
around the Earth, the sensor "sees" a certain portion of the
Earth's surface. The width of the imaged area on the surface,
is referred to as the swath. Imaging swaths for spaceborne
sensors generally vary between tens and hundreds of kilometres
wide. As the satellite orbits the Earth from pole to pole, its east-west
position wouldn't change if the Earth didn't rotate. However, as seen from
the Earth, it seems that the satellite is shifting westward because the Earth
is moving eastwards beneath it. This apparent movement allows the satellite
swath to cover a new area with each consecutive pass. The satellite's
orbit and the rotation of the Earth work together to allow complete coverage
of the Earth's surface, after it has completed one complete cycle of orbits. If we start with a randomly selected pass in a satellite's orbit, an orbit cycle will be completed when the satellite retraces its path, passing over the same point on the Earth's surface directly below the satellite (called the nadir point) for a second time. The exact length of time of the orbital cycle will vary with the altitude of each satellite. The interval of time required for the satellite to complete its orbit cycle is not the same as the "revisit period". Using steerable sensors, a satellite-borne instrument can view an area (off-nadir) before and after the orbit passes over a target, thus making the 'revisit' time less than the orbit cycle time. The revisit period is an important consideration for a number of monitoring applications, especially when frequent imaging is required (for example, to monitor the spread of an oil spill, or the extent of flooding). In near-polar orbits, areas at high latitudes will be imaged more frequently than the equatorial zone due to the increasing overlap in adjacent swaths as the orbit paths come closer together near the poles. |
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S. Farooq
Department of Geology
Aligarh Muslim University, Aligarh - 202 002 (India)
Phone: 91-571-2721150
email: farooq.amu@gmail.com