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Internal wave detection using the Moderate Resolution Imaging Spectroradiometer (MODIS) Christopher Jackson 1 Received 14 March 2007; revised 14 July 2007; accepted 3 August 2007; published 16 November 2007. [1] The Moderate Resolution Imaging Spectroradiometer (MODIS), with its combined attributes of fine spatial resolution, large swath area, and near-daily global coverage, has for the first time allowed sunglint (the near-specular reflectance pattern of sunlight off the ocean surface) to be used to analyze and survey high-frequency nonlinear internal solitary wave occurrences on a near-global scale. The sunglint area within the MODIS swath is large enough to cover an entire basin, and it’s spatial resolution is fine enough to identify internal wave signatures whose wavelength is greater than a few hundred meters. This paper describes the use of MODIS for high-frequency nonlinear internal wave detection, presents the results of a survey that detected 3581 internal wave occurrences in MODIS imagery over the period between August 2002 through May 2004, and discusses ways MODIS imagery can be used to improve the study of internal waves. Citation: Jackson, C. (2007), Internal wave detection using the Moderate Resolution Imaging Spectroradiometer (MODIS), J. Geophys. Res., 112, C11012, doi:10.1029/2007JC004220. 1. Introduction [2] Since the early 1970s, high-frequency nonlinear internal waves have been distinctive features in photographs, multispectral radiometer images, and synthetic aperture radar images of the sea surface obtained by spacecraft [Jackson, 2004]. The waves manifest themselves as alternating bands of light and dark quasilinear strips that remain coherent over tens to hundreds of kilometers. Internal waves occur globally, produced by a combination of stratification, bathymetry, and current flow and are important in the energy exchange between the large-scale tides and small- scale mixing. Historically, occurrences of these waves has been noted on the continental shelves, especially during the summer months [Colosi et al., 2001; Moum et al., 2003], as well as in straits [Farmer and Armi, 1999] and in the marginal seas [Apel et al., 1985; Osborne and Burch, 1980]. [3] The use of sunglint imagery for internal wave detec- tion has been previously applied to astronaut photography [Apel, 1979], imagery acquired from Landsat [Apel et al., 1975; Sawyer, 1983] and the Defense Meteorological Satellite Program (DMSP) satellites [Fett et al., 1979]. More recent work by Mitnik et al. [2000] examined the similarities and differences in internal wave signatures between synthetic aperture radar (SAR) and sunglint images from SPOT. These studies demonstrated the utility of sunglint for the detection of internal waves, but each was focused on a limited geographic area for a short period of time. [4] The MODIS (Moderate Resolution Imaging Spectro- radiometer) sensor collects data in a continuous, systematic manner at 250-m resolution on a 2300-km swath. It produces almost daily world wide coverage which results in a large volume of imagery that has for the first time, allowed the near-specular reflectance pattern of sunlight off the ocean surface (sunglint) to be used to identify high- frequency nonlinear internal solitary wave occurrences on a near-global scale. These characteristics make MODIS imagery particularly well suited for surveying and cata- loging internal wave occurrences and for studying the evolution of internal wave fields. [5] This paper discusses the characteristics of the MODIS sensor and how high-frequency nonlinear internal waves are detected in the sunglint regions of the true-color imagery (section 2). It then presents an overview of an internal wave survey using MODIS true-color imagery covering 21 months between August 2002 and May 2004 that resulted in the detection of 3581 internal wave occurrences (section 3). Section 4 presents the analysis of internal wave signatures in MODIS images from seven areas of the world. Section 5 discusses how the imagery can be used to support internal wave studies when wave observations are made on short timescales and when a large database of observations are available. 2. MODIS (Moderate Resolution Imaging Spectroradiometer) [6] The MODIS sensors are onboard the National Aero- nautics and Space Administration’s (NASA’s) Earth Observing System satellites Terra and Aqua. These satellites, launched in 1999 and 2002 respectively, are in Sun-synchronous orbit at approximately 700-km altitude and each MODIS sensor collects data continuously along a JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 112, C11012, doi:10.1029/2007JC004220, 2007 Click Here for Full Articl e 1 Global Ocean Associates, Alexandria, Virginia, USA. Copyright 2007 by the American Geophysical Union. 0148-0227/07/2007JC004220$09.00 C11012 1 of 13

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Page 1: Linux Support for HFC-S PCI

Internal wave detection using the Moderate Resolution Imaging

Spectroradiometer (MODIS)

Christopher Jackson1

Received 14 March 2007; revised 14 July 2007; accepted 3 August 2007; published 16 November 2007.

