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relative to the previous reporting period (uptime increased to 93.7% from 91.6%). The Special Processing System (SPS) is still the major cause of the breaks in operation (75 out of 139), the longest one lasting for more than 4 days. Statistics from short sample intervals indicate that the number of Online detections average about 200 per day with the present threshold setting, while the On-line Event Processor processes about 25 events per day for transmission to the SDAC. The average number of analyst-retrieved and accepted events has been 10.8 per day during the period. GRA

N79-22687# Naval Ocean Systems Center, San Diego, Calif.
EXACT RAY PATHS IN A MULTISEGMENT QUASIPARA-
BOLIC IONOSPHERE. EQUATIONS FOR hF RAY PATHS
AID IN DISPLAYING PROPAGATION CONDITIONS FOR
REAL-TIME MINICOMPUTER-BASED ASSESSMENT
SYSTEMS Technical Report, Jun. 1977 - Jul. 1978
J. R. Hill 15 Sep. 1978 24 p

(AD-A063994; NOSC/TR-300) Avail: NTIS HC A02/MF A01 CSCL 20/14

Exact ray path calculations in a multiple quasiparabolic layer ionosphere are derived for use in mini- and microcomputer-based propagation assessment systems. Ionospheric profiles are modeled by quasiparabolic layers of two forms: normal layers having electron density maxima and valley layers having a minimum. Ray fans are displayed, demonstrating implementation of the equations on a minicomputer (SEL 810A) and a microcomputer (Tektronix 4051). The microcomputer program (in BASIC) used to calculate the single-layer propagation is included.

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The data analyzed was from an auroral rocket probe, AF 10.312, launched in 1974 from Poker Flats, Alaska. The instrumentation is described in an AF Geophysics Laboratory Technical Report AFCRL-TR-75-0023. The data were from both a low energy and high energy electron spectrometer, which measured fluxes at 1-100 eV and 1-20 KeV respectively. The rocket flight was north along a geomagnetic meridian, crossing the Harang discontinuity and several non optical auroral arcs. Data represents the first available electron flux measurements over such an extensive energy range (1 eV to 20 KeV) at an instant of time and for a number of altitudes. The flux distribution to the south of the discontinuity showed two 'bumps', one at 5 eV and the other at 4 KeV due to a lack of loss mechanisms at the lower energy and by the monoenergetic flux from space for the higher. The fluxes generally decreased with decreasing altitude as expected. No pitch angle dependence was discovered. South of the discontinuity peak fluxes were centered on 2 KeV. An order of magnitude increase in flux at energies less than 10 keV were measured while the discontinuity was crossed (rocket was at 165 Km). In the auroral arcs, the peak flux was at 7 KeV. Wave particle interactions were interpreted as the cause for the pattern of change with altitude of the greater than 1 KeV and less than 10 eV fluxes.

N79-22689# Texas Instruments, Inc., Dallas. Group.

Author (GRA)

Equipment

GEOPHYSICAL STUDIES FOR MISSILE BASING: SEISMIC
RISK STUDIES IN THE WESTERN UNITED STATES Final
Scientific Report, 1 Mar. 31 Oct. 1978
James C. Battis 20 Dec. 1978 96 p refs
(Contract F44620-76-C-0063; AF Proj. 2309)

(AD-A064798; TI-ALEX(02)-FSR-78-01; AFOSR-79-0038TR) Avail: NTIS HC A05/MF A01 CSCL 08/11

Seismic risk studies were conducted for two military facilities in the western United States: Luke Air Force Base, Arizona, and the Nevada Test Site(NTS). Both facilities are potential sites for MX missile system installations. For each site, peak around motion risk curves, for annual risks ranging between values of 1.0 and 0.001, were estimated, based on seismicity characteristics

of the risk regions surrounding each facility. Difficulties in evaluating the risk at NTS were caused by unannounced nuclear tests and induced seismic activity in the area of study. Composite design reponse spectra were generated for each site corresponding to various levels of annual risk to provide a representation of seismic risk in a form directly useful to the engineering community. Finally, the possible effects which might result from seismic activity on potenially active faults near each site were considered.

