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Dive into the research topics where Paul S. Chang is active.

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Featured researches published by Paul S. Chang.


IEEE Transactions on Geoscience and Remote Sensing | 2004

The WindSat spaceborne polarimetric microwave radiometer: sensor description and early orbit performance

Peter W. Gaiser; K.M. St Germain; Elizabeth M. Twarog; Gene A. Poe; W. Purdy; D. Richardson; W. Grossman; W.L. Jones; D. Spencer; G. Golba; J. Cleveland; L. Choy; R.M. Bevilacqua; Paul S. Chang

The global ocean surface wind vector is a key parameter for short-term weather forecasting, the issuing of timely weather warnings, and the gathering of general climatological data. In addition, it affects a broad range of naval missions, including strategic ship movement and positioning, aircraft carrier operations, aircraft deployment, effective weapons use, underway replenishment, and littoral operations. WindSat is a satellite-based multifrequency polarimetric microwave radiometer developed by the Naval Research Laboratory for the U.S. Navy and the National Polar-orbiting Operational Environmental Satellite System Integrated Program Office. It is designed to demonstrate the capability of polarimetric microwave radiometry to measure the ocean surface wind vector from space. The sensor provides risk reduction for the development of the Conical Microwave Imager Sounder, which is planned to provide wind vector data operationally starting in 2010. WindSat is the primary payload on the Department of Defense Coriolis satellite, which was launched on January 6, 2003. It is in an 840-km circular sun-synchronous orbit. The WindSat payload is performing well and is currently undergoing rigorous calibration and validation to verify mission success.


IEEE Transactions on Geoscience and Remote Sensing | 2004

A preliminary survey of radio-frequency interference over the U.S. in Aqua AMSR-E data

Li Li; Eni G. Njoku; Eastwood Im; Paul S. Chang; K.M. St Germain

A spectral difference method is used to quantify the magnitude and extent of radio-frequency interference (RFI) observed over the United States in the Aqua AMSR-E radiometer channels. A survey using data from the AMSR-E instrument launched in May 2002 shows the interference to be widespread in the C-band (6.9 GHz) channels. The RFI is located mostly, but not always, near large highly populated urban areas. The locations of interference are persistent in time, but the magnitudes show temporal and directional variability. Strong and moderate RFI can be identified relatively easily using an RFI index derived from the spectral difference between the 6.9- and 10.7-GHz channels. Weak RFI is difficult to distinguish, however, from natural geophysical variability. These findings have implications for future microwave sensing at C-band, particularly over land areas. An innovative concept for radiometer system design is also discussed as a possible mitigation approach.


Journal of Geophysical Research | 1999

Revised ocean backscatter models at C and Ku band under high-wind conditions

William J. Donnelly; James R. Carswell; Robert E. McIntosh; Paul S. Chang; John Wilkerson; Frank D. Marks; Peter G. Black

A series of airborne scatterometer experiments designed to collect C and Ku band ocean backscatter data in regions of high ocean surface winds has recently been completed. More than 100 hours of data were collected using the University of Massachusetts C and Ku band scatterometers, CSCAT and KUSCAT. These instruments measure the full azimuthal normalized radar cross section (NRCS) of a common surface area of the ocean simultaneously at four incidence angles. Our results demonstrate limitations of the current empirical models, C band geophysical model function 4 (CMOD4), SeaSat scatterometer 2 (SASS 2), and NASA scatterometer 1 (NSCAT) 1, that relate ocean backscatter to the near-surface wind at high wind speeds. The discussion focuses on winds in excess of 15 m s−1 in clear atmospheric conditions. The scatterometer data are collocated with measurements from ocean data buoys and Global Positioning System dropsondes, and a Fourier analysis is performed as a function of wind regime. A three-term Fourier series is fit to the backscatter data, and a revised set of coefficients is tabulated. These revised models, CMOD4HW and KUSCAT 1, are the basis for a discussion of the NRCS at high wind speeds. Our scatterometer data show a clear overprediction of the derived NRCS response to high winds based on the CMOD4, SASS 2, and NSCAT 1 models. Furthermore, saturation of the NRCS response begins to occur above 15 m s−1. Sensitivity of the upwind and crosswind response is discussed with implications toward high wind speed retrieval.


