Ocean Sciences [OS]

OS34A  ACC:09   Wednesday

Ocean Remote Sensing II


Presiding: E J D'Sa, Louisiana State Univ., Baton Rouge; A Ignatov, NOAA, NESDIS/(STAR)

OS34A-01 INVITED  

Multi-sensor Satellite Analysis of Upper Ocean Response Before and After Coastally Trapped Disturbances

* Armstrong, E M (edward.m.armstrong@jpl.nasa.gov) AU: Holt, B (Benjamin.M.Holt@jpl.nasa.gov), Jet Propulsion Lab, California Institute of Technology, 4800 Oak Grove Dr MS 300/320, Pasadena, CA 91780, United States
Husson, R (husson@pacific.jpl.nasa.gov), Jet Propulsion Lab, California Institute of Technology, 4800 Oak Grove Dr MS 300/320, Pasadena, CA 91780, United States
Vazquez, J (jv@pacific.jpl.nasa.gov), Jet Propulsion Lab, California Institute of Technology, 4800 Oak Grove Dr MS 300/320, Pasadena, CA 91780, United States
Breaker, L (lbreaker@mlml.calstate.edu), Moss Landing Marine Laboratories, 8272 Moss Landing Road, Moss Landing, CA 95039, United States

Along the central California coast, periods of coastal upwelling forced by northerly winds may be followed by wind reversals that lead to cloud clearing periods that may last for several days. This study seeks to understand the upper ocean response between these periods of clear and cloudy conditions through use of multiple sensors including MODIS, which provides sea surface temperature and ocean color, and microwave imagery from synthetic aperture radar (SAR). Wide-swath SAR acquisitions were obtained from both RADARSAT1 and Envisat ASAR, along with MODIS and GOES imagery during such a wind reversal event that took place in early September 2005. We will discuss how the radar backscatter response is related to variations in temperature and ocean productivity and how the backscatter may be used to interpret the upper ocean changes during the wind reversal events. Quantitative comparisons and correlative relationships between the backscatter, and temperature and ocean color parameters will be presented.


OS34A-02  

Multi-Sensor Satellite Data Records for Climate Applications: Issues and Lessons Learned During Reanalysis of Historical AVHRR Data

* Trishchenko, A P (trichtch@ccrs.nrcan.gc.ca), Canada Centre for Remote Sensing, Natural Resources Canada, 588 Booth Str, Ottawa, Ont K1A 0Y7, Canada

The satellite observations are unique source of information about the ocean, surface and atmosphere. To be useful for climate studies, these data must be processed in the most accurate way to ensure consistency of long- time series. Although there are number of various satellite missions designed for climate applications, the optical data from medium resolution satellite sensors, such as Advanced Very High Resolution Radiometer (AVHRR) on NOAA platforms, play a central role. They deliver time series of the longest duration and global spatial coverage. The paper describes the efforts carried out at the Canada Centre for Remote Sensing (CCRS) on developing satellite data records suitable for climate applications. The archive of 25 years (since 1981) of observation from AVHRR/NOAA at 1-km spatial resolution, followed by MODerate Resolution Imaging Spectroradiometer (MODIS) on Terra platform at 250-m spatial resolution has been generated at CCRS over the large area of North America. Some critical issues were identified during re-analysis of AVHRR data. The consistency of radiometric calibration provided from various sources for all AVHRR sensors since AVHRR/NOAA-6 is analyzed. A calibration approach using the tropical deep convective clouds as the calibration target is described and evaluated. The uncertainties related to the choice of solar reference spectrum and sensor's spectral response functions are quantified. Details of newly designed cloud detection scheme are presented. It is emphasized that detection of cloud shadows should be an integral component of the scene identification process to identify truly clear-sky pixels. Some examples of long term trends in Western Arctic sea-ice extent, albedo and radiation will be discussed that demonstrate rate of climate change in high Arctic region. This work has been supported by the Canadian Space Agency under the Government Related Initiatives Program (GRIP) and the Earth Sciences Sector of the Department of Natural Resources Canada under the Program on "Enhancing Resilience in a Changing Climate".