[1] The Moderate Resolution Imaging Spectroradiometer (MODIS), with its combinedattributes of fine spatial resolution, large swath area, and near-daily global coverage, hasfor the first time allowed sunglint (the near-specular reflectance pattern of sunlight offthe ocean surface) to be used to analyze and survey high-frequency nonlinear internalsolitary wave occurrences on a near-global scale. The sunglint area within theMODIS swathis large enough to cover an entire basin, and it’s spatial resolution is fine enough toidentify internal wave signatures whose wavelength is greater than a few hundred meters.This paper describes the use of MODIS for high-frequency nonlinear internal wavedetection, presents the results of a survey that detected 3581 internal wave occurrences inMODIS imagery over the period between August 2002 through May 2004, and discussesways MODIS imagery can be used to improve the study of internal waves.

Citation: Jackson, C. (2007), Internal wave detection using the Moderate Resolution Imaging Spectroradiometer (MODIS),

J. Geophys. Res., 112, C11012, doi:10.1029/2007JC004220.

1. Introduction

[2] Since the early 1970s, high-frequency nonlinearinternal waves have been distinctive features in photographs,multispectral radiometer images, and synthetic aperture radarimages of the sea surface obtained by spacecraft [Jackson,2004]. The waves manifest themselves as alternating bandsof light and dark quasilinear strips that remain coherentover tens to hundreds of kilometers. Internal waves occurglobally, produced by a combination of stratification,bathymetry, and current flow and are important in theenergy exchange between the large-scale tides and small-scale mixing. Historically, occurrences of these waves hasbeen noted on the continental shelves, especially duringthe summer months [Colosi et al., 2001; Moum et al.,2003], as well as in straits [Farmer and Armi, 1999] andin the marginal seas [Apel et al., 1985; Osborne andBurch, 1980].[3] The use of sunglint imagery for internal wave detec-

tion has been previously applied to astronaut photography[Apel, 1979], imagery acquired from Landsat [Apel et al.,1975; Sawyer, 1983] and the Defense MeteorologicalSatellite Program (DMSP) satellites [Fett et al., 1979].More recent work by Mitnik et al. [2000] examined thesimilarities and differences in internal wave signaturesbetween synthetic aperture radar (SAR) and sunglint imagesfrom SPOT. These studies demonstrated the utility ofsunglint for the detection of internal waves, but each wasfocused on a limited geographic area for a short period oftime.

[4] The MODIS (Moderate Resolution Imaging Spectro-radiometer) sensor collects data in a continuous, systematicmanner at 250-m resolution on a 2300-km swath. Itproduces almost daily world wide coverage which resultsin a large volume of imagery that has for the first time,allowed the near-specular reflectance pattern of sunlight offthe ocean surface (sunglint) to be used to identify high-frequency nonlinear internal solitary wave occurrences ona near-global scale. These characteristics make MODISimagery particularly well suited for surveying and cata-loging internal wave occurrences and for studying theevolution of internal wave fields.[5] This paper discusses the characteristics of the MODIS

sensor and how high-frequency nonlinear internal waves aredetected in the sunglint regions of the true-color imagery(section 2). It then presents an overview of an internalwave survey using MODIS true-color imagery covering21 months between August 2002 and May 2004 thatresulted in the detection of 3581 internal wave occurrences(section 3). Section 4 presents the analysis of internal wavesignatures in MODIS images from seven areas of the world.Section 5 discusses how the imagery can be used to supportinternal wave studies when wave observations are made onshort timescales and when a large database of observationsare available.

2. MODIS (Moderate Resolution ImagingSpectroradiometer)

[6] The MODIS sensors are onboard the National Aero-nautics and Space Administration’s (NASA’s) EarthObserving System satellites Terra and Aqua. Thesesatellites, launched in 1999 and 2002 respectively, are inSun-synchronous orbit at approximately 700-km altitudeand each MODIS sensor collects data continuously along a

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 112, C11012, doi:10.1029/2007JC004220, 2007ClickHere

for

FullArticle

1Global Ocean Associates, Alexandria, Virginia, USA.

