Urban Signatures: Sensible Heat Flux (WMS)

  • Released Friday, May 27, 2005

Big cities influence the environment around them. For example, urban areas are typically warmer than their surroundings. Cities are strikingly visible in computer models that simulate the Earth's land surface. This visualization shows sensible heat flux predicted by the Land Information System (LIS) for a day in June 2001. (Sensible heat flux refers to transfer of heat from the earth's surface to the air above; for further explanation see http://www.uwsp.edu/geo/faculty/ritter/geog101/textbook/energy/energy_balance.html). Sensible heat flux is higher in the cities—that is, they transfer more heat to the atmosphere—because the surface there is warmer than in the surroundings. Only part of the global computation is shown, focusing on the highly urbanized northeast corridor in the United States, including the cities of Boston, New York, Philadelphia, Baltimore, and Washington.

This image shows sensible heat flux (watts per
square meter) predicted by LIS for 2001/06/11. The warm urban areas
have higher positive flux (heat flowing towards the atmosphere)
and stand out very distinctly against their
surroundings.This product is available through our Web Map Service.

This image shows sensible heat flux (watts per square meter) predicted by LIS for 2001/06/11. The warm urban areas have higher positive flux (heat flowing towards the atmosphere) and stand out very distinctly against their surroundings.

This product is available through our Web Map Service.

Sensible heat flux color bar. Negative values (blue) indicate heat flow from the atmosphere to the surface; positive (red)
values indicate heat flow from surface to atmosphere. The range of this color bar is greater than the flux values in the area
shown in the visualization; values in the visualization range
from -100 to +284 W/m2.

Sensible heat flux color bar. Negative values (blue) indicate heat flow from the atmosphere to the surface; positive (red) values indicate heat flow from surface to atmosphere. The range of this color bar is greater than the flux values in the area shown in the visualization; values in the visualization range from -100 to +284 W/m2.



Credits

Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio

Release date

This page was originally published on Friday, May 27, 2005.
This page was last updated on Wednesday, May 3, 2023 at 1:56 PM EDT.


Series

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