Author (GRA)

N79-22690# Ohio State Univ., Columbus. Dept. of Geodetic Science.

AN INVESTIGATION OF TWO MODELS FOR THE DEGREE VARIANCES OF GLOBAL COVARIANCE FUNCTIONS Interim Report

Christopher Jekeli Sep. 1978 80 p refs (Contract F19628-76-C-0010; AF Proj. 7600) (AD-A063196; DGS-275; AFGL-TR-78-0235; SR-18) Avail: NTIS HC A05/MF A01 CSCL 08/5

Degree variances of the covariance function for gravity anomalies are represented according to the two-component model suggested by Moritz in an attempt to arrive at a low horizontal gradient variance (200 E squared). The parameters of the model are determined through a least squares adjustment to data consisting of GEM 9 anomaly degree variances, as well as empirical point and mean anomaly variances. Results show that this model can accommodate the given point and mean anomaly variances and degree variances, while also yielding the desired low gradient variance. A comparison of this and a similar one-component model investigated by Tscherning and Rapp indicates that the latter cannot produce a low gradient variance together with a satisfactory fit to the data. Also, it does not adapt as well to the observed (GEM 9) attenuation of the anomaly degree variances. Author (GRA)

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The report surveys theoretical and experimental studies of ionospheric dynamics made during the contract period. Two major aspects of this topic were studied; the outflow of He(+) from the earth's ionosphere, and the effect of magnetospheric convection on the high latitude ionosphere. Model programs were written to study the general characteristics of the outflow of He(+) and also to make quantitative estimates of the escape flux of this ion. An existing model program for studying the effect of convection electric field on the F+region was updated and the N(+) ion was included in the model. Initial work was started to incorporate realistic convection trajectories in the model program. Experimental data from the S3-2 satellite was used to compare with theoretical predictions of both the variation of plasma density with perpendicular electric field and the onset of light ion outflow at high latitudes. While the light ion outflow showed good agreement with theory, the effects of perpendicular electric fields did not and provided further stimulus to incorporate the effect of convection trajectories in our ionospheric models. Author (GRA)

N79-22692# Computer Corp. of America, Cambridge, Mass. SIP ACCOMMODATION OF ADDITIONAL SEISMIC DATA SITES

Donald E. Eastlake, III 29 Jan. 1979 19 p refs (Contract N00039-78-C-0246; ARPA Order 3540) (AD-A064988; CCA-79-08) Avail: NTIS HC A02/MF A01 CSCL 08/11

The SIP is a dedicated minicomputer communications system developed and operated by Computer Corporation of America. It interfaces a real time seismic information network to the Datacomputer (DORIN and EASTLAKE). The Datacomputer is a network data utility designed to support very large databases and shared access by remote heterogeneous computers (MARTLL and STERN). It is the only operational general purpose database

system capable of handling datasets in excess of a trillion bits (CCA). GRA

N79-22693# Office of Science and Technology, Washington, D. C.

THE NATIONAL EARTHQUAKE HAZARDS REDUCTION PROGRAM

1978 32 p

(PB-291311/9) Avail: NTIS HC A03/MF A01

CSCL 05A The scope, limits and purpose are outlined for the National Earthquake Hazards Reduction Program formulated from the passage of the Earthquake Hazards Reduction Act of 1977. The bill charges the president with establishing such a program with both long and short run objectives. A reduction program is outlined, aimed at reducing the disaster potentialities and realities from earthquakes. The thesis centers around the conclusion that the proper balance between cost-effective hazard reduction programs and reconstruction relief must be ascertained so as to mitigate both the tragedy from the disaster and the unnecessary costs from poor planning. GRA

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(Contract EPA-68-02-1383) (PB-291842/3; EPA-906/9-78-002C) Avail: NTIS HC A05/MF A01 CSCL 04A

A statistical analysis of ozone concentrations in southern Louisiana is presented. The data used were collected at nine monitoring sites during a three-month period, July 17 October 17, in 1976. The factors which accompany high levels of ozone concentration and the observed relationships are described. The variables which influence the amount of ozone are discussed. The relationships between ozone concentration and a number of meteorological and spatial variables are explored. The relationships between ozone concentration and the concentrations of other pollutants are discussed.

