484 IEEE GEOSCIENCE AND REMOTE SENSING LETTERS, VOL. 3, NO. 4, OCTOBER 2006
Asian Dust Storm Monitoring Combining Terra
and Aqua MODIS SRB Measurements
John J. Qu, Member, IEEE, Xianjun Hao, Member, IEEE, Menas Kafatos, Member, IEEE, and Lingli Wang
Abstract—Sand and dust storms (SDSs), which present environ-
mental risks and affect the regional climate, have been worsened
in the East Asian regions over the last decade. Monitoring SDS
from space using satellite remote sensing (RS) has become one
of the most important issues in this field. At present, satellite RS
of SDS is limited to using true-color images or aerosol optical
thickness (AOT), or a new algorithm called “Deep Blue.” Using
current existing approaches makes it difficult to identify SDS from
clouds. The authors have detected SDS by combining Terra and
Aqua Moderate Resolution Imaging Spectroradiometer (MODIS)
solar reflectance band (SRB) measurements. Based on the dust
spectral characteristic, this letter proposes a normalized difference
dust index (NDDI) using MODIS reflectance measurements and
applies it to the Asian SDS cases. The simple NDDI index is found
to be able to identify SDS and clouds easily. The results suggest
that NDDI could be used to detect SDS over bright surfaces where
the MODIS AOT product is not available.
Index Terms—Aerosol, Asian, Moderate Resolution Imaging
Spectroradiometer (MODIS), normalized difference dust index
(NDDI), sand and dust storm (SDS), satellite remote sensing (RS),
Terra and Aqua.
I. I NTRODUCTION
A
SIAN sand and dust storms (SDSs) are a very important
environmental issue, and one of the major natural hazards
in the Mongolian regions and northern China [1], [2]. Major
dust storms, usually from the Mongolian desert, occur over
these regions nearly every spring. Due to the limited ground
environmental and climatic observations in the relevant regions,
satellite remote sensing (RS) has become an important ap-
proach to detect dust storms in Asia. As we know, RS can not
only provide initial parameters for model simulations but also
be used for verification and validation of model simulations
[3], [4]. Multisatellite observations such as TOMS, SeaWiFS,
AVHRR, and the Chinese FY-1C/D series have been used in
Asian dust storm monitoring. But at the present time, RS of
dust storms can only provide near global horizontal coverage
with limited vertical resolutions [5].
Early research has shown that Asian dust could transport
across the Pacific Ocean and reach as far as the western U.S.
[6]. Several international collaborative programs, such as the
Aerosol Characterization Experiment (ACE)-Asia and Asian
Dust Network (AD-Net), have been established [1]. The aerosol
Manuscript received November 19, 2005; revised April 26, 2006.
J. J. Qu is with George Mason University, Fairfax, VA 22030 USA and
also with the Goddard Space Flight Center, National Aeronautics and Space
Administration, Greenbelt, MD 20771 USA (e-mail: jqu@scs.gmu.edu).
X. Hao, M. Kafatos, and L. Wang are with George Mason University, Fairfax,
VA 22030 USA.
Digital Object Identifier 10.1109/LGRS.2006.877752
properties over the ocean are also evaluated by Moderate Reso-
lution Imaging Spectroradiometer (MODIS) during ACE-Asia
[7]. The dust storm formation mechanisms are very complex;
they are related to the local weather system, short-term pre-
cipitation, soil moisture, and extent of deforestation, long-term
increased drought, land use/land coverage changes, as well as
other human activities.
As a key research instrument of the NASA Earth Observing
System (EOS) missions, MODIS was successfully launched
onboard the Terra and Aqua satellites. MODIS senses the
Earth’s entire surface in 36 spectral bands, spanning from
the visible (0.415 µm) to the infrared (14.235 µm) regions
of the spectrum with spatial resolutions of 1 km, 500 m,
and 250 m at nadir, respectively; therefore, MODIS products
could be very useful to determine dust storm properties and
monitor dust transport. However, the current MODIS aerosol
optical depth algorithm is limited to dark surfaces [8]. There
have been limited works attempting integrated approaches to
study dust and pollution haze. Earlier works have produced
results based on true-color images or aerosol optical thickness
(AOT), but there are no MODIS AOT measurements over bright
surface regions, such as desert regions. Miller demonstrated
a new satellite-based multispectral radiometer technique for
daytime enhancement of airborne dust over water and land
using MODIS measurements [9]. The Deep Blue (minimum of
412-nm reflectance as a gridded background) approach has also
been used to physically retrieve aerosol optical properties, even
over bright surfaces, such as bright desert, semiarid, and urban
background [10].
In this letter, we describe a new index using MODIS channels
centered near 0.469 and 2.13 µm for Asian dust detection, and
apply the index to a pair of Terra and Aqua MODIS data sets.
We also discuss the index threshold to distinguish the thick
airborne dust storm from the surface features.
II. METHOD AND ANALYSIS
A. Dust Spectrum Characterization Analysis
MODIS has three different spatial resolutions including
250 m (bands 1–2), 500 m (bands 3–7), and the 1-km (bands
8–36). There are a total of 20 solar reflectance bands (SRBs)
(1–19 and 26) from 0.41–2.13 µm [11].
There are spectral signatures for hundreds of materials in
the Advanced Spaceborne Thermal Emission and Reflection
Radiometer (ASTER) spectrum library, which is used as
a reference for material identification [12]. We analyzed
the spectral signatures of sand, grass, soil, urban residential,
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