On peculiarities of convective activity of the atmosphere during the solar eclipse on 31 May 2003

Details On peculiarities of convective activity of the atmosphere during the solar eclipse on 31 May 2003 On peculiarities of convective activity of the atmosphere during the solar eclipse on 31 May 2003

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004kfnt...20..452a&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 20, no. 5, p. 452-456

Physics

Scientific paper

We give some results of measurements of the r. m. s. value of the solar limb motion amplitude for different phases of the partial solar eclipse in morning hours. It is found that the process of active destruction of the inversion layer by uprise convective flows occurs at the illuminance E > 0.2E0, where E0 is the illuminance from the Sun in zenith. Before this moment, the relationship between the motion amplitude σ and zenith distance of the Sun z corresponds to the theoretical law σ(z) = σ (0)√{sec(z)}.

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