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Scientific and Technical Aerospace Reports Volume 39 April 6, 2001

Scientific and Technical Aerospace Reports Volume 39 April 6, 2001

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validate a methodology by which drag information from all available low-altitude space objects is used to update any given density<br />

model on a comprehensive basis. The basic update <strong>and</strong> prediction algorithms <strong>and</strong> a technique to estimate true ballistic factors are<br />

derived in detail. A full simulation capability is independently verified. The process is initially demonstrated using simulated<br />

range, azimuth, <strong>and</strong> elevation observations so that issues such as required number <strong>and</strong> types of calibration satellites, density of<br />

observations, <strong>and</strong> susceptibility to atmospheric conditions can be examined. Methods of forecasting the density correction models<br />

are also validated under different atmospheric conditions.<br />

DTIC<br />

Atmospheric Density; Atmospheric Models; Real Time Operation; Algorithms; Forecasting<br />

<strong>2001</strong>0024160 Colorado Univ., Physics Dept., Boulder, CO USA<br />

Aerosol <strong>and</strong> Plasma Measurements in Noctilucent Clouds Final Report, 1 Jun. 1997 - 30 Nov. 2000<br />

Robertson, Scott, Colorado Univ., USA; Nov. 30, 2000; 3p; In English<br />

Contract(s)/Grant(s): NAG5-4526; No Copyright; Avail: CASI; A01, Hardcopy; A01, Microfiche<br />

The purpose of this project was to develop rocket-borne probes to detect charged aerosol layers in the mesosphere. These<br />

include sporadic E layers, which have their origin in meteoric dust, <strong>and</strong> noctilucent clouds, which form in the arctic summer <strong>and</strong><br />

are composed of ice crystals. The probe being developed consists of a charge collecting patch connected to a sensitive electrometer<br />

which measures the charge deposited on the patch by impacting aerosols. The ambient electrons <strong>and</strong> light ions in the mesosphere<br />

are prevented from being collected by a magnetic field. The magnetic force causes these lighter particles to turn so that they miss<br />

the collecting patch.<br />

Author<br />

Noctilucent Clouds; Aerosols; Plasmas (Physics); Probes; Rocket-Borne Instruments; Rocket Launching<br />

<strong>2001</strong>0025272 NASA Goddard Space Flight Center, Greenbelt, MD USA<br />

Ozone in the Pacific Troposphere from Ozonesonde Observations<br />

Oltmans, S. J., National Oceanic <strong>and</strong> Atmospheric Administration, USA; Johnson, B. J., National Oceanic <strong>and</strong> Atmospheric Administration,<br />

USA; Harris, J. M., National Oceanic <strong>and</strong> Atmospheric Administration, USA; Voemel, H., National Oceanic <strong>and</strong> Atmospheric Administration,<br />

USA; Koshy, K., University of the South Pacific, Fiji; Simon, P., MeteoFrance, French Polynesia; Bendura, R., NASA Langley<br />

Research Center, USA; Thompson, A. M., NASA Goddard Space Flight Center, USA; Logan, J. A., Harvard Univ., USA; Hasebe, F., Ibaraki<br />

Univ., Japan; [2000]; 78p; In English; No Copyright; Avail: CASI; A05, Hardcopy; A01, Microfiche<br />

Ozone vertical profile measurements obtained from ozonesondes flown at Fiji, Samoa, Tahiti <strong>and</strong> the Galapagos are used to<br />

characterize ozone in the troposphere over the tropical Pacific. There is a significant seasonal variation at each of these sites. At<br />

sites in both the eastern <strong>and</strong> western Pacific, ozone is highest at almost all levels in the troposphere during the September-November<br />

season <strong>and</strong> lowest during, March-May. There is a relative maximum at all of the sites in the mid-troposphere during all seasons<br />

of the year (the largest amounts are usually found near the tropopause). This maximum is particularly pronounced during, the<br />

September-November season. On average, throughout the troposphere at all seasons, the Galapagos has larger ozone amounts than<br />

the western Pacific sites. A trajectory climatology is used to identify the major flow regimes that are associated with the characteristic<br />

ozone behavior at various altitudes <strong>and</strong> seasons. The enhanced ozone seen in the mid-troposphere during September-November<br />

is associated with flow from the continents. In the western Pacific this flow is usually from southern Africa (although 10-day<br />

trajectories do not always reach the continent), but also may come from Australia <strong>and</strong> Indonesia. In the Galapagos the ozone peak<br />

in the mid-troposphere is seen in flow from the South American continent <strong>and</strong> particularly from northern Brazil. The time of year<br />

<strong>and</strong> flow characteristics associated with the ozone mixing ratio peaks seen in both the western <strong>and</strong> eastern Pacific suggest that<br />

these enhanced ozone values result from biomass burning. In the upper troposphere low ozone amounts are seen with flow that<br />

originates in the convective western Pacific.<br />

Author<br />

Ozone; Troposphere; Observation; Annual Variations; Biomass Burning; Climatology; Flow Characteristics<br />

<strong>2001</strong>0025273 NASA Goddard Space Flight Center, Greenbelt, MD USA<br />

Radiative Properties of Cirrus Clouds in the Infrared (8-13 microns) Spectral Region<br />

Yang, Ping, <strong>Scientific</strong> Systems <strong>and</strong> Applications, Inc., USA; Gao, Bo-Cai, Naval Research Lab., USA; Baum, Bryan A., NASA<br />

Langley Research Center, USA; Hu, Yong X., NASA Langley Research Center, USA; Wiscombe, Warren J., NASA Goddard<br />

Space Flight Center, USA; Tsay, Si-Chee, NASA Goddard Space Flight Center, USA; Winker, Dave M., NASA Langley Research<br />

Center, USA; [2000]; 62p; In English; Original contains color illustrations<br />

Contract(s)/Grant(s): DE-AI02-00ER-62901; NASA Order S-97894-F; No Copyright; Avail: CASI; A04, Hardcopy; A01,<br />

Microfiche<br />

204

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