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231.
Cool giant and supergiant stars generally present low velocity winds with high mass-loss rates. Several models have been proposed
to explain the acceleration process of these winds. Although dust is known to be present in these objects, the radiation pressure
on these particles is uneffective in reproducing the observed physical parameters of the wind. The most promising acceleration
mechanism cited in the literature is the transference of momentum and energy from Alfvén waves to the gas. Usually, these
models consider the wind to be isothermal. We present a stellar wind model in which the Alfvén waves are used as the main
acceleration mechanism, and determine the temperature profile by solving the energy equation taking into account both the
radiative losses and the wave heating. We also determine, self-consistently, the magnetic field geometry as the result of
the competition between the magnetic field and the thermal pressure gradient. As the main result, we show that the magnetic
geometry presents a super-radial index in the region where the gas pressure is increasing. However, this super-radial index
is greater than that observed for the solar corona. 相似文献
232.
通过原油/三元复合体系乳状液渗流规律的试验研究,得出了原油/三元复合体系乳状液在多孔介质中的渗流曲线,通过理论分析,建立了原油/三元复合体系乳状液渗流的数学模型,理论分析与试验结果比较吻 相似文献
233.
从简单的数学模型出发,利用直观的温度及浓度分布假设,对生物体冻结过程中的传热、传质进行了理论分析,并将结果与精确解及测量值进行了比较。其解法简单,省去了以往的有限差分求解的繁琐的计算过程,并且计算结果与试验数据吻合得很好。 相似文献
234.
接触式指尖密封在工作过程中不可避免地会发生磨损,而磨损又会改变其泄漏特性进而影响旋转机械的效率。为了揭示磨损对指尖密封泄漏特性的影响规律,本文在指尖密封多孔介质流动分析模型的基础之上,建立了考虑转子离心膨胀和磨损效应的指尖密封瞬态泄漏特性数值分析模型,数值研究了转速和安装过盈量对指尖密封磨损及其对应的泄漏特性的影响规律。结果表明:考虑磨损效应时,指尖密封泄漏量随磨损时间的增加呈现出先减小后增大的趋势;转子转速越低,泄漏量降低至最小值所需的磨损时间越长,但最小泄漏量及其所对应的瞬态配合过盈量始终一致;安装过盈量越小,泄漏量降低至最小值所需的磨损时间越短,但最小泄漏量所对应的瞬态配合过盈量始终一致;此外,在任意磨损时刻,密封上下游压差越大泄漏量也越大。 相似文献
235.
236.
M. Youssef R. Mawad Mosalam shaltout 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
We present a statistical study of post-flare-associated CMEs (PFA-CMEs) during the period from 1996 to 2010. By investigating all CMEs and X-ray flares, respectively, in the LASCO and GOES archives, we found 15875 CMEs of which masses are well measured and 25112 X-ray flares of which positions are determined from their optical counterparts. Under certain temporal and spatial criteria of these CMEs and solar flare events, 291PFA-CMEs events have been selected. Linking the flare fluxes with CME speeds of these paired events, we found that there is a reasonable positive linear relation between the CME linear speed and associated flare flux. The results show also the CME width increases as the flux of its associated solar flare increases. Besides we found that there is a fine positive linear relation between the CME mass and its width. Matching the flare fluxes with CME masses of these paired events, we find the CME mass increases as the flux of its associated solar flare increases. Finally we find the PFA-CME events are in regular more decelerated than the other CMEs. 相似文献
237.
Carlos Roberto Braga Alisson Dal Lago Guillermo Stenborg 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The white light coronagraphs onboard SOHO (LASCO-C2 and -C3) and most recently STEREO (SECCHI -COR1 and -COR2) have detected a myriad of coronal mass ejections (CME). They are a key component of space weather and under certain conditions they can become geo-effective, hence the importance of their kinematic characterization to help predict their effects. However, there is still a lot of debate on how to define the event boundaries for space weather purposes, which in turn makes it difficult to agree on their kinematic properties. That lack of agreement is reflected in both the manual and automated CME catalogs in existence. To contribute to a more objective definition and characterization of white-light coronagraph events, Goussies et al. (2010) introduced recently the concept of “texture of the event”. Based on that property, they developed a supervised segmentation algorithm to allow the automatic tracking of dynamic events observed in the coronagraphs field of view, which is called CORonal SEgmentation Technique (CORSET). In this work, we have enhanced the capabilities of the algorithm by adding several new functionalities, namely the automatic computation of different morphological and kinematic parameters. We tested its performance on 57 well-studied limb CME events observed with the LASCO coronagraphs between 1997 and 2001, and compared the parameters obtained with those from three existent CME lists: two of them obtained from an observer-based detection and tracking method (i.e., two manual catalogs), and the other one based on the automated detection and characterization of the CME events (i.e., a fully automated catalog). We found that 51 events could be tracked and quantified in agreement with the CME definition. In general terms, the position angle, and the radial and expansion speeds are in agreement with the manual catalogs used for comparison. On the other hand, some discrepancies between CORSET and the automated catalog were found, which can be explained by the different delimitation of the CME angular extent. 相似文献
238.
在氦质谱检漏技术理论的基础上,采用了以微电脑为中心的自动控制技术,提高了氦质谱检漏仪的全自动操作智能化水平。180°非均匀磁场的实现,使离子聚焦更好。通过电子量程切换技术,减少了量程转换时间,扩大了测量范围,对高准确度密封性智能检测系统的实现进行了详细的研究与实践。 相似文献
239.
Leen Decin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Cool objects glow in the infrared. The gas and solid-state species that escape the stellar gravitational attraction of evolved late-type stars in the form of a stellar wind are cool, with temperatures typically ?1500 K, and can be ideally studied in the infrared. These stellar winds create huge extended circumstellar envelopes with extents approaching 1019 cm. In these envelopes, a complex kinematical, thermodynamical and chemical interplay determines the global and local structural parameters. Unraveling the wind acceleration mechanisms and deriving the complicated structure of the envelopes is important to understand the late stages of evolution of ∼97% of stars in galaxies as our own Milky Way. That way, we can also assess the significant chemical enrichment of the interstellar medium by the mass loss of these evolved stars. The Herschel Space Observatory is uniquely placed to study evolved stars thanks to the excellent capabilities of the three infrared and sub-millimeter instruments on board: PACS, SPIRE and HIFI. In this review, I give an overview of a few important results obtained during the first two years of Herschel observations in the field of evolved low and intermediate mass stars, and I will show how the Herschel observations can solve some historical questions on these late stages of stellar evolution, but also add some new ones. 相似文献
240.