Copyright 2007 by the American Geophysical Union.0148-0227/07/2007JC004220$09.00

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2300-km wide swath providing near-global daily coverage.The MODIS data are acquired at 36 channels in the visibleand infrared regions the spectrum, with a spatial resolutionbetween 250 m and 1 km dependent on the collectionwavelength [Salomonson et al., 1989] and with a geo-location accuracy of at least 60 m (1s) [Wolfe, 2006]. Thetrue-color images are created from the calibrated, correctedand geolocated radiance (Level-1B) data by compositingMODIS Bands 1 (855 nm at 250 m resolution), 4 (553 nm at500 m resolution) and 3 (466 nm at 500 m resolution) intothe red, green and blue image channels respectively. Fulldetails of the characteristics of MODIS and its associateddata products are given by Qu et al. [2006] or on the NASAMODIS website (modis.gsfc.nasa.gov).[7] The MODIS imagery collected during the daylight

portion of its orbital period contain distinctive narrowsilvery-gray ellipses of reflected sunlight over the oceanswhere angle of reflection, is within approximately 30� of theSun’s specular reflection point. These sunglint ellipses,located to the east of the swath center for Terra, (west forAqua), are approximately 500 km across their minor axisand can extend for more than 45 degrees in latitude. It is inthese sunglint regions, where standard ocean color productscannot be retrieved [Esaias et al., 1998], that internal wavesignatures are readily detected.[8] Cox and Munk [1954] described the relationship

between sunlight reflected from the sea surface, the distri-bution of surface wave slopes (i.e., sea surface roughness)and wind speed. They showed that sunglint reflection isheavily biased toward the capillary and short gravity wavesset up by wind roughening [Munk et al., 2000]. It is thesecapillary and short gravity waves, modified by the variablesurface currents associated with internal waves, that allowthe internal waves to be observed in satellite imagery forwind speeds of approximately 2 m/s to 10 m/s [Hennings etal., 1994; Holt, 2004]. In addition, there is a geometrydependence that will cause either the rough or smooth zoneson the surface to appear either bright or dark depending onif the zones are contained in what Munk et al. [2000]describe as the inner ‘‘glitter’’ or outer ‘‘glitter’’ regions.The inner glitter regions require only a small slope on theocean surface to satisfy the specular (or near specular)condition where in the outer glitter region, farther off thesensor nadir, requires steeper facets to produce the sunglintreflection.[9] Nonlinear internal waves manifest themselves as

either isolated wave fronts (usually called solitons) or incollections of waves, called packets, were the number ofindividual waves in a packet can vary from three to a fewdozen, depending on their age and distance from thegeneration point. The internal waves appear in the imageryas alternating bands of light and dark strips that result fromvariations in sea surface roughness [Alpers, 1985]. Theroughness variations are caused by the creation of conver-gent (rough) and divergent (smooth) zones set up by theinternal wave currents that move across the surface in phasewith wave’s subsurface crests and troughs [Munk et al.,2000]. Internal wave wavelength, here defined as thedistance between two corresponding points on successivewaves in a packet, varies from approximately 200 m to15 km and the waves can have along crest lengths from afew tens to few hundred kilometers.

[10] While sunglint imagery from other optical sensors(Landsat, SPOT, ASTER, AVHRR, DMSP) can be, or hasbeen, used for internal wave observation, these imagery allhave limitations for large area internal wave surveyingcompared to imagery from MODIS. Higher-resolution sen-sors like Landsat, SPOT and ASTER (Advanced Space-borne Thermal Emission and Reflection Radiometer) havesignificantly smaller swath widths (60–100 km) and cover acorrespondingly smaller portion of the world on a dailybasis. Wide area coverage instruments like AVHRR(Advanced Very High Resolution Radiometer) and DMSPcollect data at only 1 km and 4 km resolution respectively,from which only a limited number of very large internalwave signatures can be detected. A 500-m collection modefor DMSP provides nearly comparable sunglint imagery toMODIS but these data are not collected systematically on aworldwide basis and are not readily available.[11] The only sensors that approach the capabilities of

MODIS for large area detection and study of internal wavesinclude MERIS (MEdium-spectral Resolution, ImagingSpectrometer) with a 1150 km swath [Curran and Steele,2005] and the synthetic aperture radars on ENIVISAT andRADRSAT-1 while operating in their wide swath (orscanSAR) modes which have swath widths of 450 and500 km respectively. Also, while SAR is independent ofcloud cover and the reliance on a specific (near specular)imaging geometry, it does not acquire imagery in the samecontinuous, systematic near-global way acquired byMODIS.