Geophysical Research Letters | 2001

QuikSCAT's sea winds facilitates early identification of tropical depressions in 1999 hurricane season

Kristina B. Katsaros; Evan B. Forde; Paul S. Chang; W. Timothy Liu

Far from land and surface ship observations, most tropical depressions are identified by examining images from geostationary satellites for the presence of rotation of the convective cloud masses. During the 1999 hurricane season, surface wind vectors obtained by the SeaWinds scatterometer on the QuikSCAT satellite for the tropical Atlantic and Caribbean Sea were examined to test the hypothesis that developing tropical depressions (TDs) could be observed with this satellite sensor, before identification by the traditional means. QuikSCAT was able to detect the presence of closed circulation in the surface winds before the systems were designated as depressions. The satellites unprecedented large swath width of 1800 km allows twice a day observation of most of the tropical oceans. SeaWinds data can, therefore, provide valuable guidance that are an important addition to the tools available to the tropical cyclone forecasting community.


Weather and Forecasting | 2006

Operational Impact of QuikSCAT Winds at the NOAA Ocean Prediction Center

Joan M. Von Ahn; Joseph Sienkiewicz; Paul S. Chang

Abstract The NASA Quick Scatterometer (QuikSCAT) has revolutionized the analysis and short-term forecasting of winds over the oceans at the NOAA Ocean Prediction Center (OPC). The success of QuikSCAT in OPC operations is due to the wide 1800-km swath width, large retrievable wind speed range (0 to in excess of 30 m s−1), ability to view QuikSCAT winds in a comprehensive form in operational workstations, and reliable near-real-time delivery of data. Prior to QuikSCAT, marine forecasters at the OPC made warning and forecast decisions over vast ocean areas based on a limited number of conventional observations or on the satellite presentation of a storm system. Today, QuikSCAT winds are a heavily used tool by OPC forecasters. Approximately 10% of all short-term wind warning decisions by the OPC are based on QuikSCAT winds. When QuikSCAT is available, 50%–68% of all weather features on OPC surface analyses are placed using QuikSCAT. QuikSCAT is the first remote sensing instrument that can consistently disting...


Bulletin of the American Meteorological Society | 2016

New Ocean Winds Satellite Mission to Probe Hurricanes and Tropical Convection

Christopher S. Ruf; Robert Atlas; Paul S. Chang; Maria Paola Clarizia; James L. Garrison; Scott Gleason; Stephen J. Katzberg; Zorana Jelenak; Joel T. Johnson; Sharanya J. Majumdar; Andrew O'Brien; Derek J. Posselt; Aaron J. Ridley; Randall Rose; Valery U. Zavorotny

AbstractThe Cyclone Global Navigation Satellite System (CYGNSS) is a new NASA earth science mission scheduled to be launched in 2016 that focuses on tropical cyclones (TCs) and tropical convection. The mission’s two primary objectives are the measurement of ocean surface wind speed with sufficient temporal resolution to resolve short-time-scale processes such as the rapid intensification phase of TC development and the ability of the surface measurements to penetrate through the extremely high precipitation rates typically encountered in the TC inner core. The mission’s goal is to support significant improvements in our ability to forecast TC track, intensity, and storm surge through better observations and, ultimately, better understanding of inner-core processes. CYGNSS meets its temporal sampling objective by deploying a constellation of eight satellites. Its ability to see through heavy precipitation is enabled by its operation as a bistatic radar using low-frequency GPS signals. The mission will depl...


IEEE Transactions on Geoscience and Remote Sensing | 2004

Retrieving ocean surface wind speed from the TRMM Precipitation Radar measurements

Li Li; Eastwood Im; Laurence N. Connor; Paul S. Chang

Spaceborne scatterometery has been used for many years now to retrieve the ocean surface wind field from normalized radar cross-section measurements of the ocean surface. Though designed specifically for the measurement of precipitation profiles in the atmosphere, the Precipitation Radar (PR) of the Tropical Rainfall Measuring Mission (TRMM) also acquires surface backscattering measurements of the global oceans. As such, this instrument provides an interesting opportunity to explore the benefits and pitfalls of alternative radar configurations in the satellite remote sensing of ocean winds. In this paper, a technique was developed for retrieving ocean surface winds using surface backscattering measurements from the TRMM PR. The wind retrieval algorithm developed for TRMM PR makes use of a maximum-likelihood estimation technique to compensate for the low backscattering associated with the PR configuration. The high vertical resolution of the PR serves to filter-out rain-contaminated cells normally integrated into Ku-band scatterometer measurements. The algorithm was validated through comparisons of ocean surface wind speeds derived from PR with remotely measured winds from TMI and QuikSCAT, as well as in situ observations from oceanographic buoys, revealing good agreements in wind speed estimations.


