Observations and models of deuterated H3+ in proto-planetary disks

Details Observations and models of deuterated H3+ in proto-planetary disks Observations and models of deuterated H3+ in proto-planetary disks

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rspta.364.3091c&link_type=abstract

Royal Society of London Transactions Series A, vol. 364, Issue 1848, p.3091-3100

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Some of the physical mechanisms that arise in interactions, upstream influence and separation are discussed for boundary layers and internal motions. Mechanism 1 involves pressure-displacement interaction, stemming from the Goldstein singularity and the issue of its removal. At least six other mechanisms, 2-7, arise in more recent studies for two- and three-dimensional flows. These are in blade-wake rotary flows, where streamwise periodicity, inner-outer interactions at very low incidence, and leading-edge jump effects enter the reckoning, and in surface-mounted roughness flows, concerning three-dimensional upstream influence, pressure feedback and longitudinal (e.g. horseshoe) vortex formation. Full Text Access Full Text Available The full text of this article is available. You may view the article as (a): PDF Although it may be a lengthier download, this is the most authoritative online format. Open: Entire document One page at a time

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