N79-22695# Radian Corp., Austin, Tex.

GRA

RELATIONSHIP OF METEOROLOGY TO SUMMER OZONE IN SOUTHERN LOUISIANA

David L. Harper Sep. 1978 53 p refs (Contract EPA-68-02-1383)

(PB-290454/8; RAD-TN-100-195; EPA-906/9-78-002B) Avail: NTIS HC A04/MF A01 CSCL 13B

Continuous ozone data obtained at nine sites across southern Louisiana showed that the ozone levels frequently exceeded the federal standard of 80 parts per billion during the three month study period. The days with ozone over the standard were generally characterized as having light winds, abundant sunshine, and high temperatures. Intermittent periods of region wide low ozone were primarily associated with widespread thunderstorm activity. The cold fronts which passed through southern Louisiana during the study period were conducive to nighttime ozone levels which were higher than nighttime levels typically observed during the study period.

GRA

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The U.S. National Committee for Rock Mechanics, in the Assembly of Mathematical and Physical Sciences of the National Research Council, has served United Stated scientists and engineers concerned with rock-mechanics problems since 1967. This fourth periodic report for 1977 describes the work of the Committee and its Panels for calendar year 1977. The activities of the two Panels concerned with educational requirements and domestic/international activities are summarized. The last section of this report presents the findings and recommendations of the following three technical-study Panels, which were organized early in 1976 and completed their studies and reports in 1977: the

Panel on Rock Mechanics Problems That limit Energy Resources Recovery and Development; the Panel on Rock Mechanics Problems Related to Underground Construction and Tunneling: and the Panel on Rock Mechanics Problems Related to Seismology and Earthquake Engineering. GRA

N79-22697# Pennsylvania State Univ., University Park. for Research on Land and Water Resources. SOIL MORPHOLOGIC AND HYDRAULIC CHANGES ASSOCIATED WITH WASTEWATER IRRIGATION Research Project Technical Completion Report, 1 Jul. 1975 31 Dec. 1978

T. W. Simpson and R. L. Cunningham Nov. 1978 212 p refs (Contract DI-14-34-0001-8040)

(PB-291399/4; W79-02817; OWRT-A-045-PA(1)) Avail: NTIS HC A10/MF A01 CSCL 08M

Fifteen topographically matched pit transects were examined in treatment areas. Detailed profile descriptions and sketches were prepared for each transect. The morphologic data were quantified using a relative morphology rating scale developed to show differences in morphologic properties that could be related to hydraulic properties that had been significantly altered due to wastewater irrigation. This total score was used to establish suitability levels for sites based on the scores from the relative profile rating scale. Potential longevity of the site for wastewater irrigation was estimated using the average annual percentage of decrease in the relative profile rating score for all treatments, assuming a linear rate of change. U.S. EPA (1975) guidelines were used to make decisions on suitability using morphologic criteria. Morphologic properties such as mottling, soil structure and moist consistence have changed due to wastewater irrigation. The 118 and 231 cm per year treatment areas have been altered sufficiently so they are not suitable for irrigation. The 59 cm per year area was considered marginally suitable for continued wastewater irrigation. GRA

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A glacial silty clay was compacted in a field test pad to determine what variables control density and strength and their variabilities. Correlation was attempted to provide a prediction process for the field result. A procedure was identified by which quality assurance and design engineers can interpret and write compaction specifications that insure a desired field strength. Strength is controlled by water content, density, and incompactive effort. Dry density is controlled by water content, compactive effort, and the interaction between them. The quantitative influence of each constituent variable varied 'with type of equipment. Variabilities of both density and strength are significant. A procedure is presented for this soil which develops a computer tabulation of the variables to allow an estimate of field compacted strength knowing inspection test results. A procedure to allow the design engineer to directly determine his compaction specification to insure a desired strength and its variability is developed.

