Evolutionary theory of convective organization
| Autor: | Mapes, Brian E. |
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| Rok vydání: | 2024 |
| Předmět: | |
| Druh dokumentu: | Working Paper |
| Popis: | Observed patterns of convective cloud would be extremely improbable from random walks in an abstract space of configurations. Forcing is sometimes the driver, but complexity can also develop spontaneously. Here pattern evolution is considered as a natural selection process in a strategic game among configurations, akin to ecological succession. Information (entropy) quantifies improbability, interpreted as Darwinian fitness to the extent larger-scale forcings are properly accounted. Reconciling inferred or revealed fitness with energetics could make convection a showcase of evolutionary theory, simply as reinterpretation of spectral kinetic energy (KE) budgets for dry convection. For moist convection, the flux of a total energy E, the teleological reason for convection, is conjectured to be the central resource of an evolutionary game, with water playing a constraining role like nutrients in ecology. Shannon information H is reviewed in context of this evolutionary reasoning. Analysis of a new Cloud Botany shallow convection simulation set shows growth of H over tens of hours (perhaps more pertinently, it grows with KE throughput or cumulative buoyancy flux). Anisotropy and precipitation boost H in qualitatively distinct and contingent ways, like separate species or ecological guilds. Deep convection over lowland South America also shows many-hour evolution times, beyond simple convective adjustment notions. If evolving horizontal patterns contain or imply information about vertical density profiles, they could become a new resource in data assimilation to predict larger scale flow. Comment: 40 pages with 9 figures, to be submitted to J. Atmos. Sci |
| Databáze: | arXiv |
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