3. MODIS Internal Wave Survey

[12] The previous work by Apel et al. [1975], Fett et al.[1979], and Sawyer [1983] using sunglint to study internalwaves motivated the examination of MODIS sunglintimagery to identify internal wave occurrences to supportthe development of an Atlas of Internal Solitary-like Waves[Jackson, 2004] (www.internalwaveatlas.com). The surveyrelied on MODIS true color images on the NASA MODISRapid Response System web site (rapidfire.sci.gsfc.nasa.gov) which posts daily, near-real-time imagery to supportactive fire detection [Descloitres et al., 2002]. Imagery onthe Rapid web site includes 20-km resolution thumbnailsthat were used to identify images that contained sunglintand direct links to the 250-m imagery allowed the finerresolution imagery to be examined relatively quickly. Whileit is possible to detect the internal wave signatures in 1-kmresolution images in a few areas of the world, the 250-mimagery was required to identify the majority of internalwave signatures found in the survey.[13] Beginning with August 2002, MODIS 250-m true-

color sunglint imagery were examined for internal wavepackets or isolated soliton signatures. Figure 1 shows thelocation of 3581 internal wave occurrences noted in theimagery during 21 months from 1 August 2002 through16 May 2004 (excluding January 2003). The survey wasdone entirely ‘‘by eye,’’ and did not count individual wavepackets but rather distinct regions of wave activity visible inany given image. For example, wave packets visible in aparticular image that were generated on subsequent phasesof the tide but which originated at the same location wereconsidered to be a single occurrence. The internal wave

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Figure

1.

Locationofinternal

waves

observed

inMODIS

imageryfrom

August2002throughMay

2004alongwiththe

geographicboundaryforthe15regionslisted

inTable1.T

hesurvey

identified

atotalnumberof3581waveoccurrenceswhich

combinetocreate2774distinctregion,area,anddateoccurrences.Well-knownoccurrence

sitesareshowningray,new

areas

ofactivityareshownin

red,andareasofgeographically

expanded

activityareshownin

blue.

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occurrences were noted on 589 of the 621 days examined.Although limited to times of light cloud cover and theproper location of the sunglint ellipse, it was found that upto a dozen internal wave occurrences could be identified ona given day. It should be noted, that NASA’s Rapid websiteis not a comprehensive archive of MODIS imagery and sothe survey represents a lower limit on the number of internalwaves detectable by MODIS over the survey period.[14] Table 1 presents a summary of the survey results for

the top 15 regions of wave activity, representing 76% of theinternal waves observed in the MODIS survey. The regionalbreak down was chosen to take into account both histori-cally reported locations of wave activity and to groupsimilar occurrences within a geographic area. Some regionstherefore have one or more or subregions of unique internalwave activity. Table 1 list the number of subregionscontained in each region along with the total number ofinternal waves observed over the region and the totalnumber of distinct region, subregion and occurrence datecombinations. The survey identified a total number of 3581wave occurrences which combine to create 2774 distinctregion, subregion and date occurrences.[15] In addition to their geographic delineation, the inter-

nal wave occurrences can be divided into three categoriesbased on how well the occurrences in a particular region/subregion have been previously studied. In the first categoryare regions where internal waves have been previouslyreported and their characteristics well documented. In thesecond category are regions where internal wave activityhas been reported, usually from in situ measurements orindividual remote sensing images (like an astronaut photo-graph), but the full extent of the activity (geographically ortemporally) and the characteristics of the waves have notbeen determined. In the third category are regions in which

the MODIS survey found a significant amount of internalwave activity where little or no activity had been previouslyreported. This categorization of wave types is reflected bythe colors in Figure 1 where waves from category 1 arepresented as dark gray, category 2 as blue and category 3 asred.[16] Figure 1 highlights that high-frequency nonlinear

waves are ubiquitous in many areas of the world. Thewaves are present throughout many of the marginal seas(Andaman, Sulu, Celebes as well as almost all the seas ofIndonesia), occupy much of the Equatorial Indian Ocean,are spread across the Central Atlantic (between Brazil andWest Africa) and cover a large area in Eastern EquatorialPacific (from the coast of Central America to south of theGalapagos Islands) with more localized occurrences in theeastern Caribbean, the Persian Gulf, south of Japan amongthe Bonin Islands and in the Tasman Sea west of NewZealand. Section 4 will discuss several of these areas indetail.[17] Figure 1 also highlights some of the limitations the of