GRA

N79-22699# Arizona Univ., Tucson. Dept. of Geosciences. GRAVITY ANALYSIS OF THE SUBSURFACE STRUCTURE OF THE UPPER SANTA CRUZ VALLEY, SANTA CRUZ COUNTY, ARIZONA M.S. Thesis

Robert Wade Parker 1978 152 p refs (Contracts DI-14-34-0001-7005; DI-14-34-0001-7006; OWRT Proj. A-078-ARIZ(2))

(PB-291919/9; W79-03002) Avail: NTIS HC A08/MF A01 CSCL 08E

A gravity survey was conducted in the Upper Santa Cruz Valley, Santa Cruz County, Arizona. Residual gravity anomalies were interpreted to define the subsurface structure and to estimate the water resource potential. A north-south trending fault system with at least 2000 ft of vertical displacement forms the western half of the basin graben structure. The eastern basin boundary is a combination of northwest- and northeast-trending scarps.

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Avail:

Univ. Microfilms Order No. 7907695

A method was developed to increase the amount of climatic information obtained from observational records of climatic variables such as temperature, humidity, radiation, and wind that are only one or a few years long. The method relates the climatic variables at the observational site for each day of the record to the sea level and 500 mb atmospheric pressure fields over a large area surrounding the site. The climatic variables for days not in the record can then be estimated from the relatively long and reliable record of pressure data. The method relates conditions at the observational site to the pressure fields by assigning days to sets of circulation types, developed from eight years of pressure data by a SAHN centroid clustering technique; the short observational record provides estimates of mean conditions for the circulation types at the site.

Dissert. Abstr.

N79-22701 Pennsylvania State Univ., University Park. MEASUREMENT OF MICROMETEOROLOGICAL TEMPERATURE PROFILES BY THE INVERSION OF OPTICAL DATA Ph.D. Thesis

William Howard Mach 1978 115 p

Avail: Univ. Microfilms Order No. 7909099

Optical data containing the relative positions of an observer, a target and an image of the target are inverted with a set of nonlinear polynomial equations to obtain a temperature profile near the earth's surface. The temperature that is predicted at a specific height with the inversion of optical data is verified with a temperature that was measured with thermocouples when the optical data were collected. When the maximum uncertainty of + or - 0.04 C in the measured temperature is known, the largest difference between the measured temperature and the temperature obtained with the optical data is within + or 0.02 C. The inversion of optical data with these nonlinear polynomial equations produces a set of coefficients that is used to calculate the temperature profile. Dissert. Abstr.

N79-22702 State Univ. of New York at Albany. LABORATORY STUDIES OF THE SHAPES OF HAILSTONES Ph.D. Thesis

Steven Barry Newman 1978 65 p

Avail: Univ. Microfilms Order No. 7907221

Artificially produced hailstones of various diameters were suspended in the updraft of a small vertical wind tunnel and allowed to melt for time intervals up to five minutes. It is hypothesized that this melting is analogous to the wet growth phase of hailstones in supercooled clouds during the time when large accreted drops presumably form a layer of slowly freezing water on hail surfaces. It was observed that films of liquid water which accumulated on the hailstones surface served to mold and reshape the hailstone from its original shape. In clouds, the development of various shapes is believed to be the result of aerodynamic molding of the surface of the hailstone during the wet growth phase by a film of liquid water. The surface temperature of the stone rapidly comes to O C when covered

by such a film and the shape which develops is dependent on the terminal velocity of the stone. Dissert. Abstr.

N79-22703 Saint Louis Univ., Mo.

