Midterm 1 Flashcards
What is Remote Sensing
Obtaining info about an object, area, or phenomenon through the analysis of data acquired by a device that is not in contact with it.
Electromagnetic Spectrum
Cosmic Rays Gamma Rays 10^-6 microns X-Rays 10^-4 microns Ultraviolet 0.1 microns Visible .4 to .7 microns Near-IR 1 micron Mid-IR Thermal IR 10 microns Microwave 10 cm TV and Radio 100 m
Frequency
Cycles per second
Stefan-Boltzmann Law
All matter above absolute zero continuously emits EM radiation and the amount of radiation is a function of the surface temperature of the object
Black body
Hypothetical ideal radiator that totally absorbs and reemits all energy incident upon it.
Wein’s Displacement Law
As the temperature increases, there is a shift toward shorter wavelengths. (Causes Red-Shift because as objects in the universe recede they cool)
Remote Sensing Steps
Energy source Radiation and the atmosphere Interaction with the target Recording of energy by the sensor Transmission, reception, processing Interpretation and analysis Application
Types of Atmospheric Effects
Scattering
Absorption
Atmospheric Scattering
Rayleigh EM > particle
Mie EM = particle
No selective EM < particle
Rayleigh Scatter
EM > particle
Shorter wavelengths more susceptible
Why the sky is blue: because blue light scatters more.
At sunset and sunrise light goes through more atmosphere so more colors are scattered.
Causes of atmospheric absorption
Water vapor
Carbon dioxide
Ozone
Atmospheric Windows
Wavelength ranges that are trans missive of EM spectrum
Energy interactions with surface features
Reflection
Absorption
Transmission
Spectral Reflectance
The percent of incident energy that is reflected from a surface.
What causes different types of Reflection?
Surface roughness.
Specular vs diffuse reflectors.
Roughness is relative to wavelength.
Radiance
Brightness on the image - the sum of light coming from the object and atmospheric scatter.