Jets and Large Scale Outflows: Theory Confronts the Observations     

Ralph E. Pudritz 《Astrophysics and Space Science》2004,292(1-4):471-478

This article summarizes recent theoretical, numerical and observational progress on the nature of jets and outflows in regions of star formation. The emphasis is placed on the role of hydromagnetic phenonmena in understanding these new results. The confluence of sophisticated 3D numerical MHD simulations and the recent observations of rotating jets makes it possible, for the first time, to rigorously test jet models.  相似文献   

Multi‐generational carbonate assemblages in martian meteorite Allan Hills 84001: Implications for nucleation,growth, and alteration     

Catherine M. CORRIGAN  Ralph P. HARVEY 《Meteoritics & planetary science》2004,39(1):17-30

Abstract— The carbonate mineralogy of several complex carbonate‐rich regions in Allan Hills (ALH) 84001 has been examined. These regions contain familiar forms of carbonate, as well as textural forms previously unreported including carbonate rosettes, planiform “slab” carbonates, distinct “post‐slab” magnesites, and carbonates interstitial to feldspathic glass and orthopyroxene. Slab carbonates reveal portions of the carbonate growth sequence not seen in the rosettes and suggest that initial nucleating compositions were calcite‐rich. The kinetically controlled growth of rosettes and slab carbonates was followed by an alteration event that formed the magnesite‐siderite layers on the exterior surfaces of the carbonate. Post‐slab magnesite, intimately associated with silica glass, is compositionally similar to the magnesite in these exterior layers but represents a later generation of carbonate growth. Feldspathic glasses had little or no thermal effect on carbonates, as indicated by the lack of thermal decomposition or any compositional changes associated with glass/carbonate contacts.  相似文献   

Gemini observations of disks and jets in young stellar objects and in active galaxies     

Peter McGregor  Michael Dopita  Ralph Sutherland  Tracy Beck  Thaisa Storchi-Bergmann 《Astrophysics and Space Science》2007,311(1-3):223-230

We present first results from the Near-infrared Integral Field Spectrograph (NIFS) located at Gemini North. For the active galaxies Cygnus A and Perseus A we observe rotationally-supported accretion disks and adduce the existence of massive central black holes and estimate their masses. In Cygnus A we also see remarkable high-excitation ionization cones dominated by photoionization from the central engine. In the T-Tauri stars HV Tau C and DG Tau we see highly-collimated bipolar outflows in the [Fe II] λ 1.644 micron line, surrounded by a slower molecular bipolar outflow seen in the H₂ lines, in accordance with the model advocated by Pyo, T.-S., et al., Astrophys. J. 570, 724 (2002).  相似文献   

Biogeochemistry of Ethanol and Acetaldehyde in Freshwater Sediments     

J. Alan RoebuckJr.  G. Brooks Avery  J. David Felix  Robert J. Kieber  Ralph N. Mead  Stephen A. Skrabal 《Aquatic Geochemistry》2016,22(3):177-195

This study reports the first ethanol and acetaldehyde measurements in sediment porewaters collected at multiple freshwater locations. Ethanol concentrations ranged from 11 to 2535 nM and acetaldehyde concentrations ranged from 6 to 320 nM. A significant positive correlation (p < 0.001) was observed between ethanol concentrations and the percent organic carbon content of sediments (TOC). Porewater depth profiles at two sites within the same lake indicated potential diffusion of ethanol into sediments from the overlying water at a lower TOC site and upwards diffusion from sediment into the water column at a higher TOC site. Diffusion of water column ethanol into sediments was observed at individual sites from October to January, whereas the opposite was true from June to August indicating the seasonal variability of ethanol flux from sediments. Changes in ethanol concentrations during a long-term sediment incubation experiment showed an inverse relation with acetaldehyde concentrations. The lack of a quantitative conversion was likely due to other sources and sinks that control their abundance. Our study provided new information on the biogeochemistry of ethanol in freshwater sediments and shed light on the potential role of ethanol in the global carbon cycle.  相似文献   

Titan: Interior,surface, atmosphere,and space environment,edited by I. Müller‐Wodarg,C. A. Griffith,E. Lellouch,and T. E. Cravens. Cambridge,UK: Cambridge University Press, 2014, 474 p. $135, hardcover (ISBN #978‐0521199926).     

Ralph D. Lorenz 《Meteoritics & planetary science》2014,49(6):1139-1140

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A photogrammetric surveying method for field applications     

Dirk H.  Rieke-Zapp  Ralph  Rosenbauer  Fritz  Schlunegger 《The Photogrammetric Record》2009,24(125):5-22

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William A. Cassidy (1928–2020)     

John Schutt  Ralph Harvey  Christian Koeberl 《Meteoritics & planetary science》2020,55(7):1709-1712

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Reflectance spectroscopy of insoluble organic matter (IOM) and carbonaceous meteorites     

Hannah H. Kaplan  Ralph E. Milliken  Conel M. O'D. Alexander  Christopher D. K. Herd 《Meteoritics & planetary science》2019,54(5):1051-1068

Insoluble organic matter (IOM) is the major organic component of chondritic meteorites and may be akin to organic materials from comets and interplanetary dust particles (IDPs). Reflectance spectra of IOM in the range 0.35–25 μm are presented as a tool for interpreting organic chemistry from remote measurements of asteroids, comets, IDPs, and other planetary bodies. Absorptions in the IOM spectra were strongly related to elemental H/C (atom) ratio. The aliphatic 3.4 μm absorption in IOM spectra increased linearly in strength with increasing H/C for H/C > 0.4, but was absent at lower H/C values. When meteorite spectra from the Reflectance Experiment Laboratory (RELAB) spectral catalog (n = 85) were reanalyzed at 3.4 μm, this detection limit (H/C > 0.4) persisted. Aromatic absorption features seen in IOM spectra were not observed in the meteorite spectra due to overlapping absorptions. However, the 3.4 μm aliphatic absorption strength for the bulk meteorites was correlated with both H/C of the meteorite's IOM and bulk C (wt%). Gaussian modeling of the 3 μm region provided an additional estimate of bulk C for the meteorites, along with bulk H (wt%), which is related to phyllosilicate abundance. These relationships lay the foundation for determining organic and phyllosilicate abundances from reflectance spectra. Both the full IOM spectra and the spectral parameters discussed here will aid in the interpretation of data from asteroid missions (e.g., OSIRIS‐REx, Hayabusa2), and may be able to place unknown spectral samples within the context of the meteorite collection.  相似文献   

三维正交非结构网格数值模型中物理流场的定义方法与改进     

刘晓辉  董礼先  Ralph T. Cheng 《海洋与湖沼》2010,41(4):621-627

使用Casulli等(2000)的数值方法建立了基于正交非结构网格的U型渠道的三维近岸正压水动力数值模型,检验了模型使用ELM(Eulerian-Lagrangian Method)方法处理平流项时,物理流场的定义对模拟结果的作用。数值试验和结果分析说明,使用ELM方法计算平流项所需的物理流场对计算结果影响明显,而目前常用的两种物理流场定义方法都存在一定不足——水位计算值对流速变化的反映不灵敏或者会产生小扰动等。针对常用物理流场定义方法的不足之处,作者在Casulli方法的基础上利用对多边形切向流速分量进行平均的方法改进了物理流场定义,抑制了小扰动。  相似文献   

Marine and estuarine shallow water science and management: The interrelationship among habitats and their management     

Francis J. Reill  Ralph J. Spagnolo  Edward Ambrogio 《Estuaries and Coasts》1999,22(3):731-734

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