Your SlideShare is downloading. ×
Cloud shadow detection over water
Upcoming SlideShare
Loading in...5

Thanks for flagging this SlideShare!

Oops! An error has occurred.

Saving this for later? Get the SlideShare app to save on your phone or tablet. Read anywhere, anytime – even offline.
Text the download link to your phone
Standard text messaging rates apply

Cloud shadow detection over water


Published on

Published in: Technology, Business

1 Comment
  • Be the first to like this

No Downloads
Total Views
On Slideshare
From Embeds
Number of Embeds
Embeds 0
No embeds

Report content
Flagged as inappropriate Flag as inappropriate
Flag as inappropriate

Select your reason for flagging this presentation as inappropriate.

No notes for slide


  • 1. PresentationOptical Algorithm for Cloud ShadowDetection over Water(REMOTE SENSING)
  • 2. REMOTE SENSING• The diagram shows the general process of gathering information by optical sensors.• Light from source A falls on the landmass C which is reflected to the sensor D.• The signals are then sent to the receiving station where the images are processedreferring to F which is then passed as data to the human interpreter G.• B and E refer to the Electromagnetic waves.
  • 3. Role of Clouds in RemoteSensing•Clouds cause a serious problem forthe sensors. They not only conceal theground but also cast shadows.•These shadows also occur in theobserved images along with theclouds.•The main problem caused by shadowsis either a reduction or total loss ofinformation in an image.•But shadows can also be used toestimate both cloud base and cloud-top height which are still a challengefrom space.•It can also impact mesoscaleatmospheric circulations that lead tomajor convective storm systems.Clouds and their shadows over land.Clouds and their shadows over water.
  • 4. SENSORSHYPERION• A hyper spectral sensor on board NASA’sEO-1 satellite.• Spatial resolution about 30 meters.• Spectral configuration of 430nm-2400nm.• Designed for land operations.• Useful for coastal areas and Navyoperations.• Not suitable for water studies.MODIS• Moderate Resolution ImagingSpectroradiometer(MODIS) is currentlyaboard the Terra and Aqua spacecraft.• Two spatial resolution bands of 250meters each.• Wide spectral range: 0.41-14.24µm.• Used for global monitoring of terrestrialecosystems, fires, ocean biologicalproperties and sea surface temperature.
  • 5. SHADOW DETECTION OVER LAND• Location of shadows depends on:– Cloud elevation.– Incidence angle of the sunlight at that time.• For geometrical calculations ,we need:– Cloud-top and cloud-bottom heights.– Sun and satellite positions.• Main issue is determination of cloud vertical height.• Thermal channels can be used to estimate cloud-top height but cloud-bottomheight estimation is still a challenge.• Another method is to use brightness thresholds of clouds but it is a difficultprocess as the brightness values can be very close to those of their neighbors.
  • 6. The image on the left depicts a sun-cloud geometry for shadow detection.The image on the right tells the projections of clouds at discrete heights fromsea level.
  • 7. SHADOW DETECTION OVER WATER• The brightness of shadows over water pixels varies with atmospheric conditions. Thereforethe brightness values from shadow and close-by sunlit regions over water can provideinformation if a small portion of the image is examined at a time.• It is because water-leaving radiance over sunlit pixels results from both direct and diffusesolar irradiance while the water-leaving radiance over shadowed pixels results from onlydiffuse solar irradiance.Sunlit pixelhaving direct anddiffuse radianceShadow pixel having onlydiffuse solar radiance
  • 8. •The diffuse part of the incident radiation is radiation from the sky, exclusive of thesun. It comes from clouds or from the blue sky, i.e. from many directionssimultaneously.•The direct part comes directly from the direction of the sun and can, therefore, castshadows.•Water-leaving radiance is the light emitted from the water pixels.•This paper does not use any angular information or cloud height estimation. It isa cloud shadow detection technique acquired over water by satellite/airbornesensors.It is derived for optical imageries entirely based on measurements in the opticalchannels.
  • 9. DATA OF THE RESEARCH• Hyperspectral Imager for the Coastal Ocean(HICO)– The HICO has been operating aboard the ISS since 24 September, 2009.– Provides hyperspectral images at 100 meters resolution optimized for the coastal ocean.– Collects radiance at 128 contiguous spectral channels from 350 to 1070nm range.– Each HICO scene is 50km in width by 200km in length.– HICO data flow from the ISS provides 15 scenes per day and managed by U.S. Naval Research Lab.– Has high spectral resolution, thus contrast between shadowed and adjacent sunlit regions would behigher after integrating the spectra which is advantageous for shadow detection.
  • 10. Lsdw w (λ)From shadowed regionLsny w(λ)From sunlit region•Assuming sensor is at nadir, i.e. directly below and a thick cloud over water preventing directsolar photons on the sea surface and generating a shadow region.•The total radiance measured by the sensor from the sunlit area is:Lsny t (λ) = La (λ) + t(λ) Lsny w (λ)---------------------->(1)La from the atmosphere