the MODIS sunglint survey. In general, Figure 1 shows onlya limited number of internal wave detections over the deepocean. This is due to limitations on the imagery availablefrom the MODIS Rapid website and not limitations on thecoverage by the MODIS sensor. Unlike data from othersensors, MODIS imagery over the central ocean is residentin the Level 1 and Atmosphere Archive and DistributionSystem (LAADS) archive and can be processed and exam-ined to support internal wave detection in the open ocean.Figure 1 also shows that internal waves were only detectedbetween 45�S and 55�N, close to the maximal extent of thesunglint that occurs at the summer and winter solstices, (thetermination at 45�S is not due to sunglint limitations butdetectable internal wave activity). The variation in thelatitude of internal wave detections over the course of theyear is shown in Figure 2 and results from the shiftinglocation of the sunglint region. Figure 2 shows that sunglintportions of the MODIS imagery have the advantage of

Table 1. Top 15 Regions of High-Frequency Nonlinear Internal

Wave Activity Identified in the MODIS Sunglint Surveya

Region

Numberof

Subregions

Total Numberof IW

Occurrences

Total DistinctOccurrences (Region,Subregion, Date)

Indonesia 14 465 321South China Sea 8 278 252Western Equatorial Indian 1 324 202Pacific Central America 5 234 185Andaman Sea 3 231 164West Central Africa 3 192 147Sulu Sea 2 142 129Western EquatorialAtlantic

1 180 126

Eastern EquatorialIndian

1 123 97

Southwest Africa 2 110 85Australia-NW 1 112 80Eastern EquatorialPacific

1 104 78

Gulf of California 1 90 70Northwest SouthAmerica

1 83 55

Celebes Sea 1 69 50aThese regions represent 76% of the observed occurrences. The table

shows the number of subregions contained in each region along with thetotal number of internal waves observed in the region and the total numberof distinct region, subregion, and occurrence date combinations.

Figure 2. Latitude of internal wave observations observedin MODIS imagery as a function of day of year. The latituderange of detections follows the movement of the changinglocation of the sunglint pattern.

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Figure 3. True-color MODIS image of the Banda Sea acquired on 24 February 2004 at 5:05 UTC. Fourgroups of internal waves are visible in the central sea radiating from a generation point in the OmbaiStrait. Imaged area is approximately 450 km � 600 km.

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tracking in phase with the seasonal heating of the ocean’supper layer that provides the stratification necessary forinternal wave creation.

4. Internal Wave Occurrence Regions

[18] This section examines seven regions of significantnonlinear internal wave activity that were found duringthe MODIS survey. A image showing the wave signaturesin each region is presented along with a short descriptionof the wave characteristics that could be derived from theMODIS true-color imagery.

4.1. Indonesia

[19] The survey identified the largest number of waveoccurrences in the Indonesian Seas. Waves were noted in14 distinct subregions around Indonesia including the BaliSea, Banda Sea, Cream Sea, Flores Sea, Halmahera Sea,Molucca Sea, Savu Sea, the Sumba Strait and north andsouth of the Lombok Strait. The profusion of waves in thisregion is due to the large number of shallow interisland sillsthat separate deeper basins and which are accompanied by

the strong currents of the Indonesian throughflow betweenthe Pacific and Indian Oceans. The survey indicates thatwave occurrences take place all year round in the Indonesiaregion. Figure 3 is a true-color MODIS sunglint imageacquired on 24 February 2004 at 5:05 UTC that showsinternal wave signatures in the Banda Sea. Four groups ofsolitary-like internal waves are visible as dark bands againstthe silver-gray sunglint which covers almost the entire seasurface area visible in the image. The waves appear tooriginate in the Ombai Strait between the islands of Alorand Wetar and persist for more than 500 km into the BandaSea from their generation point. Modeling of the M2baroclinic tide in this area has shown that the Ombai Straithas some of the strongest internal tidal flow in Indonesia[Robertson and Ffield, 2005]. The strong current in com-bination with a small sill in the strait would cause thenecessary displacement of the pycnocline for the genera-tion of internal waves in a manner similar to that of theSulu Sea. A finer-scale packet of internal waves is alsovisible immediately north of Timor propagating eastward.Figure 3 is one of a pair of images collected over theBanda Sea on 24 February 2004. Figure 3 combined with

Figure 4. A contrast enhanced true-color MODIS image over the southwestern South China Seaacquired on 6 March 2003 at 3:20 UTC. More than ten internal wave packets are visible northeast of theNatuna Bessar Island. The packets are finescale (approximately 500 m wavelength) propagating primarilyto southwest and aligned with the local bathymetry are typical of continental shelf generated internalwaves. Imaged area is approximately 223 km � 223 km.