INFLUENCE OF PERTURBATION PRESSURE FORCES ON
THE MOVEMENT OF A MATURE, QUASI-STEADY, GREAT
PLAINS SUPERCELL THUNDERSTORM Ph.D. Thesis
Roger Carter Whiton 1978 207 p
Avail:

Univ. Microfilms Order No. 7908316

A three-dimensional model of a severe, rotating, Great Plains supercell thunderstorm in its steady state right- or left-moving stage was used to study the internal dynamics structure, and movement of a typical severe thunderstorm. Results indicate the jet-like inner core updraft of the model storm acts to a large extent as a fluid obstacle to the invading environmental air and is rather well protected from the effects of lateral entrainment. The storm has two updrafts: a primary updraft at the core attributable entirely to the Rankine combined vortex, and a secondary updraft induced by dynamical interaction between the storm's core and its environment. The secondary, dynamically induced updraft of a cyclonically rotating storm is in the right-front quadrant of right-moving storms and in the left-front quadrant of left-movers. The magnitude of the dynamically induced up- and downdrafts in the model is controlled by the vertical shear of the horizontal environmental winds relative to the storm. Dissert. Abstr.

N79-22704*# Pennsylvania State Univ., University Park. Dept. of Meteorology.

VERTICAL MOTIONS IN THE EQUATORIAL MIDDLE ATMOSPHERE Final Report

Morris Larry Weisman Washington NASA Apr. 1979 121 p refs

(Contract NAS6-2726)

(NASA-CR-3096) Avail: NTIS HC A06/MF A01 CSCL 04B A single station vertical velocity equation which considers ageostrophic and diabatic effects derived from the first law of thermodynamics and a generalized thermal wind relation is presented. An analysis and verification procedure which accounts for measurement and calculation errors as well as time and space continuity arguments and theoretical predictions are described. Vertical velocities are calculated at every kilometer between 25 and 60 km and for approximately every three hours for the above diurnal period at Kourou (French Guiana), Fort Sherman (Panama Canal Zone), Ascension Island, Antigua (British West Indies) and Natal (Brazil). The results, plotted as time series cross sections, suggest vertical motions ranging in magnitude from 1 or 2 cm/sec at 30 km to as much as 15 cm/sec at 60 km. Many of the general features of the results agree well with atmospheric tidal predictions but many particular features suggest that both smaller time scale gravity waves (periods less than 6 hours) and synoptic type waves (periods greater than 1 day) may be interacting significantly with the tidal fields. The results suggest that vertical motions can be calculated for the equatorial middle atmosphere and must be considered a significant part of the motion for time scales from 8 to 24 hours. Author

N79-22705*# Pennsylvania State Univ., University Park. Dept. of Meteorology.

MESOSPHERIC HEATING DUE TO INTENSE TROPOSPHERIC CONVECTION Final Report

Lauren Ludlum Taylor Washington NASA Apr. 1979 62 p refs

(Contract NAS6-2818)

(NASA-CR-3132) Avail: NTIS HC A04/MF A01 CSCL 04B A series of rocket measurements made twice daily at Wallops Island, Va., revealed a rapid heating of the mesosphere on the order of 10 K on days when thunderstorms or squall lines were in the area. This heating is explained as the result of frictional dissipation of vertically propagating internal gravity waves generated by intense tropospheric convection. Ray-tracing theory is used to determine the spectrum of gravity wave groups that actually reach mesospheric heights. This knowledge is used in an equation describing the spectral energy density of a penetrative convective element to calculate the fraction of the total energy initially available to excite those waves that do reach the level of heating. This value, converted into a vertical velocity, is used as the lower boundary condition for a multilayer

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A computer model to predict the frost formation process on a flat plate was developed for application to most environmental conditions under which frost occurs. The model was analytically based on a generalized frost thermal conductivity expression, on frost density and thickness rate equations, and on modified heat and mass transfer coefficients designed to fit the available experimental data. The broad experimental ranges reflected by the extremes in ambient humidities, wall temperatures, and convective flow properties in the various publications which were examined served to severely test the flexibility of the model. An efficient numerical integration scheme was developed to solve for the frost surface temperature, density, and thickness under the changing environmental conditions. The comparison of results with experimental data was very encouraging. Author

N79-22707*# TRW Systems and Energy, Redondo Beach, Calif. ANALYTIC STUDIES ON SATELLITE DETECTION OF SEVERE, TWO-CELL TORNADOES Final Report