IEEE Transactions on Geoscience and Remote Sensing | 2000

Ocean surface wind retrievals using the TRMM microwave imager

Laurence N. Connor; Paul S. Chang

An analysis of one year of brightness temperature data from the TRMM microwave imager (TMI) is presented with regard to the retrieval of ocean surface wind speeds using standard regression techniques with in situ meteorological buoy measurements. Comparisons to similar satellite radiometer data from the special sensor microwave/imager (SSM/I) are also presented to help quantify atmospheric contributions to the surface wind retrievals. Particular emphasis is placed upon the use of the 10.7 GHz channels aboard the TMI in overcoming the contamination in the ocean surface brightness temperature measurements caused by precipitation and water vapor in the propagation path. The resulting wind retrieval improvements permit a relaxation in the rain flag definitions used to determine precipitation interference cutoff criteria, allowing accurate wind speed retrievals over a wider range of precipitation conditions. These improvements are realized through the construction of a new D-matrix wind speed retrieval algorithm suitable for the middle and low latitude coverage provided by the TRMM orbit.


Journal of Marine Systems | 2002

Geostationary satellites reveal motions of ocean surface fronts

Richard Legeckis; Chris W. Brown; Paul S. Chang

A new method of locating and viewing ocean surface fronts is demonstrated in animations of daily composites of hourly sea surface temperatures derived from the NOAA Geostationary Operational Environmental Satellites (GOES). The animation of the satellite images allows the human eye to separate the faster-moving residual clouds from slower-moving ocean currents, fronts and eddies. The animations produce the sense of an ocean in motion that is not apparent in individual satellite images. Three years of GOES animations of sea surface temperatures of the Atlantic and Pacific Oceans are used to illustrate the westward propagation of Pacific Tropical Instability Waves (TIW) during La Nina, the seaward deflection of the Gulf Stream at the Charleston Bump, a time series of the Loop Current and separation of six warm core eddies in the Gulf of Mexico, and the cyclonic eddies and westward-moving meridional fronts near the Hawaiian Islands.


IEEE Transactions on Antennas and Propagation | 1996

Polarimetric backscatter from fresh and metamorphic snowcover at millimeter wavelengths

Paul S. Chang; James B. Mead; E.J. Knapp; G.A. Sadowy; R.E. Davis; Robert E. McIntosh

This paper presents 35, 95, and 225 GHz polarimetric radar backscatter data from snowcover. It compares measured backscatter data with detailed in situ measurements of the snowcover including microstructural anisotropies within the snowpack. Observations of backscatter mere made during melt-freeze cycles, and measurable differences in the normalized radar cross section between older metamorphic snow and fresh low-density snow were observed. In addition, these data show that the average phase difference between the copolarized terms of the scattering matrix, S/sub vv/and S/sub hh/, is nonzero for certain snow types. This phase difference was found to be related to snowpack features including anisotropy, wetness, density, and particle size. A simple backscatter model based on measured particle size and anisotropy is found to predict the Mueller matrix for dry snowcover with reasonable accuracy.

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Zorana Jelenak

National Oceanic and Atmospheric Administration

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James R. Carswell

University of Massachusetts Amherst

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Stephen J. Frasier

University of Massachusetts Amherst

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Seubson Soisuvarn

National Oceanic and Atmospheric Administration

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Peter G. Black

National Oceanic and Atmospheric Administration

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Frank D. Marks

Atlantic Oceanographic and Meteorological Laboratory

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Laurence N. Connor

National Oceanic and Atmospheric Administration

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Robert E. McIntosh

University of Massachusetts Amherst

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Faozi Said

National Oceanic and Atmospheric Administration

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David J. McLaughlin

University of Massachusetts Amherst

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