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its corresponding Terra image acquired at 2:15 UTC, indi-cates the waves propagated a distance of between 25 to 30 km(depending on the packet) with an average propagationvelocity for the leading soliton of between 2.5 and 3.0 m/s.

4.2. Southwestern South China Sea

[20] Internal wave occurrences have been well docu-mented in the northern portion of the South China Seabetween the Luzon Strait and the Dongsha Coral Reef [Hsuand Liu, 2000]. However, the MODIS survey also identifiedsignificant nonlinear internal wave activity all along thecoast of Vietnam and in the southwestern portion of theSouth China Sea on the continental shelf between Vietnamand Borneo. Figure 4 is a true-color MODIS sunglint imageacquired over the southwestern South China Sea on 6 March2003 at 3:20 UTC. More than ten internal wave packets arevisible northeast of Natuna Bessar Island. The packets arefinescale, approximately 500-m wavelength, propagatingprimarily to southwest and are aligned with the localbathymetry. The separation distance between packets of

25 to 30 km indicates a propagation speed of approximately0.6 m/s, assuming a semidiurnal generation period. Thecharacteristics of these wave signatures are typical ofcontinental shelf generated internal waves observed in otherareas of the world.

4.3. Celebes Sea

[21] The MODIS survey found significant internal waveactivity from February through December in the CelebesSea. The waves manifest themselves as isolated solitarywave fronts or as groups of 3 to 5 waves that propagateacross the sea to the southeast and the west. The southeastpropagating waves originate in (or near) the Sulu Archi-pelago and western propagating waves originate at theeastern edge of the sea, most likely near the Sangi Islands.Figure 5 is a true-color MODIS sunglint image acquiredover the Celebes Sea on 6 March 2006 at 5:25 UTCshowing both kinds of wave occurrences. Five groups ofinternal waves are visible in western half of the sea, twopropagating west toward Borneo, two propagating south-

Figure 5. True-color MODIS image of the Celebes Sea acquired on 6 March 2006 at 5:25 UTC. Fivegroups of internal waves are visible in western half of the sea, two propagating west toward Borneo, twowave groups propagating southeast toward Celebes, and the partial signature of a fifth group visibleimmediately adjacent to the coast of Celebes. Imaged area is approximately 555 km � 445 km.

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east toward Celebes and the partial signature of a fifthgroup is visible immediately adjacent to the coast ofCelebes. The separation distances between the leadingwaves suggest that both types are generated semidiurnallywith propagation velocities of approximately 3.0 m/sacross the deep basin.

4.4. Eastern Equatorial Indian Ocean

[22] The survey identified a significant amount of internalwave activity from February to November in the EasternEquatorial Indian Ocean between the Nicobar Islands andSri Lanka. Figure 6 is a true-color MODIS sunglint imageshowing the symmetric generation of internal waves aroundthe Nicobar Islands at the eastern edge of the Indian Ocean.The image was acquired on 6 April 2004 at 4:25 UTC andshows finescale internal waves with 500 to 800 m wave-length. Packets 1, 2 and 3 appear to the west of the islandsand these packets propagate across the eastern equatorialIndian Ocean and shoal near Sri Lanka. Packets 1 and 2 willeventually merge into a single packet similar to packet 3,which was generated on the previous tidal cycle. Theseparation distance between packets 2 and 3 of 90 km givesa propagation speed of approximately 2.0 m/s, assuming asemidiurnal generation period. The waves on the east sideof the islands (Packets 4 and 5) develop into the well-known

internal waves that propagate across the southern portion ofthe Andaman Sea.