  • 11. where t(λ) represents the diffuse transmittance of the atmosphere for the water-leaving radiance.The total radiance over the shadowed region is :Lsdw t (λ) = La (λ) + {t(λ) +Δt(λ)} Lsdw w (λ)------------>(2)where Δ represents the perturbations due to the differences in illuminations between the sunlit andshadowed regions.Water-leaving radiance can be expressed as two parts:•Part caused by the backscattering of the diffuse skylight•Part caused by the backscattering of the direct solar beamFor sunlit and shadowed regions ,the water-leaving radiance can be expressed as:Lsny w (λ) = Lsny wsky (λ) + Lsny wdir (λ) andLsdw w (λ) = Lsdw wsky (λ)Where Lsny wsky (λ) / Lsdw wsky (λ) and Lsny wdir (λ) / Lsdw wdir (λ) represent the water-leaving radiances caused by diffuse skylight and direct solar beam / shadowed regionin the sunlit region.
  • 12. According to P.Reinersman , K.L. Carder and F.R. Chen, “Satellite-sensor calibrationverification with the cloud shadow method” vol. 37, no. 24, pp.5541-5549, Aug. 1998., Lsnywsky (λ) can be expressed asLsny wsky (λ) = Lsdw wsky (λ) + ΔLsdw wsky (λ)•From the analysis , it can be expected that the water-leaving radiance from the shadowedpixel reaching the satellite sensor is lower than the water-leaving radiance from theneighboring sunlit pixels.•Thus, the total radiance measured over the shadowed pixel is lower than that measuredover the neighboring sunlit pixel.•An example of HICO image taken over Guamisland in 2009. the adjacent sunlit pixel hashigher digital counts(green line) overshadowed pixels(red line).
  • 13. DEVELOPMENT OF CSDI• The above proposed technique indicates that the spectral shape or amplitude alone is notadequate to separate the two regions for an entire image. It can be only done if a smallportion is examined.• So , we introduce a cloud shadow detection technique called the CSDI asCSDI=IV c / <IV ASB >---------------->(3)– Where IVc represents the IV index of the pixel (the central pixel of ASB which is thesmall portion ) that needs to be classified as a shadowed or sunlit pixel.– The <IV ASB > represents the spatial mean of the IV indices within the selected ASB ofthis pixel.– The IV index is defined as• IV=∫ Lt(λ) dλ from 400nm to 600 nm---------------------(4)• CSDI is mainly used for deep waters. Before applying CSDI , cloud needs to be removedproperly. The ASB needs to be selected carefully so that it only contains shadowed and sunlitpixels or only sunlit pixels because to make the denominator of CSDI larger than thenumerator for shadowed and vice versa for sunlit pixels.
  • 14. •It is important to select the ASB in such a way that it is bigger than the shadowed region.•This can be achieved by using the cloud size information since cloud is generally bigger thanthe shadow and relatively easy to detect.•If the selected ASB contains only sunlit pixels and the pixel under examination is also asunlit pixel, the CSDI value for this pixel would be around one since the mean of the ASB[denominator of (3)] and the IV index [numerator of (3)] would be about the same.•If the ASB contains both shadowed and sunlit pixels and the pixel under examination is asunlit pixel, the CSDI value will be greater than one since the mean of the ASB will be slightlylower than the IV index of the pixel under examination.•On the other hand, if the pixel under examination happens to be a shadowed pixel, theCSDI value would be less than one since the IV index of this shadowed pixel would besmaller than the mean of the ASB. Now, if the ASB contains only shadowed pixels, it can beproblematic since the CSDI value will be around one, like the case of only sunlit pixels. Theywill be classified as sunlit pixels if the CSDI threshold is put less than one.
  • 16. Images showing relatively larger area of clouds using CSDI technique
  • 17. BENEFITS AND DRAWBACKS OF CSDI•Benefits•Relatively easy to use and faster than geometry based approach.•Does not require thermal channels which are not always present on ocean sensors.•Based on top-of-the-atmosphere readings or airborne sensors.•Drawbacks•May give spurious results in non-homogenous or shallow waters.•Cannot detect shadows in the edge pixels of satellite images. But an IV image can beused to visually identify the shadows in those pixels since shadows appear dimmer inan IV image.
  • 18. CONCLUSION•A cloud shadow-detection technique (CSDI) has been developed and applied to HICO datacollected from various locations to isolate shadowed pixels. The shapes of the clouds andcloud shadows observed in the CSDI images closely resemble those of clouds and cloudshadows in the corresponding true color and IV images. The agreement between the truecolor, IV, and CSDI images is very reasonable over open ocean.• This suggests the potential of the cloud shadow detection using the proposed techniquewhich only uses the top-of-the atmosphere optical readings of the space borne or airborneimagers. Although the proposed CSDI threshold works reasonably well on the selected HICOimages, further studies are necessary to fine tune the threshold and the selection of optimalASB size based on image scene content for automated processing.