chapter 5 observing the atmosphere atmo 1300 spring 2010

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Chapter 5 Chapter 5 Observing the Observing the Atmosphere Atmosphere ATMO 1300 SPRING 2010

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Page 1: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Chapter 5Chapter 5Observing the Observing the AtmosphereAtmosphere

ATMO 1300SPRING 2010

Page 2: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Two Types of Two Types of MeasurementsMeasurements

• Direct Methods– Taken in place,

instruments in direct contact with atmospheric property you are trying to measure

• Indirect Methods– Atmospheric properties

measured from a distance (i.e., no direct contact).

– Also referred to as remote sensing.

Page 3: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Direct MeasurementsDirect Measurements

• Automated Surface Observing System (ASOS) – Typically located at airports

Page 4: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Automated Surface Observing System(ASOS)

Over 600 ASOS sites across North America Measures and reports standard atmospheric variables with a frequency of 1-60 minutes

TemperatureDew point temperaturePressureWind direction/speedRainfallCloud heightVisibility

Page 5: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Displaying Surface Observations

Fig. 1-17, p. 21

Page 6: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

West Texas Mesonet

www.mesonet.ttu.edu

Page 7: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Fig. 1-16, p. 19

Station Model

Page 8: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Box 5-1, p. 128

Meteogram

• Displays a time series of meteorological variables for a single station

Page 9: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

How are atmospheric How are atmospheric variables measured?variables measured?

• Unique instrumentation exists for each variable

Page 10: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

TemperatureTemperature

• ASOS uses resistance thermometers, which measure the change in electrical resistance of a piece of metal (a function of temperature)

• Often sheltered by a white “Stevenson Screen”, protecting thermometer from direct solar irradiation

• Well ventilated

Fig. 5-2, p. 129

Page 11: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Humidity• Dew point hygrometer• Also called a “chilled

mirror sensor”• A clean mirror will exactly

reflect laser light to the receiver

• Temperature of mirror is decreased incrementally until water vapor condenses on it. Laser light scattered by the water droplets, reduction in intensity at receiver, dewpoint temperature reported.

Fig. 5-3, p. 130

Page 12: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

PressurePressure

• Mercury barometers (top) and aneroid barometers (bottom) are what we are used to.

• ASOS uses electronic barometers.

Fig. 5-4, p. 131

Page 13: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Wind Direction / Speed• Cup anemometer used to

measure wind speed• Wind vane used to measure

wind direction• Also, there are sonic

anemometers (below), which measure how wind affects the propagation of acoustic energy (no moving parts!)

Page 14: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

PrecipitationPrecipitation• Tipping bucket rain

gauge• Upper heated collector

(melts frozen precipitation)

• Collector empties into bucket underneath, which tips and empties after every 0.01” of precipitation is collected.

• Wind guard around outside to keep precipitation from blowing across opening.

Page 15: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Measuring the Upper Measuring the Upper AtmosphereAtmosphere

• Upper atmosphere is sorely undersampled• These measurements needed for improved model

forecasts!• Radiosondes released twice a day from stations

spaced far apart

Page 16: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Indirect MeasurementsIndirect Measurements

• Two forms:– Active sensors – transmit and

receive energy– Passive sensors – just receive energy

• Examples?

Page 17: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Satellite ObservationsSatellite Observations

• Two orbits for satellites– Geosynchronous or Geostationary orbit – 36,000

km above Earth’s surface. • Satellite rotates at same rate that the planet does.

Therefore, the satellite constantly views the same footprint on Earth.

• Good for constructing animations to determine motion of atmospheric features .

– Low earth orbit (~ 500 miles above the surface)• Satellite rotates faster than the planet• Therefore, this strategy is good for scanning many

portions of the planet• Usually, scans are from pole to pole

Page 18: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Fig. 5-13, p. 140

Page 19: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Typical coverage for a low-earth orbit

http://sharaku.eorc.jaxa.jp/AMSR/ocean_wind/manual/images/sunglitter_e.bmp

Page 20: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Operational U. S. Satellites

• Geostationary Operational Environmental Satellite (GOES)

Page 21: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Visible Satellite Animations

Page 22: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Types of Satellite Types of Satellite ImageryImagery

• Visible– What we have seen thus far– Solar radiation reflected/scattered by earth

and atmosphere

• Infrared– Allows us to visualized how much infrared

energy the earth and atmosphere are emitting– Tells us the temperature of the emitting

substance– For clouds, this information is valuable for

determining altitude of cloud tops!

Page 23: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Recall Wien’s LawRecall Wien’s Law

• λmax = C / T

• The wavelength of maximum emission is inversely proportional to temperature

• Graphic from www.cira.colostate.edu/ramm/goes39

Fig. 2-8, p. 36

Page 24: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Visible vs. Infrared

VISIBLE satellite image INFRARED satellite image

X X XX

cold warm

Page 25: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Types of Satellite Types of Satellite ImageryImagery

• Water Vapor– Tracks infrared emission primarily from water

vapor (6.5-7 mm)– Altitude of emission: 300-600 mb– Can track upper-atmospheric flow– Useful for diagnosing upper-air weather

pattern (e.g., troughs, ridges…more later)– Since water vapor exists in some proportion

everywhere across the globe, continuous surveillance of flow is possible (do not need to have clouds)

Page 26: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Water Vapor Animation

Page 27: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Radar(Radio Detection and Ranging)

Page 28: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

RADAR basics• Electromagnetic energy

transmitted into atmosphere

• Backscattered energy (“radar echo”) measured by radar and displayed

• The larger the object, the more energy that is returned. Therefore, the intensity of the radar echo tells us how much precipitation is falling

• Sources of backscattering: raindrops, hail, snow, ground targets, debris

Fig. 5-19, p. 145

Page 30: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Storm Total Precipitation

Page 31: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

WSR-88D Doppler Radar

Page 32: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Doppler Effect

• Johann Christian Doppler (1803-1853)• Apparent frequency of radiation is affected

by motion of emitting source– Frequency increases for motion towards

observer– Frequency decreases for motion away from

observer

• Can use this effect to deduce motion of scatterers in atmosphere (driven by wind)

Page 33: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Doppler Effect Animation

The Doppler Effect

Page 34: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

WSR-88D Network

Page 35: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Radar Reflectivity & Doppler Velocity

Page 36: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Research Radars

Doppler on Wheels (DOW) –Center for Severe Weather Research

Shared Mobile Atmospheric Research and Teaching Radar (SMART-R) – Texas Tech, Texas A&M,University of Oklahoma,National Severe Storms Laboratory

University of Massachusetts Tornado Radar

COMING IN 2007:TEXAS TECH Ka-band Radars

Page 37: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

UMass Tornado Radar Data3 May 1999

Reflectivity Velocity

Page 38: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Wind Profilers

• Wind direction and speed inferred from three separate radar beams (one vertical, two orthogonal oblique)

• Vertical profiling

Image from B. GeertsUniv. of Wyoming

Page 39: Chapter 5 Observing the Atmosphere ATMO 1300 SPRING 2010

Fig. 5-23, p. 148