4.5. West Central Africa

[23] The survey identified wave occurrences in threeareas off the Atlantic coast of Africa between the equatorand 20�N. Slightly more than half (54%) of the waveactivity occurred offshore as finescale waves from the areaof the Cape Verde Islands south to the Sierra Leone rise.The remaining wave activity was primarily shorewardpropagating continental shelf generated waves, concentratedon the wide shelf between 7�N to 15�N. However, thesurvey also identified 20 occurrences of seaward propagat-ing internal waves just south of this wide shelf area. Figure 7shows a true-color MODIS image acquired on 27 October2002 at 11:45 UTC containing these seaward propagatingwaves. Two distinct wave packets (1 and 2) are visible inthe upper right quadrant of the image propagating to thesouthwest. Near the image center is also the strong signatureof a packet (3) with 4 waves amid a large number of moreirregularly spaced wave signatures. The generation mecha-nism for these seaward propagating wave packets is not yetunderstood. A packet separation distance of 50 to 55 kmgives a propagation speed of approximately 1.1 m/s,assuming a semidiurnal generation period.

Figure 6. True-color MODIS image acquired on 6 April 2004 at 4:25 UTC showing the symmetricgeneration of internal waves around the Nicobar Islands. Packets on the west of the islands (1, 2, and 3)propagate across the eastern equatorial Indian Ocean and shoal near Sri Lanka. The packets on the eastside of the islands (packets 4 and 5) develop into the well-known internal waves in the southern part ofthe Andaman Sea. Imaged area is approximately 260 km � 165 km.

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4.6. Western Equatorial Atlantic

[24] Internal waves in the Atlantic Ocean near the mouthof the Amazon have been reported by Ivanov et al. [1993]and more recently by Brandt et al. [2002], who detectedthree large-amplitude internal solitary waves of unknownorigin propagating toward the north-northeast at 44�Wbetween 4.5�N and 6�N. The MODIS survey showed thatthe internal wave activity in this region extends over a widegeographic area (Figure 1) from at least March throughDecember.[25] Figure 8 is a true-color MODIS image acquired on

13 August 2003 at 16:05 UTC showing pulse-like internalsolitary wave signatures beginning approximately 500 kmfrom the mouth of the Amazon River and extending morethan 700 km into the Atlantic. Isolated wave fronts in thelower half of the image change into irregularly organizedpackets in the upper half. A reduced resolution MERISimage, acquired on 13 August 2003 at 13:21 UTC, containsthe signature of the southern most solitary wave visible inthe MODIS image and indicates the wave traveled approx-imately 33 km in the time between images yielding anaverage propagation speed of 3.3 m/s. This speed is

consistent with the separation distance of 135 km to the nextsolitary wave to the north given a semidiurnal generationperiod. The actual generation location and mechanism forlarge solitary waves in this region is still not known but theregularity in generation, and nearly year round occurrences ofthe waves points to a tidal origin.

4.7. Pacific Coast of Central America

[26] The survey revealed an unexpectedly large amountof finescale internal wave activity year round over a largearea from the Pacific coast of Central America extendingdown to the equator (Eastern Equatorial Pacific). Figure 9shows a true-color MODIS image acquired on 22 March2003 at 16:30 UTC that shows these finescale internalwaves signatures southwest of Central America. Visiblethroughout the image are packets of waves with wave-lengths between 600 and 1200 m propagating primarilynorthwest, parallel to the shore. Packet separation distancesare between 35 and 50 km which produce a propagationspeed of 0.8 to 1.2 m/s with semidiurnal generation. Thewave signatures in Figure 9 are located to the seaward sideof the continental shelf and cover a region with very little

Figure 7. True-color MODIS image seaward propagating waves off west central Africa acquired on27 October 2002 at 11:45 UTC. Two distinct wave packets (1 and 2) are visible in the upper rightquadrant of the image. Near the image center is also a strong signature of a packet (3) with four wavesamid more irregular signatures. Imaged area is approximately 230 km � 230 km.

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Figure 8. True-color MODIS image of the western equatorial Atlantic acquired 13 August 2004 at16:05 UTC. The image showing pulse-like internal solitary wave signatures beginning approximately500 km from the mouth of the Amazon River and extending more than 700 km into the Atlantic.Individual solitary waves in the lower half of the image change into irregularly organized packets in theupper half. Imaged area is approximately 555 km � 670 km.

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Figure 9. A contrast enhanced true-color MODIS image of the Pacific southwest of Central Americaacquired on 22 March 2003 at 16:30 UTC. Finescale internal waves signatures are visible throughout theimage two propagating toward the northwest. Imaged area is approximately 334 km � 556 km.

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topographic variation. It is not currently understood howsuch a large number of waves in the region are generated.

