Lennon Hall Rooftop Weather Station

Department of the Earth Sciences Rooftop Weather Station


Meteogram Yesterday's Climate Summary Past Summaries Preliminary Summary (for today)


This page provides information concerning the Department of the Earth Sciences Rooftop Weather Station. The station, located on the roof of Lennon Hall, is pictured at left. The weather station was purchased from Climatronics Corporation of Bohemia, New York. Wind speed and direction, temperature, relative humidity, and solar irradiance are measured by instrumentation on the metal tripod. A tipping bucket raingauge is located nearby; the heated precipitation collector also measures snowfall water equivalent. These data are collected by a datalogger, which also contains a barometer to measure atmospheric pressure. The data are then automatically transferred to a personal computer, where data collection software runs continuously. The data are written to a disk that is also mounted by our local UNIX computer network. On the UNIX system there are a series of programs that perform additional computations, write the data into html format for display on the web, and store the data in GEMPAK format. In addition to the current weather display, a brief climate summary for the previous day is now available. Starting in August 1997, an archive of climate summaries for past days is available.


Current Rooftop Weather Station Observation, 17:15 EST:

Temperature: 64.7 F Wind: 220 degrees at 25.3 knots
Relative Humidity: 39.4% Sea Level Pressure: 1007.5 mb
Dewpoint Temperature: 39.8 F Solar Radiation: 501.6 Watts/m2

Solar Radiation Measurement

The instrument used for measurement of incoming solar radiation is called a pyranometer. The particular instrument used by our weather station is a model Mk 1-G pyranometer, built by Matrix, Inc. of Mesa Arizona. Pyranomemeters operate by measuring the temperature difference between two types of absorbing materials, one that is a nearly-perfect absorber of solar wavelengths (black material) and another that reflects nearly all solar radiation (white material). This temperature difference is related to the intensity of incoming solar radiation; when there is no solar radiation (i.e., at night) the temperature difference between the two materials is negligible. Perhaps the most familiar units for solar radiation are Watts per square meter (W/m2).



Temperature and Humidity

The thermometer and relative humidity sensors are located in the white plastic shelter pictured at left. The relative humidity sensor, a Rotronic model MP601A, provides a 0 to 1 volt output signal that linearly corresponds to 0-100% relative humidity. The enclosure for these sensors is white in order to ensure that the temperature reading is not biased by absorption of incoming solar radiation. The location of the temperature sensor on top of Lennon Hall (approx. 60 feet above ground level) may not be representative of conditions near the ground on clear, calm nights. In these instances, cool air will generally be confined to a shallow layer near the surface. Therefore the minimum temperature readings shown here will occasionally be several degrees warmer than readings from the airport or other nearby weather stations where the thermometer readings are taken closer to ground level.



Precipitation

Precipitation measurements are taken with a model TRP-525 tipping bucket raingauge built by Texas Electronics. The collection cone is heated for wintertime precipitation measurement. There is some problem with exposure at this buildingtop site because increased winds above the surface could reduce the amount of precipitation "captured" by our gauge. This will particularly be true in high-wind situations. However, we have the luxury of intercomparison with our weighing gauge located at a nearby site. The weighing gauge provides more reliable measurements during winter because tipping-bucket gauges are not designed to measure snowfall accurately.



Pictured at right is a closeup of the inside of the tipping-bucket gauge. The black object in the center of the gauge is a two-sided bucket mounted on a fulcrum halfway between the two buckets. As precipitation collects in one side of the bucket, it eventually tips the bucket, activating a contact switch in the process. (A magnet swings close to an electric switch.) Then, the other side of the gauge fills, and the bucket tips back, and so forth. Each switch activation is recorded by the datalogger and stored on the departmental UNIX system. Every bucket tip is equivalent to 0.01" of rainfall. Spent water drains out the bottom of the gauge.



Atmospheric Pressure Measurement


The pressure sensor used here is a Setra Model 276 pressure transducer. In general, station pressure is a strong function of altitude, so in order to observe pressure fluctuations associated with mobile weather systems all pressure measurements must be "reduced" to a common altitude. The most common altitude used is sea level; hence we report sea level pressure readings for comparison with readings on synoptic weather maps.



Wind Speed and Direction


The Wind Mark IIIa wind sensor measures the wind speed and direction with separate sensors. Wind speed is measured with the three-cup anemometer pictured above. The cups rotate and the frequency of rotation is measured by a "light chopper". The frequency is proportional to wind speed.



The wind vane is coupled to a potentiometer; the voltage on the potentiometer is then related to the wind direction. We have thus far only undertaken rough calibration of the wind direction, so there may be an error of up to 20 degrees in our currently reported values. More careful calibration will be made shortly.



The rooftop weather station and the rooftop web page were set up by Prof. Gary Lackmann of the Department of the Earth Sciences . Any comments, suggestions, or questions concerning these data or instruments should be sent to the Earth Sciences Department Secretary by clicking here.