Why Do We Need Discrete Global Grids?

Satellite Remote Sensing Perspective

Ralph Kahn
Jet Propulsion Laboratory
California Institute of Technology
May 19, 1997






NASA's Earth Observing System (EOS)

AM-1 Platform (June 1998 Launch)

MODIS -- Moderate Resolution Imaging Spectrometer (36 Spectral Channels)

MISR -- Multi-angle Imaging SpectroRadiometer (4 Spectral x 9 Angles)

CERES -- Clouds and Earth's Radiant Energy System

ASTER -- Advanced Spaceborne Thermal Emission and Reflection radiometer

MOPITT -- Measurements of Pollution In The Troposphere

MISR (and MODIS) Used to Characterize, on a Global Basis: At about 1/4 km spatial resolution

Reflected Solar Radiation Budget of Earth

Measurements for global coverage:
    5.1 x 108   x   16     x      36       =     2.9 x 1011
    km2/Earth     1/4 km       channels      basic measurements


Actual MISR data:
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What Do We Want to Do With All That Data?

(Why Global?)

Early Work with Satellite Data focused on: On Time Scales of Several Weeks or more, Meridional Issues Become Important ("Climate")

Examples: To get the budgets right, you need to study global data
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What Global Grids Could Do to Help




An aside on Numerical Models:



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EOS Data "Classification"


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The Equal Angle Grid

EOS "Nominal Grid"

Intended to satisfy the basic needs of the "global modeling" community, which includes GCM builders, carbon cycle modelers, and some oceanographers, hydrologists, and bio-geo-chemical modelers



Advantages




Issues


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The Quasi-Equal Area (ISCCP) Grid

Proposed Grid Scheme from Richard Green & Bruce Weilicki:



Advantages




Issues


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How Grid Cells Are Filled

Usually the arithmetic mean of all points falling into a grid cell



Occasionally the median value of all points falling into a grid cell



Area-weighted, bi-linear interpolation used to alter cell size for comparisons among gridded data sets




How Current Binning Techniques Can Degrade Data

The three illustrations below were created as part of a global geophysical data validation exercise (Kahn, et.al., 1991) using cloud parameters derived from the High Resolution Infrared Radiation Sounder 2 (HIRS2) and the Microwave Sounding Unit (MSU) instruments aboard the NOAA polar orbiting meteorological satellites.

This illustration shows the monthly mean cloud amount for July of 1979 from the HIRS2/MSU data on a 2 degree latitude by 2.5 degree longitude grid.

Click on the image to see an enlarged gif image.
Here the data above is rebinned using area-weighted averaging into a 500 km by 500 km grid that is used for Earth radiation budget studies.

Click on the image to see an enlarged gif image.
Finally, the data in the second picture is resampled back to the 2 x 2.5 degree grid used in the first picture, and this is subtracted from the first picture. Note that the differences are nearly as large as the range of the signal, with both positive and negative values.

Click on the image to see an enlarged gif image.

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Icosahedral Snyder Equal Area (ISEA) Grid

  1. Begin with a regular icosahedron inscribed in a sphere.

  2. Each face of the icosahedron is an equilateral triangle; inscribe a hexagon in each triangle, by dividing each edge into thirds

  3. Project these hexagons back onto the sphere using the Inverse Snyder Icosahedral Equal Area Projection.

    This yields a coarse-resolution global grid, which we call Grid Resolution 1. It consists of 20 hexagons on the surface of the sphere, and 12 pentagons (each centered on one of the 12 vertices of the icosahedron). All the hexagons have the same area, and each pentagon has an area exactly 5/6 of a hexagon.

  4. To form higher resolution grids, return to the planar representation of the hexagons. Let ri be the edge length of a hexagon, on the plane, for Grid Resolution i. Tessellate each face of the icosahedron with regular hexagons of r(i+1) = 2/3 ri sin(60º).



    The area of each hexagon is sub-divided into thirds by cells at the next higher resolution.


Characteristic Length Scales for the ISEA Nested Global Grid for Earth

Resolution Number of Cells Length Scale (km)
1 32 4,684.2571
2 92 2,694.2932
3 272 1,553.6212
4 812 896.6139
5 2,432 517.5892
6 7,292 298.8166
7 21,872 172.5192
8 65,612 99.6035
9 196,832 57.5060
10 590,492 33.2011
11 1,771,472 19.1687
12 5,314,412 11.0670
13 15,943,232 6.3896
14 47,829,692 3.6890
15 143,489,072 2.1299
16 430,467,212 1.2297
17 1,291,401,632 0.7100
18 3,874,204,892 0.4099

From: Sahr et al., 1997



Advantages




Issues


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Icosahedral Snyder Equal Area (ISEA) Grid

The Possibility...

Embed each Level 2 data set in a grid with appropriate spatial resolution



Make comparisons among data sets with different inherent spatial resolution, automatically carrying along estimates of the formal errors (e.g., field validation studies)



Calculate regional and global fluxes of budget quantities, using formalism to evaluate uncertainties


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Icosahedral Snyder Equal Area (ISEA) Grid

Implementation