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Passive Microwave Remote Sensing

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Title: Intro to Remote Sensing Author: Hongjie Last modified by: Hongjie Xie Created Date: 5/19/2004 4:34:46 AM Document presentation format: On-screen Show (4:3) – PowerPoint PPT presentation

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Title: Passive Microwave Remote Sensing


1
Passive Microwave Remote Sensing
  • Lecture 11

2
Principals
  • While dominate wavelength of Earth is 9.7 um
    (thermal), a continuum of energy is emitted from
    Earth to the atmosphere. In fact, the Earth emits
    a steady stream of microwave energy as well,
    though it is relatively weak in intensity due to
    its long wavelength.
  • The spatial resolution usually low (kms) since
    the weak signal.
  • A suit of radiometers can record it. They measure
    the brightness temperature emitted from the
    terrain or the atmospheric gasses, dusts. This is
    much like the thermal infrared radiometer for
    temperature measurement as we discussed before.
  • A matrix of brightness temperature values can
    then be used to construct a passive microwave
    image.
  • To measure soil moisture, precipitation, ice
    water content, sea-surface temperature, snow-ice
    temperature, and etc., based on brightness
    temperature images.

3
Rayleigh-Jeans approximation of Plancks law
Thermal infrared domain (Plancks law)
Microwave domain (Rayleigh-Jeans approximation)
Recall
Let
We have
We have
Unit is Wm-2Hz
4
  • For a Lambertian surface, the surface brightness
    radiation B(v,T),
  • The really useful simplification involves
    emissivity and brightness temperature in
    microwave range

Unit is Wm-2Hzsr
In comparison with thermal infrared (TB)4 e?
(T)4
5
Some important passive microwave radiometers
  • Special Sensor Mirowave/Imager (SSM/I)
  • It was onboard the Defense Meterorological
    Satellite Program (DMSP) since 1987
  • It measure the microwave brightness temperatures
    of atmosphere, ocean, and terrain at 19.35,
    22.23, 37, and 85.5 GHz.
  • TRMM microwave imager (TMI)
  • It is based on SSM/I, and added one more
    frequency of 10.7 GHz.

6
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7
AMSR-E
  • Advanced Microwave Scanning Radiometer EOS
  • It observes atmospheric, land, oceanic, and
    cryospheric parameters, including precipitation,
    sea surface temperatures, ice concentrations,
    snow water equivalent, surface wetness, wind
    speed, atmospheric cloud water, and water vapor.
  • At the AMSR-E low-frequency channels, the
    atmosphere is relatively transparent, and the
    polarization and spectral characteristics of the
    received microwave radiation are dominated by
    emission and scattering at the Earth surface.
  • Over land, the emission and scattering depend
    primarily on the water content of the soil, the
    surface roughness and topography, the surface
    temperature, and the vegetation cover.
  • The surface brightness T (TB ) tend to increase
    with frequency due to the absorptive effects of
    water in soil and vegetation that also increase
    with frequency. However, as the frequency
    increase, scattering effects from the surface and
    vegetation also increase, acting as a factor to
    reduce the TB

8
AMSR-E
Najoku et al. 2005
9
Example1 Snow depth or snow water equivalent
(SWE)
  • The microwave brightness temperature emitted from
    a snow cover is related to the snow mass which
    can be represented by the combined snow density
    and depth, or the SWE (a hydrological quantity
    that is obtained from the product of snow depth
    and density).

?Tb Tb19V-Tb37V
10
Large grains tend to scatter microwave radiation
more than smaller grains
Volume fraction () snow density/900 From
fresh snow to packsnow, the snow density increase
from lt100 kg m-3 to between 200-400 kg m-3
Kelly et al. 2003
11
3. Study Area (1)
Example 1
12
Impact of snow density (4)-mean SD
Snow density 0.4 g/cm3 or 400 kg m-3
Multi-snow density
Wang, Xie, and Liang 2006
13
Results AMSR-E vs ground- SD at individual
stations (snow density 0.4 g/cm3)
14
Results AMSR-E vs ground- SD at individual
stations (snow density 0.4 g/cm3)
15
Results Annual change of SWE in YWR
16
Antarctic sea ice
Example 2
17
Footprint size 58 km 37 km 21
km 11 km 5 km
Level 2 data
18
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19
Footprint size 58 km 37 km 21
km 11 km 5 km
AMSR Bootstrap/ Ice temperature
20
Footprint size 58 km 37 km 21
km 11 km 5 km
AMSR Bootstrap/ Ice temperature
Bootstrap
21
Footprint size 58 km 37 km 21
km 11 km 5 km
AMSR Bootstrap/ Ice temperature
Bootstrap
NASA Team 2/ Snow depth
22
AMSR-E derived sea ice concentrations
23
Ice Concentration/area
Based on SMMR-SSM/I (http//nsidc.org)
24
Compare AMSR-E ice concentration and NIC ice edge
Cicek et al. 2009
25
Snow cover
  • Idea
  • Radiation from the ground is scattered by the
    snow cover.
  • The more snow the more scattering.
  • Scattering efficiency is frequency dependent.
  • hs c (T37GHz-T19GHz)
  • Difficulties
  • Different terrain forms (e.g., tundra, mountains,
    plains) different ice properties (FY/MY icel,
    ridges)
  • Scattering varies with snow physical properties
    (e.g., grain size, density, wetness)

(From C.L. Parkinson, Earth from above,1997)
26
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27
Monthly snow depth data are derived from
satellite passive microwave data
28
A Weddell Sea 7/86 - 9/86
(Wadhams et al., 1986) B East Antarctic
10/88 - 12/88 (Allison et al.,
1993) C Weddell Sea 9/89 -
10/89 (Eicken et al., 19994) D East
Antartic 11/91
(Worby and Massom, 1991) E Weddell Sea
6/92 - 7/92 (Drinkwater and Haas,
1994) F East Antarctic 10/92 -
11/92 (Worby and Massom, 1995) G East
Antarctic 3/93 - 5/93 (Worby
and Massom, 1995) H Bellingshausen
8/93 - 9/93 (Worby et al., 1996) I
Amundsen 9/94 - 10/94
(Sturm et al., 1998) J East Antarctic
9/94 - 10/94 (Jeffries et al.,
1995) K Ross Sea 5/95
- 6/95 (Sturm et al.,1998) L Ross
Sea/Bellingshausen 8/95-9/95 (Sturm et al.,
1998)
29
Inter-annual variability of September snow
depth (on a pixel-by-pixel basis)
30
Radio-frequency interference contaminate the 6.9
and 10.7 GHz channels
Example 3
  • Radio-frequency interference (RFI) includes the
    cable television relay, auxiliary broadcasting,
    mobile. RFI is several orders of magnitude higher
    than natural thermal emissions and is often
    directional and can be either continuous or
    intermittent.
  • Radio-frequency interference (RFI) is an
    increasingly serious problem for passive and
    active microwave sensing of the Earth.
  • The 6.9 GHz contamination is mostly in USA,
    Japan, and the Middle East.
  • The 10.7 GHz contamination is mostly in England,
    Italy, and Japan
  • RFI contamination compromise the science
    objectives of sensors that use 6.9 and 10.7 GHz
    (corresponding to the C-band and X-band in active
    microwave sensing) over land.

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32
radio-frequency interference (RFI) index (RI)
33
Li et al. 2004
34
6.9 GHz contamination
Najoku et al. 2005
35
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