George F. Carrier (TRW Systems and Energy, Redondo Beach, Calif.), Paul Dergarabedian (TRW Systems and Energy, Redondo Beach, Calif.), and Francis E. Fendell (TRW Systems and Energy, Redondo Beach, Calif.) Washington NASA Apr. 1979 71 p refs

(Contract NAS1-14578)

(NASA-CR-3127) Avail: NTIS HC A04/MF A01 CSCL 04B From funnel-cloud-length interpretation, the severe tornado is characterized by peak swirl speed relative to the axis of rotation of about 90 m/s. Thermohydrodynamic achievement of the pressure deficit from ambient necessary to sustain such swirls requires that a dry, compressionally heated, non-rotating downdraft of initially tropopause-level air lie within an annulus of rapidly swirling, originally low-level air ascending on a near-moistadiabatic locus of thermodynamic states. The two-cell structure furnishes an observable parameter possibly accessible to a passively instrumented, geosynchronous meteorological satellite with mesoscale resolution, for early detection of a severe tornado. Accordingly, the low-level turnaround region, in which the surface inflow layer separates to become a free ascending layer and for which inviscid modeling suffices, is examined quantitatively. Preliminary results indicate that swirl overshoot, i.e., swirl speeds in the turnaround region in excess of the maximum achieved in the potential vortex, is modest. Author

N79-22708*# National Aeronautics and Space Administration. Goddard Space Flight Center, Greenbelt, Md.

RF RADIATION PRODUCED BY INTRACLOUD LIGHTNING DISCHARGES

D. M. LeVine, E. P. Krider, and C. D. Weidman Apr. 1979 17 p refs

(NASA-TP-1454; G-7951-03) Avail: NTIS HC A02/MF A01 CSCL 04B

The RF radiation produced during intracloud lightning flashes is presented, together with associated fast and slow electric field changes. These data were collected during the Thunderstorm Research International Project in Florida during the summer of 1977. The RF radiation is essentially simultaneous with the fast-field change but has a tendency to peak during the initial half-cycle of the bipolar field changes associated cloud processes. This is in marked contrast to previous observations of RF radiation during return strokes in cloud-to-ground discharges and provides a clue to the physics of the intracloud discharge.

Author

N79-22709*# National Aeronautics and Space Administration.
Langley Research Center, Hampton, Va.
ANALYSES OF EARTH RADIATION BUDGET DATA FROM
UNRESTRICTED BROADBAND RADIO METERS ON THE
ESSA 7 SATELLITE

William L. Weaver and Frederick B. House (Drexel Univ.) May 1979 56 p refs

(NASA-TP-1402; L-12587) Avail: NTIS HC A04/MF A01 CSCL 04B

Six months of data from the wide-field-of-view low resolution infrared radiometers on the Environmental Science Services Administration (ESSA) 7 satellite were analyzed. Earth emitted and earth reflected irradiances were computed at satellite altitude using data from a new in-flight calibration technique. Flux densitites and albedos were computed for the top of the earth's atmosphere. Monthly averages of these quantities over 100 latitude zones, each hemisphere, and the globe are presented for each month analyzed, and global distributions are presented for typical months. Emitted flux densities are generally lower and albedos higher than those of previous studies. This may be due, in part, to the fact that the ESSA 7 satellite was in a 3 p.m. Sun-synchronous orbit and some of the comparison data were obtained from satellites in 12 noon sun-synchronous orbits. The ESSA 7 detectors seem to smooth out spatial flux density variations more than scanning radiometers or wide-field-of-view fixed-plate detectors. Significant longitudinal and latitudinal variations of emitted flux density and albedo were identified in the tropics in a zone extending about + or - 25 deg in latitude. Author

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lengths, pulse shapes, pulse lengths, and flux intensities. The predicted densities are compared with the criteria for triggering lightning. A conclusion is drawn that the triggering of lightning with a laser pulse is feasible from the standpoint of the physics involved; but would require large laser apertures, short pulse lengths, and flux intensities at the aperture near the threshold for the breakdown of air. Author (GRA)

