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Platforms for Remote Sensing – Rees, Ch. 10 David Sandwell, April, 2014

Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

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Page 1: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

Platforms for Remote Sensing – Rees, Ch. 10 David Sandwell, April, 2014

Page 2: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

© Cambridge University Press 2011

REES_Fig 10.01

Altitudes of various remote

sensing platforms

Page 3: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

low and high orbits

Page 4: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

NOTES ON BB http://topex.ucsd.edu/rs/orbits.pdf

Page 5: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

geometry of orbit plane

Page 6: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

elliptical orbit motion

perigee apogee

© Cambridge University Press 2011

Page 7: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create
Page 8: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

ground track of circular orbit

Page 9: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create
Page 10: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

low and high orbits

Page 11: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

geostationary orbit orbit period = 1 day

© Cambridge University Press 2011

Page 12: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create
Page 13: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create
Page 14: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

low and high orbits

Page 15: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

sun synchronous orbit

© Cambridge University Press 2011

Page 16: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

precession of orbit plane

© Cambridge University Press 2011

Page 17: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

Landsat ground tracks

© Cambridge University Press 2011

Page 18: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create
Page 19: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create
Page 20: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

How to compute an orbital track - 1

Page 21: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

How to compute an orbital track

Page 22: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

How to compute precise orbits from elements

Orbital elements are based on precise GPS tracking and orbit dynamic modeling.

Page 23: Platforms for Remote Sensing – Rees, Ch. 10For many remote sensing applications it is important to have the ascending node pass over the equator at the same local time. To create

http://earthobservatory.nasa.gov/Features/OrbitsCatalog/page3.php

Platforms for Remote Sensing – Rees, Ch. 1

~18,000 man-made objects orbiting the Earth