GEOG*2420
The Earth From Space
Electromagnetic Radiation
and the Spectrum
John Lindsay
Fall 2015
Readings
JR Jensen Chapter 2
Wave Properties of EM radiation
- Maxwell (1831-1879) conceptualized EMR as wave traveling through space at the speed of
light, c.
- c = 3x108 m/s, enough to circle the Earth 7.5 times a second!
- The EM wave consists of two orthogonal fluctuating fields, one electric and one magnetic.
(source: Jensen, 2007)
Wave Properties of EM radiation
(source: http://www.molphys.leidenuniv.nl/monos/smo/index.html?basics/light_anim.htm)
Properties of EM radiation
- Wavelength (λ) – distance between maximums
- Frequency (ν) – number of wavelengths that pass per unit of time
- Long wave lengths = lower frequency and vice versa
- That is, ν is inversely proportional to λ such that:
\(\nu=\frac c\lambda\)
Properties of EM radiation
(source: Jensen, 2007)
Common Units of Measurement
- Micrometre (not micrometer) μm: one millionth of a metre, 1 × 10-6 m
- Nanometre (nm): one billionth of a metre, 1 × 10-9 m or 1 × 10-3 μm
- Angstrom (Å): 0.1 nanometre or 1 × 10-10 m
- Also cm or metres for longer wavelengths
Common Units of Measurement
The Electromagnetic Spectrum
(source: "EM Spectrum Properties edit" by Inductiveload, information by NASA)
The Electromagnetic Spectrum
(source: Christopherson and Byrne, 2008)
The Electromagnetic Spectrum
(source: Jensen, 2007)
Portions of the Spectrum Important for Remote Sensing
- Ultraviolet: .10 μm — .40 μm
- Visible: .40 μm — .70 μm
- Blue: .40 μm — .50 μm
- Green: .50 μm — .60 μm
- Red: .60 μm — .70 μm
- Infrared: (.7—1) μm — 1000 μm, i.e. 1 mm
- Near or reflected: (.7—1) μm to 3 μm
- Mid-infrared: 3 μm to (25–50) μm
- Far or thermal: (25–50) μm to 1000 μm
- Microwave 0.3 cm to 30.0 cm
- Note: All ranges are approximate
The amount of energy associated with EMR is inversely related to its wavelength
(source: Jensen, 2007)
Interaction with matter
Reflectance
Reflectance is the ratio of energy reflected (bounced off) to the energy incident upon.
Reflectance
(source: NASA’s Observatorium, 1999)
Transmittance and Refractance
- Transmittance is the propagation of energy through a medium.
- Refractance occurs when EMR is transmitted through the interface between materials
of different optical density.
Refraction is bending of light due to a change
in speed
Absorptance
Why is the transmitted light from these filters coloured?
(source: http://www.aoe.com.au/filters.html)
Absorptance
- Absorbed energy is converted to some other form, e.g. heat.
- It is frequently re-radiated (emitted).
Atmospheric Scattering
- Results in a change in the path of a ray, but not the characteristics of light, i.e. the
speed and wavelength.
- Rayleigh Scattering: diameter of matter is smaller (<0.1) than λ
- Mie Scattering: due to particles approximately equal to the λ (dust, pollen, water vapour)
- Non-selective Scattering: due to large particles (water droplets)
Atmospheric Scattering
(source: Jensen, 2007)
Atmospheric Scattering
(source: Unknown)
The blue sky results from the preferential
scattering of the shorter blue wavelength of visible light...Rayleigh scattering!
Atmospheric Absorption
- Absorption occurs in the atmosphere due to interaction with water, carbon dioxide,
ozone and nitrous oxide.
- This gives the atmosphere absorption bands where no EMR at a certain λ is
available for remote sensing.
Atmospheric Windows
(source: Jensen, 2007)
Atmospheric Windows
(source: Jensen, 2007)