OS34A-03 INVITED  

Progress and Pitfalls in Satellite Surveillance of Loop Current Frontal Eddy Cyclones

* Walker, N D (nwalker@lsu.edu), Dept. of Oceanography and Coastal Sciences, Louisiana State Universtiy, Baton Rouge, LA 70803, United States
Leben, R R (leben@colorado.edu), Colorado Center for Astrodynamics Research, University of Colorado, Boulder, CO 80309, United States
Anderson, S P (steve@horizonmarine.com), Horizon Marine Inc., 15 Creek Road, Marion, MA 02738, United States
Balasubramanian, S (sbalas1@lsu.edu), Earth Scan Laboratory, Coastal Studies Institute, Baton Rouge, LA 70803, United States

In the last decade, significant advances in active and passive remote sensing have transpired that are enabling researchers to better quantify and model time and space scales of ocean processes. This paper presents recent attempts to track the motion and development of rapidly propagating cyclonic mesoscale eddies along the outer margin of the Loop Current in the Gulf of Mexico. Recent research has shown the critical role that these features play in the intensification of surface currents and as trigger mechanisms for deep flows in oil and gas producing areas in the northern Gulf of Mexico. The rapid motion of these cyclonic frontal features (35 km/day) has made their study problematic. In this paper, we discuss the use of several remote sensing systems and the integration of data from these systems to better understand the behavior and impacts of the frontal eddy cyclones on Gulf circulation processes. Mid-infrared (3.5-3.9 micron) measurements from GOES GVAR, available in real-time every 15 minutes over the Gulf, provide an excellent source of "de-clouded" night-time surface temperature information, from which sea surface temperatures (SST) are estimated with daily updates (http:www.esl.lsu.edu). Measurements in this atmospheric window maximize the sampling frequency of ocean information in cloudy and humid ocean regions such as the Gulf of Mexico. On the other hand, satellite altimetry measurements provide the only remote sensing technique that directly measures a dynamical variable of ocean state - the sea surface height (SSH). Detection of mesoscale eddies has been improved by combining multi-mission measurements from TOPEX-Poseidon, ERS- 2, GFO, Jason-1 and Envisat into a gridded product, updated daily (http:argo.colorado.edu/~realtime/welcome). Ocean color sensors (SeaWiFS, MODIS, Oceansat-1 OCM) provide surface pigment information (chlorophyll a, CDOM) that can aid in the discrimination of Gulf features as cold core eddies contain more chlorophyll a, due to the upwelling of nutrients. In our attempt to characterize the behavior of these dynamic mesoscale features and their impacts on circulation, we present several case studies which showcase our progress as well as potential problems associated with these sensors. We present new results on air-sea interaction and hurricane intensity changes over Gulf eddies as well as the impacts of eddies on surface and sub-surface current accelerations in deep water.
http:www.esl.lsu.edu/research/


OS34A-04  

Multi-Year Optical Variability in the Northern Gulf of Mexico: Impact of Atmospheric and Oceanic Forcing

* Gould, R W (gould@nrlssc.navy.mil), Naval Research Laboratory, Code 7333, Stennis Space Center, MS 39529, United States
Green, R E (Rebecca.Green@nrlssc.navy.mil), Naval Research Laboratory, Code 7333, Stennis Space Center, MS 39529, United States
Martinolich, P M (martinol@nrlssc.navy.mil), Naval Research Laboratory, Code 7333, Stennis Space Center, MS 39529, United States
Smith, R D (regina@nrlssc.navy.mil), OTI, Code 7333, Stennis Space Center, MS 39529, United States
Townsend, T L (townsend@nrlssc.navy.mil), Naval Research Laboratory, Code 7323, Stennis Space Center, MS 39529, United States

One of the main advantages of a data base of archived satellite imagery is the ability to examine consistent products over several years, to assess long-term variability. The distributions of bio-optical properties are influenced by atmospheric and oceanic forcing through local and remote processes. We examine the impact of winds, waves, precipitation, and river discharge on coastal optical properties in the northern Gulf of Mexico, to assess the response of the optical fields to the forcing. We also couple the ocean color imagery with a numerical circulation model (HYCOM), with the ultimate goals of improving our understanding of the linkages between the physical forcing and the optical response, and providing a short-term predictive capability (1-3 day time scale) for ocean optics. We have assembled a complete 5-year data base of ocean color imagery (SeaWiFS, MODIS) covering the Gulf of Mexico (2001-2005). We have reprocessed all the imagery with consistent atmospheric correction and bio-optical algorithms to produce a full suite of optical products, including remote sensing reflectances, absorption (partitioned) and backscattering coefficients, chlorophyll concentration, total suspended sediment concentration (partitioned into organic and inorganic components), and new optical water mass classification images. We have also constructed data bases of winds (from buoys in the northern Gulf of Mexico), rainfall (from the TRMM satellite), and river discharge (USGS stream flow data) corresponding to the time period covered by the imagery. We present quantitative, statistical, time-series analyses to characterize the spatial/temporal changes in the water mass optical properties over time and how they relate to the physical forcing in the northern Gulf of Mexico. A frequency analysis using monthly optical water mass classification images provides an indication of the expected seasonal spatial distributions of optical water types. We also present examples of predicted optical fields (derived by coupling ocean color imagery with the numerical circulation model).


