Remote sensing
• Remote sensing is the acquiring of information from a
distance.
• NASA observes Earth and other planetary bodies via
remote sensors on satellites and aircraft that detect and
record reflected or emitted energy.
• Orbits
• Observing with the Electromagnetic Spectrum
• Sensors
• Resolution
• Data Processing, Interpretation, and
• Analysis
Orbits
• Satellites can be placed in several types of orbits around Earth.
• Low-Earth orbit (approximately 160 to 2,000 km above Earth),
• Medium-Earth orbit (approximately 2,000 to 35,500 km above
Earth), and
• High-Earth orbit (above 35,500 km above Earth).
• Satellites orbiting at 35,786 km are at an altitude at which their
orbital speed matches the planet's rotation, and are in what is
called geosynchronous orbit (GSO).
• In addition, a satellite in GSO directly over the equator will
have a geostationary orbit.
• A geostationary orbit enables a satellite to maintain its position
directly over the same place on Earth’s surface.
• Sun-synchronous; the satellite passes over the same location at
the same solar time each cycle, e.g. NASA’s Aqua satellite
Geostationary
Sun-synchronous
Observing with the Electromagnetic Spectrum
• Visible light sits in the middle of that range of long to shortwave
radiation.
• human eye is able to detect a small portion.
• Instrumentation is needed to detect all other forms
• The primary source of the energy observed by satellites, is the Sun.
• Snow has a very high albedo and reflects up to 90% of incoming
solar radiation.
• The ocean, on the other hand, reflects only about 6%.
Sensors
• Sensors that use natural energy from the Sun
are called passive sensors.
• Those that provide their own source of energy
are called active sensors.
Resolution
• Radiometric resolution is the amount of information in each pixel,
that is, the number of bits representing the energy recorded.
• Spatial resolution is defined by the size of each
pixel within a digital image and the area on
Earth’s surface represented by that pixel.
Pixel resolution
• Spectral resolution is the ability of a sensor to discern
finer wavelengths, or
• the ability of a sensor to define fine wavelength intervals.
or
• The range of wavelengths that a single band in an
imaging system can detect.
• Temporal resolution is the time it takes for a
satellite to complete an orbit and revisit the same
observation area.
• This resolution depends on the orbit, the sensor’s
characteristics, and the swath width.
• Because geostationary satellites match the rate at
which Earth is rotating, the temporal resolution is
much finer.
• Polar orbiting satellites have a temporal resolution
that can vary from 1 day to 16 days.
Imagery
Interpretation of imagery
Look for a Scale
• One of the first things people want to do when they look at a
satellite image is identify the places that are familiar to them:
• Look for patterns, shapes, and textures
• Define colours
• Water
• Plants
• Bare ground
• Cities
• Atmosphere
• Ground truthing

Remote sensing presentation explanation pptx

  • 1.
  • 2.
    • Remote sensingis the acquiring of information from a distance. • NASA observes Earth and other planetary bodies via remote sensors on satellites and aircraft that detect and record reflected or emitted energy. • Orbits • Observing with the Electromagnetic Spectrum • Sensors • Resolution • Data Processing, Interpretation, and • Analysis
  • 3.
    Orbits • Satellites canbe placed in several types of orbits around Earth. • Low-Earth orbit (approximately 160 to 2,000 km above Earth), • Medium-Earth orbit (approximately 2,000 to 35,500 km above Earth), and • High-Earth orbit (above 35,500 km above Earth). • Satellites orbiting at 35,786 km are at an altitude at which their orbital speed matches the planet's rotation, and are in what is called geosynchronous orbit (GSO). • In addition, a satellite in GSO directly over the equator will have a geostationary orbit. • A geostationary orbit enables a satellite to maintain its position directly over the same place on Earth’s surface. • Sun-synchronous; the satellite passes over the same location at the same solar time each cycle, e.g. NASA’s Aqua satellite
  • 4.
  • 5.
    Observing with theElectromagnetic Spectrum • Visible light sits in the middle of that range of long to shortwave radiation. • human eye is able to detect a small portion. • Instrumentation is needed to detect all other forms
  • 6.
    • The primarysource of the energy observed by satellites, is the Sun. • Snow has a very high albedo and reflects up to 90% of incoming solar radiation. • The ocean, on the other hand, reflects only about 6%.
  • 7.
    Sensors • Sensors thatuse natural energy from the Sun are called passive sensors. • Those that provide their own source of energy are called active sensors.
  • 8.
    Resolution • Radiometric resolutionis the amount of information in each pixel, that is, the number of bits representing the energy recorded.
  • 9.
    • Spatial resolutionis defined by the size of each pixel within a digital image and the area on Earth’s surface represented by that pixel.
  • 10.
  • 11.
    • Spectral resolutionis the ability of a sensor to discern finer wavelengths, or • the ability of a sensor to define fine wavelength intervals. or • The range of wavelengths that a single band in an imaging system can detect.
  • 12.
    • Temporal resolutionis the time it takes for a satellite to complete an orbit and revisit the same observation area. • This resolution depends on the orbit, the sensor’s characteristics, and the swath width. • Because geostationary satellites match the rate at which Earth is rotating, the temporal resolution is much finer. • Polar orbiting satellites have a temporal resolution that can vary from 1 day to 16 days.
  • 13.
  • 14.
    Interpretation of imagery Lookfor a Scale • One of the first things people want to do when they look at a satellite image is identify the places that are familiar to them:
  • 15.
    • Look forpatterns, shapes, and textures
  • 17.
  • 18.
    • Water • Plants •Bare ground • Cities • Atmosphere • Ground truthing