Satellite Remote Sensing

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Introductory Digital Image Processing. 3rd edition. Jensen, 2004
Electromagnetic Energy Introductory Digital Image Processing. 3rd edition. Jensen, 2004 Thermonuclear fusion on the surface of the Sun yields a continuous spectrum of electromagnetic energy. The 6,000 K temperature of this process produces a large amount of short wavelength energy (from 0.4 - 0.7 µm; blue, green, and red light) that travels through the vacuum of space at the speed of light. Some energy is intercepted by the Earth where it interacts with the atmosphere and surface materials. The Earth may reflect some of the energy directly back out to space or it may absorb the short wavelength energy and then re-emit emit it at a longer wavelength.
Page 1 and 2: Satellite Remote Sensing GE 4150- N
Page 3 and 4: Remote Sensing A remote sensing ins
Page 5: Remote Sensing Information about an
Page 9 and 10: Sensors Passive Sun’s energy wh
Page 11 and 12: Introductory Digital Image Processi
Page 13 and 14: Radiometric Resolution 0 0 7-bit (0
Page 15 and 16: MODIS Moderate Resolution Imaging
Page 17 and 18: Mount Belinda South Sandwich Islan
Page 19 and 20: ASTER Advanced Spaceborne Thermal
Page 21: http://asterweb.jpl.nasa.gov/conten
Page 24 and 25: LANDSAT Launched in 1972, Managed
Page 26 and 27: http://www.geo.mtu.edu/volcanoes/re
Page 28 and 29: Active Sensors Emits energy pulse,
Page 30: LIDAR Light Detection and Ranging

Satellite Remote Sensing

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