OS34A-05  

Global 9 km multi-satellite, multi-sensor sea surface temperatures from MODIS, AMSR-E, and TMI

* Gentemann, C L (gentemann@remss.com), Remote Sensing Systems, 438 First St, #200, Santa Rosa, CA 95401, United States
* Gentemann, C L (gentemann@remss.com), University of Miami - RSMAS, 4600 Rickenbacker Cswy, Miami, FL 33149, United States

Current global sea surface temperature (SST) datasets do not take full advantage of the numerous satellites and different sensors now retrieving SST. Existing operational SST products depend on a single sensor to produce global datasets. This results in a lower spatial and temporal resolution than what is possible with a multi satellite, multi sensor SST analysis. Initial efforts indicate that blending data from different sensors requires much more rigorous bias and error characterization than is necessary when only including data from a single sensor type. Therefore, creating a high-quality multi-sensor SST requires careful inter-calibration of different satellite sensors, calculation of sensor-specific observation errors that consider environmental variables, location of observation, and sensor calibration problems; and development of techniques for relating and combining measurements at different spatial resolutions and times of the day. A global daily 9 km optimally interpolated SST has been calculated from MODIS, AMSR-E and TMI SST data. Initial methodology, validation results, and future work will be discussed. This improved global daily SST should be useful for a wide range of scientific and operational activities.
http:www.misst.org


OS34A-06  

Oceanic Aerosol Network: A Maritime Component of AERONET

* Smirnov, A (asmirnov@ltpmail.gsfc.nasa.gov), Goddard Earth Sciences and Technology Center, UMBC, code 614.4, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, United States
Holben, B N (brent@ltpmail.gsfc.nasa.gov), code 614.4, NASA/Goddard Space Flight Center, Greenblet, MD 20771, United States
McClain, C R (chuck@seawifs.gsfc.nasa.gov), code 614.8, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, United States
Sakerin, S M (sms@iao.ru), Institute of Atmospheric Optics, SB RAS, Akademichesky, 1, Tomsk, Russian Federation
Smyth, T (tjsm@pml.ac.uk), Plymouth Marine Laboratory, Prospect Place, Plymouth, PL1 3DH, United Kingdom
Radionov, V F (vradion@aari.nw.ru), Arctic and Antarctic Research Institute, Beringa, 38, Saint Petersburg, Russian Federation
Zielinski, T (tymon@iopan.gda.pl), Institute of Oceanology, PAS, Powstancow Warszawy, 55, Sopot, Poland
Matarrese, R (raffaella.matarrese@ba.infn.it), University of Bari, via Amendola 173, Bari, 70126, Italy
Zibordi, G (giuseppe.zibordi@jrc.it), Institute for Environment and Sustainability, Joint Research Center, Ispra, 21020, Italy
Proshutinsky, A (aproshutinsky@whoi.edu), Woods Hole Oceanographic Institution, MS#29, WHOI, Woods Hole, MA 02543, United States
Robertson, L (lislrobertson@gmail.com), University of Cape Town, Department of Oceanography, RW James Building, Upper Campus, Cape Town, South Africa
Harvey, M (m.harvey@niwa.co.nz), National Institute of Water and Atmospheric Research, NIWA, P.O. Box 14-901, Kilbirnie, Wellington, New Zealand
Slutsker, I (ilya@ltpmail.gsfc.nasa.gov), Science Systems and Applications, Inc., code 614.4, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, United States
Giles, D (dgiles@ltpmail.gsfc.nasa.gov), Science Systems and Applications, Inc., code 614.4, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, United States
Tran, A (atran@pop600.gsfc.nasa.gov), Science Systems and Applications, Inc., code 614.4, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, United States

We suggest the establishment of the Oceanic Aerosol Network as a new component of the Aerosol Robotic Network (AERONET) that adheres to AERONET calibration and processing. Climate change studies, atmospheric correction of the satellite data, satellite data validation, and aerosol modeling creates a strong demand for new data acquisition. Ship-based measurements can at least partly fill the gap in our knowledge on the global aerosol distribution over the oceans and complement island-based AERONET sites. We plan to reestablish NASA's ship-based aerosol optical depth measurement network by deploying hand-held sun photometers on various ships of opportunity; developing an archival system, similar to the AERONET browser, but specifically designed for "moving" objects (i.e., ships); developing a calibration protocol; developing stand alone processing, utilizing AERONET's Version 2 algorithm; and developing a centralized archiving and distribution system allowing for public domain, web-based access. The suggested Oceanic Aerosol Network (AERONET - OAN) will provide important information for the Ocean Color community as well as global ocean and global climate studies.


