Field Measurements of Terrestrial and Martian Dust Devils

Surface-based measurements of terrestrial and martian dust devils/convective vortices provided from mobile and stationary platforms are discussed. Imaging of terrestrial dust devils has quantified their rotational and vertical wind speeds, translation speeds, dimensions, dust load, and frequency of occurrence. Imaging of martian dust devils has provided translation speeds and constraints on dimensions, but only limited constraints on vertical motion within a vortex. The longer mission durations on Mars afforded by long operating robotic landers and rovers have provided statistical quantification of vortex occurrence (time-of-sol, and recently seasonal) that has until recently not been a primary outcome of more temporally limited terrestrial dust devil measurement campaigns. Terrestrial measurement campaigns have included a more extensive range of measured vortex parameters (pressure, wind, morphology, etc.) than have martian opportunities, with electric field and direct measure of dust abundance not yet obtained on Mars. No martian robotic mission has yet provided contemporaneous high frequency wind and pressure measurements. Comparison of measured terrestrial and martian dust devil characteristics suggests that martian dust devils are larger and possess faster maximum rotational wind speeds, that the absolute magnitude of the pressure deficit within a terrestrial dust devil is an order of magnitude greater than a martian dust devil, and that the time-of-day variation in vortex frequency is similar. Recent terrestrial investigations have demonstrated the presence of diagnostic dust devil signals within seismic and infrasound measurements; an upcoming Mars robotic mission will obtain similar measurement types

Physical Processes in Star Formation

© 2020 Springer-Verlag. The final publication is available at Springer via https://doi.org/10.1007/s11214-020-00693-8.Star formation is a complex multi-scale phenomenon that is of significant importance for astrophysics in general. Stars and star formation are key pillars in observational astronomy from local star forming regions in the Milky Way up to high-redshift galaxies. From a theoretical perspective, star formation and feedback processes (radiation, winds, and supernovae) play a pivotal role in advancing our understanding of the physical processes at work, both individually and of their interactions. In this review we will give an overview of the main processes that are important for the understanding of star formation. We start with an observationally motivated view on star formation from a global perspective and outline the general paradigm of the life-cycle of molecular clouds, in which star formation is the key process to close the cycle. After that we focus on the thermal and chemical aspects in star forming regions, discuss turbulence and magnetic fields as well as gravitational forces. Finally, we review the most important stellar feedback mechanisms.Peer reviewedFinal Accepted Versio

I lidi della conoscenza. La storia della Biblioteca Alessandrina

Storia del primo e più importante centro culturale del mondo antico, creato da Tolomeo I per conservare il patrimonio culturale di tutta l'umanit

Falklands wetlands and aquatic habitats: baselines for monitoring future change. Indicator monitoring report

A report under Darwin Plus Project 116 by the South Atlantic Environmental Research Institute. The report provides a framework for on-going and future long-term monitoring of the Falkland Islands wetlands

β-Adrenergic regulation of IL-6 release from adipose tissue: in vivo and in vitro studies

UNLABELLED: Circulating IL-6 levels are elevated in obesity. Although IL-6 is expressed in adipose tissue, neither its regulation nor cell of origin is well characterized. Here we investigated the beta-adrenergic regulation of IL-6 release in a combination of studies on humans and animals in vivo and cultured adipocytes in vitro. Human in vivo study: Human volunteers were infused with isoproterenol, norepinephrine, or saline [4 M:4F; mean (SD) age 35.5 (5.8) yr; body mass index 24.6 (4.2) kg/m(-2)]. Plasma IL-6 levels increased during a 3-h infusion of isoproterenol (P = 0.01) and fell 2 h post infusion (P = 0.05). IL-6 levels did not change significantly with either norepinephrine or saline. Murine in vivo study: C57BL6/J male mice were injected ip with dobutamine (beta(1) agonist), clenbuterol (beta(2)), CL316243 (beta(3)), or saline placebo. Plasma IL-6 levels at 3 h were increased by clenbuterol (P = 0.02) and CL316243 (P = 0.02) but not dobutamine (P = 0.51), compared with placebo.IN VITRO STUDIES: In human peripheral blood cells, lipopolysaccharide treatment enhanced secretion of IL-6 (vs. controls; P &lt; 0.001), whereas isoproterenol inhibited IL-6 secretion (P = 0.012) and norepinephrine had no significant effect. In contrast, isolated human adipocytes and differentiated 3T3F442A adipocytes all rapidly secreted IL-6 in response to adrenergic agonists (P &lt; 0.01, compared with untreated cells). We conclude that beta 2/beta 3 adrenoceptor stimulation on adipocytes, rather than macrophages, may be responsible for the increases in plasma IL-6 concentrations observed during sympathetic activation and in obesity.</p

Drawing Euler diagrams from region connection calculus specifications with local search

International audienceThis paper describes a local search based approach and a software tool to approximate the problem of drawing Euler diagrams. Specifications are written using RCC-8-constraints and radius constraints. Euler diagrams are described as set of circles