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741.
742.
743.
Solar magnetic field is believed to play a central role in solar activities and flares, filament eruptions as well as CMEs
are due to the magnetic field re-organization and the interaction between the plasma and the field. At present the reliable
magnetic field measurements are still confined to a few lower levels like in photosphere and chromosphere. Although IR technique
may be applied to observe the coronal field but the technique is not well-established yet. Radio techniques may be applied
to diagnose the coronal field but assumptions on radiation mechanisms and propagations are needed. Therefore extrapolation
from photospheric data upwards is still the primary method to reconstruction coronal field. Potential field has minimum energy
content and a force-free field can provide the required excess energy for energy release like flares, etc. Linear models have
undesirable properties and it is expected to consider non-constant-alpha force-free field model. As the recent result indicates
that the plasma beta is sandwich-ed distributed above the solar surface (Gary, 2001), care must be taken in modeling the coronal
field correctly. As the reconstruction of solar coronal magnetic fields is an open boundary problem, it is desired to apply
some technique that can incorporate this property. The boundary element method is a well-established numerical techniques
that has been applied to many fields including open-space problems. It has also been applied to solar magnetic field problems
for potential, linear force-free field and non-constant-alpha force-free field problems. It may also be extended to consider
the non-force-free field problem. Here we introduce the procedure of the boundary element method and show its applications
in reconstruction of solar magnetic field problems.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
744.
745.
T W Tibbitts W Cao 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1994,14(11):427-433
This report discusses the advantages and limitations of several different procedures for growth of potatoes for CELSS. Solution culture, in which roots and stolons are submerged, and aeroponic culture were not found useful for potatoes because stolons did not produce tubers unless a severe stress was applied to the plants. In detailed comparison studies, three selected culture systems were compared, nutrient film technique (NFT), NFT with shallow media, and pot culture with deep media. For the NFT and NFT plus shallow media, plants were grown in 0.3 m2 trays and for the deep medium culture, in 20 liter pots. A 1 cm depth of arcillite, a baked montmorillonite clay, was used as shallow media (NFT-arc). Peat-vermiculite mixture was used to fill the pots for the deep media. Nutrient solution, modified half-strength Hoagland's, was recirculated among the tray culture plants with pH automatically controlled at 5.5, and conductivity maintained at approximately 1100 microS cm-1 by adding stock nutrients or renewing the solution. A separate nutrient solution was used to water the pot plants four times daily to excess and the excess was discarded. Plants of Norland cv. were utilized and transplanted from sterile-propagated stem cutting plantlets. The plants were grown for 66 days under 12 h photoperiod in a first study and grown for 54 days under 24 h photoperiod in a second study. Under both photoperiods, total plant growth was greater in NFT-arc than in either NFT or pot culture. Under 12 h photoperiod, tuber dry weight was 30% higher with NFT-arc, but 50% lower with NFT, than with pot culture. Under 24 h photoperiod, however, tuber dry weight in both NFT and NFT-arc was only 20% of that in pot culture. The NFT and NFT-arc produced a greater shoot growth and larger number of small tubers than pot culture, especially with 24 h photoperiod. It is concluded that there are serious limitations to the use of NFT alone for growth of potatoes in a CELSS system. These limitations can be minimized by using a modified NFT with a shallow layer of media, such as arcillite, yet additional work is needed to ensure high tuber production with this system under long photoperiods. 相似文献
746.
A method of motion compensation for inverse synthetic aperture radar (ISAR) is proposed. The techniques of interpolation, cross correlation, and estimation are used together. Essential to the method is the fact that avoiding cross-range image aliasing due to Doppler ambiguities requires range profiles to be generated at an adequate rate. The effect of noise on motion compensation is studied by means of simulation. The quality of the reconstructed image is used to evaluate the method 相似文献
747.
有热解的轴对称烧蚀体传热有限元计算 总被引:1,自引:0,他引:1
本文采用有限元法,分析和计算了有热解的再入烧蚀体的传热问题。计算方法和程序先用两个算例进行了考证,最后给出了沿真实弹道的计算结果。 相似文献
748.
曹翠微%肖琰%魏伯荣 《宇航材料工艺》2006,36(4):58-60
介绍了用动态热机械分析仪测定天然橡胶(NR)硫化胶耐老化性能的原理及方法。通过测定胶料在160℃、恒温30min下的动态模量谱,来评估硫化胶的耐老化性能。同时测定硫化胶力学性能随老化时间的变化情况。结果显示:老化后储能模量减少,损耗模量和损耗因子tanδ总体呈增加趋势。力学性能随老化时间的延长呈先增加而后下降趋势。 相似文献
749.
崔益华%陶杰%徐勇%沃丁柱 《宇航材料工艺》2003,33(4):10-15,23
系统地综述了近年来纳米改性环氧树脂基复合材料的研究现状。介绍了环氧树脂基纳米复合材料的制备方法和无机纳米粒子的表面修饰方法,分析了环氧树脂基纳米复合材料的形成机理和固化反应动力学,概括了此类复合材料的性能特点并展望了环氧树脂基纳米复合材料未来的发展和应用前景。 相似文献
750.
描述了一台能够对长度达1m的线纹尺和长度达2m的光栅尺(线位移传感器)进行测量的激光干涉仪,干涉仪设计成了双干涉光路系统,以消除光栅尺安装引入的阿贝误差,这台测量仪采用干涉条纹计量原理,对光栅尺和线纹尺的线值精度进行检测,并能对光机信号的质量进行评价。测量过程中,对空气折射率实现了实时修正。 相似文献