Laboratory simulation of inertial and frictional effects on barotropic rotating flows over and past obstacles: Comparison with simple numerical and analytical models |
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Authors: | S. Alessio L. Briatore R. Cremonini E Ferrero C. Giraud A. Longhetto O. Morra R. Purini |
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Affiliation: | (1) Istituto di Fisica Generale, Università di Torino, Torino, Italy;(2) Dipartimento di Scienze e Tecnologie Avanzate, Università di Torino Sede di Alessandria, Alessandria, Italy;(3) Istituto di Cosmogeofisica, CNR, Torino, Italy;(4) Istituto di Fisica dell'Atmosfera, CNR, Roma, Italy |
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Abstract: | Summary This paper presents the results of laboratory experiments designed to simulate some basic process of large-scale flows interacting with obstacles, also in order to better understand details of subsynoptic disturbances that are created in the lee of large topographic features. For this event, the experimental facilities of the Istituto di Cosmogeofisica of Consiglio Nazionale delle Ricerche (CNR) were exploited, consisting in a hydraulic channel mounted on a rotating platform, along whose longitudinal axis a hemispherical obstacle was towed at various speeds. Because of the conversion of potential vorticity, the experimental results showed, as expected, the existence of a region of anticyclonic circulation, located above the obstacle; however, also an asymmetric pattern of positive vorticity located downwind of the obstacle did appear, which cannot be interpreted in terms of simple quasi-geostrophic inviscid dynamics. This behaviour is not surprising, if one considers that the real flow near the obstacle could hardly ever match the conditions of inviscid quasi-geostrophy (Ro≪1,E∼0), but was similar to that characterising the zone close to the surface of the obstacle, where inertial and viscous effects are not negligible. Finally, in order to investigate the importance of these effects on the interaction processes, simple numerical and analytical models were applied, by which the consistency of some laboratory simulations, chosen among the most significant ones, could be compared. |
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Keywords: | Cosmic rays |
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