5. Applications for Internal Wave Field Studies

[27] The ability to collect large amounts of imagery overa region and to obtain both high temporal and spatialresolution data by combining data from Aqua and Terra,or combining MODIS imagery with imagery acquired fromMERIS and wide swath SAR imagery, has importantapplications for the study of internal wave field evolutionand the broader study of ocean characteristics.[28] Internal wave velocity is to first order determined by

the internal wave wavelength, the ocean depth and thedensity profile of the water column. By using pairs ofMODIS/MODIS, MODIS/MERIS or MODIS/SAR imagesseparated in time by only a few minutes to a few hours it ispossible to estimate the propagation speed of individualwave packets more accurately than by computing a velocityfrom the distance between packets with assumptions aboutgeneration time. With better internal wave velocity esti-mates, there are now new opportunities to use internal waveobservations to derive the ocean properties of mix layerdepth, Brunt-Vaisala frequency and heat storage originallyput forth by Li et al. [2000], Porter and Thompson [1999],Jones [1995] and Mollo-Christensen and Mascarenhas[1979].[29] The ability to collect large amounts of imagery over

a particular area of wave activity at many different phases ofthe tidal cycle and varying environmental conditions pro-vides another way to study internal wave field evolution andpotentially estimate changes in the water column character-istics. By building up a database of internal wave locationsthroughout the phases of the tidal cycle, it becomes possibleto estimate a ‘‘mean’’ propagation time (image acquisitiontime minus the wave generation time) to all points through-out the area of internal wave activity. This can be done byeither averaging the calculated propagation time at variouslocations throughout a region or by fitting a simple model(e.g., wave velocity as a function of depth) to the observa-tions. The difference between the mean travel times andobserved travel times can be analyzed via statistical meth-ods to determine if a particular factor (year, season, month,etc.) or combinations of factors produce a statisticallysignificant variation in travel time. Similarly, if a particularset of travel times can be associated with a set of environ-mental conditions, variations in the travel times can be usedto make an estimate of the required change in velocitywhich can then be used to determine changes in the oceanproperties.

6. Summary

[30] MODIS with its combined attributes of fine resolu-tion, large swath area, near-daily global coverage and readyimage access, has for the first time allowed sunglint to beused to survey internal solitary wave occurrences on a near-global scale. A survey of true-color MODIS imageryacquired between August 2002 through May 2004 found

3581 internal wave occurrences between 45�S and 55�N.The survey identified significant amounts of internal waveactivity in areas where little or no activity had beenpreviously reported in particular in the Indonesian Seas, inthe South China Sea along the coast of Vietnam and aroundthe Natuna Besar Islands, across the Central Atlantic(between Brazil and West Africa), in the Eastern EquatorialIndian Ocean (between the Nicobar Islands and Sri Lanka),and in Eastern Equatorial Pacific (from the coast of CentralAmerica to south of the Galapagos Islands).[31] The ability to use MODIS imagery, particularly in

combination with other sensors has important applicationsin the study of internal wave field evolution and the broaderstudy of ocean characteristics. By using pairs of imagesseparated in time by a few minutes to a few hours it ispossible to estimate the propagation speed of individualwave packets more accurately and then apply establishedtechniques to estimate oceanic mix layer depth or heatstorage.[32] The ability to use MODIS to compile a large data-

base of internal wave observations over a particular area ofwave activity provides another way to determine if aparticular factor (year, season, month, etc.) or combinationsof factors (each associated with a change in environmentalconditions) significantly effects internal wave propagationtimes in a region. Work on the examination of MODISimagery for internal wave signatures is ongoing.

[33] Acknowledgments. This work was supported by the Office ofNaval Research Physical Oceanography Program through contract N00014-03-C-0176. The author would also like to acknowledge the contributions ofGeorge Mason University graduate students Ritesh Gautam and DebabrartaGhoshal who assisted in the examination of the MODIS imagery. Theauthor would also like to thank Carl C. Gaither for his many usefuldiscussions. Note that the NASA MODIS Rapid Response System websiteannounced that effective 1 October 2007 all 250-m true color swath imagesolder than 30 days from the current date would be deleted and no longeravailable as part of the Rapid Real-Time archive.

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�����������������������C. Jackson, Global Ocean Associates, 6220 Jean Louise Way, Alexandria,

VA 22310, USA. ([email protected])

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