4.6 Article

Land-Atmosphere Responses to a Total Solar Eclipse in Three Ecosystems With Contrasting Structure and Physiology

Journal

JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES
Volume 124, Issue 2, Pages 530-543

Publisher

AMER GEOPHYSICAL UNION
DOI: 10.1029/2018JD029630

Keywords

eclipse micrometeorology and biometeorology; eddy covariance; ecosystem science

Funding

  1. NASA through the Interdisciplinary Science For Eclipse 2017 program [NNX17AH79G]
  2. U.S. Department of Energy, Office of Science, Office of Biological and Environmental Research Program, Climate and Environmental Sciences Division through Oak Ridge National Laboratory's Terrestrial Ecosystem Science-Science Focus Area
  3. U.S. Department of Energy [DE-AC05-00OR22725]
  4. USDA-ARS Project [5070-12130-005-00D]
  5. National Science Foundation [IIA-1355406]

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Mid-Missouri experienced up to 2min 40s of totality at around solar noon during the total eclipse of 2017. We conducted the Mid-Missouri Eclipse Meteorology Experiment to examine land-atmosphere interactions during the eclipse. Here, research examining the eclipse responses in three contrasting ecosystems (forest, prairie, and soybeans) is described. There was variable cloudiness around first and fourth contacts (i.e., the start and end of partial solar obscuration) at the forest and prairie; however, solar irradiance (K) signals during the eclipse were relatively clean. Unfortunately, the eclipse forcing at the soybean field was contaminated by convective activity, which decreased K beginning about an hour before first contact and exposed the field to cold outflow 30min before second contact. Turbulence was suppressed during the eclipse at all sites; however, there was also an amplified signal at the soybean field during the passage of a gust front. The standard deviations of the horizontal and vertical wind velocities and friction velocities decreased by 75% at the forest (aerodynamically rough), and 60% at the prairie (aerodynamically smooth). The eddy fluxes of energy were highly coherent with the solar forcing with the latent and sensible heat fluxes approaching 0W/m(2) and changing in direction, respectively. For the prairie site, we estimated a canopy-scale time constant for the surface conductance light response of 10min. Although the eclipse imparted large forcings on surface energy balances, the air temperature response was relatively muted (1.5-2.5 degrees C decrease) due to the absence of topographic effects and the relatively moist land and atmosphere.

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