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Remote Sensing

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Remote Sensing
Introduction to Remote

Sensing





Orbital Considerations

Orbital Characteristics (1)

Orbital Considerations (2)

Height vs. Life of Satellite









10,000 km orbit is permanent

Orbital Characteristics (3)

Low Earth Orbits (LEO;

<2500km)





Equatorial Orbit

(Not very useful)

International Space Station Orbit









The station travels from west to east on an orbital inclination of 51.6°. Each orbit takes

90-93 minutes, depending on the altitude of the ISS. During that time, part of the Earth is

viewed under darkness and part under daylight. The ISS orbital altitude drops gradually

over time due to the Earth's gravitational pull and atmospheric drag. Periodic reboosts

adjust the ISS orbit. The orbit of the Space Shuttle is very similar.

http://city.jsc.nasa.gov/orbtutor/page1.htm

International Space Station Orbit









The inclination of orbits of natural or artificial satellites is measured relative to the equatorial plane

of the body they orbit if they do so close enough. The equatorial plane is the plane perpendicular to

the axis of rotation of the central body.

an inclination of 0 degrees means the orbiting body orbits the planet in its equatorial plane, in the same direction as the planet

rotates;

an inclination of 90 degrees indicates a polar orbit, in which the spacecraft passes over the north and south poles of the planet; and

an inclination of 180 degrees indicates a retrograde equatorial orbit.

Orbital Characteristics (4)

Low Earth Orbits (LEO; <2500km)

2. Polar Orbits

-Orbit in plane of Earth’s rotation

axis

-Successive orbits cross the

equator at different times

-Preferred for missions intended to

view longitudinal zones under full

range of illumination conditions

-Nodes:

Nodes mark the intersection of the

plane of the equator and the plane of

the orbit.

N-flying =

ascending node

S-flying =

descending node

Orbital Characteristics (5)

Low Earth Orbits (LEO; <2500km)









3. Oblique Orbits (orbital plane intersects equator not at 90°)

-Most satellites in LEO use near-polar oblique

-Launched eastward = direction of Earth’s rotation = Prograde orbit

-Launched westward = opposite direction of Earth’s rotation = Retrograde orbit

Cape Canaveral Spaceport









Required for safety reasons to launch over water (eastward). All

orbits launched from here are prograde.

NASA Space Shuttle

• Altitude 200-600 km

• Inclinations: Max 62°, usually ~28° (latitude

of Cape Canaveral)

• Always in a Prograde Oblique orbit.

Vandenberg Air Force Base









Required for safety reasons to launch over water (westward). All

orbits launched from here are retrograde.

Orbital Characteristics (6):

Oblique Orbits

Orbital Characteristics (7):

Oblique Orbits









16

Landsat 7

Orbital

Characteristics

Landsat Paths on Consecutive Orbits

Spacing Between Consecutive

Landsat Orbits at Equator

Complete Landsat coverage

takes 15 days

251paths/14 orbits per day = ~18 days for repeat coverage

233 paths/ 14.5 orbits per day = ~15 days for repeat coverage

Eccentricity





The eccentricity of a satellite's orbit is defined as the ratio of the satellite orbit's

focus length (c) to the orbit's semi-major axis (average orbit radius) (a). It defines

how elliptical the orbit is, and defines the orbit height at both the apogee and

perigee points.



The eccentricity of a satellite's orbit (or any orbit for that matter) is a unitless

value that ranges from 0 (perfectly circular) to 1 (parabolic). All of Earth's

artificial satellites have orbit eccentricities of between 0 and 1. Within a TLE

(Two Line Element) file, the decimal point is not present, but is always assumed

to be placed before the first number, even if it is a zero.

Aqua and Terra Satellites



• Aqua (EOS-PM) Orbit •Terra (EOS-AM) Orbit

Characteristics Characteristics

• Sun synchronous, near- •Sun synchronous, near-polar

polar orbit

orbit

• Equatorial Crossing Time

•Equatorial Crossing Time

– 1:30 p.m., ascending -10:30 a.m., ascending node

node •Inclination 98°

• Inclination 98° •Altitude: 705 km

• Altitude: 705 km •Period: 99 minutes

• Period: 99 minutes •Semi-major axis 7085 km

• Semi-major axis 7085 km

•Eccentricity 0.0015

• Eccentricity 0.0015

SPOT has better repeat

coverage because it can look

off-nadir

SPOT Viewing Opportunities

High-level Satellites:

Geosynchronous Orbits

Geostationary Satellites

• That orbit is achieved when the spacecraft is "parked" above the Earth

at 35,800 km (22,300 miles) and is moving along a circular path around

the planet at approximately 11052 km/hr (6802 mph). A point on the

Equator that remains directly underneath is traveling at ~1667 km/hr or

1042 mph. At these speeds there is no relative motion differences, so

that the observing satellite is synchronously locked into a geostationary

position above the hemisphere it is intended to view and (unless it

drifts) will always view the same scene.



• Most imagery shown on TV news weather segments comes from these

satellites. GOES-1 arrived in a geostationary orbit at 135° W, soon after

its launch on October 16, 1975. Others launched at two to three year

intervals (GOES-10 entered its orbit on April 25, 1997,).

To exemplify GOES imagery, we show the the first test IR

image from GOES-9 on June 19, 1995 (left). Such

hemispherical images can be subdivided to concentrate on

specific areas. The GOES-8 (East) images shows a large

continental storm on March 20, 1994.

• Satellite covering the Atlantic Ocean and the eastern U.S. is called

GOES-East (located above the equator at 75°W longitude), and that

over the Pacific is GOES-West (at 135°W longitude). Together, they

provide coverage of both the Atlantic and Pacific, as shown in this

drawing which also illustrates the full disk nature of the view:









To cover the entire Earth, four GOES would be needed. However, other parts of

the world are monitored by other systems. As of late 2006, GOES-11 and GOES-

12 are operating, with GOES-9 and GOES-10 also in orbit serving as back-up.

• The GOES-8 sounder has a visible band and 18 thermal bands, which

are sensitive to temperature variations related to CO2, ozone, and

water vapor at different atmospheric levels. We can convert each band

into an image, to which we assign colors, to identify thermal differences,

as demonstrated in this panel of images taken on May 5, 1997.


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