N79-22713# Air Force Geophysics Lab., Hanscom AFB, Mass. CIRRUS PARTICLE DISTRIBUTION STUDY, PART 2 Air Force Surveys in Geophysics

D. J. Varley 10 Oct. 1978 104 p refs (AD-A063807; AFGL-TR-78-0248-Pt-2; AFGL-AFSG-399) Avail: NTIS HC A06/MF A01 CSCL 04/2

This report presents particle spectrometer data obtained by the AFGL instrumented MC-130E aircraft during a flight through various types of cirriform clouds in the Albuquerque area on 26 February 1978. The data consist of average particle concentration figures as a function of size for consecutive 30-sec periods during the 96-min sampling mission. Additionally, data for some particular 15-sec segments of the flight are closely examined. These segments, selected to represent various cirriform conditions, as dense cirrostratus and thin cirrus, are documented with aircraft nose camera photographs of clouds and with plots of resulting particle concentrations and calculations of liquid water content. Author (GRA)

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Naval Weather Service Detachment, Asheville, SUMMARY OF SYNOPTIC METEOROLOGICAL OBSERVATIONS (SSMO) SOUTH AMERICA AND SELECTED ISLAND COASTAL MARINE AREAS WEST COAST. VOLUME 5: AREA 31, MOLLENDO; AREA 32, LIMA; AREA 33, PUNTA NEGRA; AREA 34, GUAYAQUIL; AREA 35, BUENAVENTURA SW; AREA 36, GULF OF PANAMA; AREA 37, GALAPAGOS ISLANDS

Feb. 1979 480 p

(AD-A064337) Avail: NTIS HC A21/MF A01 CSCL 04/2

This report presents marine climatological data for specific coastal areas in 21 different tables including weather occurrence, wind direction and speed, cloud amount, ceiling height, visibility, precipitation, dry bulb, relative humidity, air-sea temperature difference, sea height and period, sea surface temperature and sea level pressure. Author (GRA)

N79-22720# Naval Weather Service Detachment, Asheville,

N.C.

SUMMARY OF METEOROLOGICAL OBSERVATIONS, SURFACE (SMOS) ROOSEVELT ROADS, PUERTO RICO Reference Report, 1948 - 1977

Jul. 1978 356 p

(AD-A063835) Avail: NTIS HC A16/MF A01 CSCL 04/2 This data report consists of a six part statistical summary of surface weather observations. The six parts are: Part 1 Weather Conditions/Atmospheric Phenomena, Part 2 Precipitation/Snowfall/Snow Depth, Part 3 - Surface Winds, Part 4 -Ceiling versus Visibility/Sky Cover, Part 5 Psychrometric Summaries, and Part 6 Station Pressure/Sea Level Pressure. Author (GRA) N79-22721# Naval Weather Service Detachment, Asheville, SUMMARY OF SYNOPTIC METEOROLOGICAL OBSERVATIONS (SSMO), SOUTH AMERICA AND SELECTED ISLAND COASTAL MARINE AREAS, WEST COAST. VOLUME 4. AREA 25-MAGELLAN STRAIT WEST, AREA 26-GULF OF PENAS, AREA 27-VALDIVIA, AREA 28-VALPARAISO, AREA 29-COQUIMBO, AREA 30-ANTOFAGASTA Feb. 1979 486 p

N.C.

(AD-A064027) Avail: NTIS HC A21/MF A01 CSCL 04/2 This report presents marine climatological data for specific coastal areas in 21 different tables including weather occurrence, wind direction and speed, cloud amount, ceiling height, visibility, precipitation, dry bulb, relative humidity, air-sea temperature difference, sea height and period, sea surface temperature and sea level pressure. Author (GRA)

N79-22722# Naval Weather Service Detachment, Asheville,

N.C.

SUMMARY OF METEOROLOGICAL OBSERVATIONS, SURFACE (SMOS) BARBERS POINT, HAWAII Reference Report, 1949 - 1977

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