OS34A-07  

Unusual blooms of Noctiluca miliaris in the Arabian Sea during the Northeast Monsoon

* Gomes, H d (hgomes@bigelow.org), Bigelow Laboratory for Ocean Sciences, 180 McKown Point Road, West Boothbay Harbor, ME 04575, United States
Goes, J I (jgoes@bigelow.org), Bigelow Laboratory for Ocean Sciences, 180 McKown Point Road, West Boothbay Harbor, ME 04575, United States
Matondkar, P (sgpm@nio.org), National Institute of Oceanography, Biological Oceanography Division, Dona Paula, Goa 403001, India
Parab, S (sushma@nio.org), National Institute of Oceanography, Biological Oceanography Division, Dona Paula, Goa 403001, India
Al-Azri, A R (adnazri@squ.edu.om), Dept. Marine Sciences & Fisheries, Sultan Qaboos University, Al-Khod, 123, Oman
Thoppil, P G (thoppil@nrlssc.navy.mil), Naval Research Laboratory, Code 7323, Stennis Space Centre, MS 39529, United States

Until the late 1990's Noctiluca miliaris Suriray (synonym Noctiluca scintillans Macartney), a large heterotrophic dinoflagellate was a minor component of phytoplankton populations in the Arabian Sea, appearing in bloom form only sporadically in coastal regions predisposed to upwelling and deep slope water intrusions during the Southwest monsoon. Since then however, N. miralis blooms have increased in frequency and intensity, but with the majority of blooms being observed following the Northeast monsoon (NEM) and at times, in association with the well known blooms of the diazotroph Trichodesmium sp. Microscopy and chemotaxonomy from HPLC analysis of phytoplankton pigments undertaken in 2003-2004. as well as satellite ocean color data suggest that N. miralis blooms are becoming more intense and widespread in the Arabian Sea. Large blooms of these organisms have started appearing in the Gulf of Oman and off the coast of Oman. This study uses recent, merged SeaWiFS and MODIS-Aqua ocean color datasets to investigate the temporal evolution and spatial extent of these taxonomically validated blooms. Aqua-MODIS SST and altimetry data suggest that mesoscale eddies that populate the Western Arabian Sea during the NEM may be playing a significant role in the production and dispersal of these blooms from the Gulf of Oman into the Central Arabian Sea.
http:www.bigelow.org/climatechange


OS34A-08  

A Multi-frequency Beam-forming HF Radar for Tsunami Detection

* Trizna, D B (dennis@isr-sensing.com), Imaging Science Research, Inc, 6103B Virgo Court, Bukre, VA 22015-3249, United States

We discuss a new multi-frequency beam-forming HF radar design for robust detection and tracking of tsunami waves from 200 km distances, providing continuous coverage of the tsunami wave pattern after it impinges on the continental shelf. The method works by mapping ocean currents at long range using traditional HF radar method of radial Bragg line Doppler shift measurements. The tsunami is detected by anomalous spatial patterns of higher than normal Bragg-line shifts due to the large orbital wave of the series of tsunami wave crests as they impinge on the continental shelf. An approach using beam forming of 16 or 32 antenna elements provides an update every five minutes or less, while Direction-of-Arrival method systems using just a few antenna elements inherently require of the order of 30 to 60 minutes for a reliable current map. The multi-frequency radar provides a more robust capability than the single frequency HF radar for at least two reasons. First, because the HF channel user spectrum suffers diurnal variability in channel occupancy due to the ionosphere changing with time of day, low frequencies can become contaminated with user noise, so that maximum range for reliable detection not achieved. Under this condition, one would rely on quiet higher HF frequencies that lie above the Maximum Usable Frequency (MUF) for ionospheric reflection propagation. Alternatively, for daylight operation when low frequency utilization can be used to minimize surface wave propagation loss, the sea state might not be sufficiently active to allow long range coverage needed for reliable detection, due to the lack of ocean wave spectral energy at the Bragg-resonant wave frequency. Thus, single- frequency radars, operating in the 4-6 MHz range to minimize propagation losses to achieve long-range coverage, would suffer due to low wind conditions. The multi-frequency HF radar discussed here allows one to dynamically choose the optimum frequency from a set of 8 to 16, as allowed by local radio frequency allocation authorities, assuming just a single frequency is used at a time. Alternatively, one may choose four to eight frequencies operating simultaneously, to allow the clearest channel and best signal strength channel for enhanced processing. We will discuss the tradeoffs on multiple frequency use versus single optimum frequency use, both using a multi-frequency radar capability. Results of preliminary testing of a prototype system at Duck, NC will also be presented.
http:www.isr-sensing.com