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Observing System


Observing System Home


Physical Observations
Weather Stations
Buoyed Weather Stations
Surface Current Measurements
Ocean Moorings and Hydrography
Satellite Imaging
Synthetic Aperture Radar (SAR)


Forecasts
Weather Forecast
Wave Forecast
Ocean Forecast


Biological Observations
Nutrients, Phytoplankton, Zooplankton
Benthic Plants and Animals
Fishes and Shellfishes
Aquaculture
Marine Birds
Marine Mammals


Instruments
Anemometers
RH
Solar Radiation
Precipitation
Thermistors
Salinometers
Current Meters
Pressure Sensors
Web Cameras
Wave & Tide Height


Models
Atmospheric Circulation
Wave Dynamics
Ocean Circulation


Solar Radiation


Without the sun there?d be no sunbathing on Florida?s beaches and the sunscreen industry would face ?dark? times as well, but more importantly, the sun is our primary energy source and the origin of life on earth. The sun is a celestial body with an average temperature of ~6000 degrees C. Every body sends out radiation according to its temperature and since the sun is such a hot body with so much mass it sends out a lot of radiation, which we call solar radiation.

Solar radiation is a governing parameter in all different scientific aspects. Solar energy along with other ingredients delivers the energy that biological organisms use to grow.

Nuclear fusion powers the sun which emits thermal radiation. Solar radiation is the sun's radiant, electromagnetic energy. Radiation in the visible, short- wave portion of the electromagnetic spectrum contains about half of the total radiation, and the near-infrared portion constitutes the other half.

The solar constant is the mean energy density of solar radiation in a plane perpendicular to the sun's rays just above the Earth's atmosphere. It has a value of about 1367 W/mē that fluctuates daily by a few parts per thousand. The amount received at the surface depends on atmospheric factors and the latitude. Solar radiation is measured with a pyranometer.

Data Access

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