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Hemant L. Gohil Melanie J. Correll Thomas Sinclair 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
As part of a Bio-regenerative Life Support System (BLSS) for long-term space missions, plants will likely be grown at reduced pressure. This low pressure will minimize structural requirements for growth chambers on missions to the Moon or Mars. However, at reduced pressures the diffusivity of gases increases. This will affect the rates at which CO2 is assimilated and water is transpired through stomata. To understand quantitatively the possible effects of reduced pressure on plant growth, CO2 and H2O transport were calculated for atmospheres of various total pressures (101, 66, 33, 22, 11 kPa) and CO2 concentrations (0.04, 0.1 and 0.18 kPa). The diffusivity of a gas is inversely proportional to total pressure and shows dramatic increases at pressures below 33 kPa (1/3 atm). A mathematical relationship based on the principle of thermodynamics was applied to low pressure conditions and can be used for calculating the transpiration and photosynthesis of plants grown in hypobaria. At 33 kPa total pressure, the stomatal conductance increases by a factor of three with the boundary layer conductance increasing by a factor of ∼1.7, since the leaf conductance is a function of both stomatal and the boundary layer conductance, the overall conductance will increase resulting in significantly higher levels of transpiration as the pressure drops. The conductance of gases is also regulated by stomatal aperture in an inverse relationship. The higher CO2 concentration inside the leaf air space during low pressure treatments may result in higher CO2 assimilation and partial stomata closure, resulting in a decrease in transpiration rate. The results of this analysis offer guidelines for experiments in pressure and high CO2 environments to establish ideal conditions for minimizing transpiration and maximizing the plant biomass yield in BLSS. 相似文献
514.
马文坡 《运载火箭与返回技术》2007,28(4):23-27
介绍了卫星光学遥图像获取与图像处理一体化优化设计的思路;运用通用像质方程(GIQE)对于利用小相对孔径光学系统和调制传递函数补偿(MTFC)方法得到的图像的品质与利用相对较大相对孔径光学系统得到的图像的品质进行了对比分析。 相似文献
515.
Werner Däppen 《Space Science Reviews》1998,85(1-2):49-60
The equation of state is one of the three fundamental ingredients used to construct stellar models. The plasma of the interiors
of stars such as the Sun is only slightly non-ideal. However, the extraordinary accuracy of the helioseismological data requires
refined equations of state. It turned out to be necessary to include a Coulomb correction, commonly evaluated in the Debye-Hückel
approximation. Higher-order non-ideal effects have implications as well, both for plasma physics and for solar physics. As
a typical example, the recently studied thermodynamic consequence of excited states in compound particles is discussed. This
effect is of considerable relevance in the helioseismic determination of the helium abundance in the solar convection zone.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
516.
Douglas Gough 《Space Science Reviews》1998,85(1-2):141-158
Standard solar models, although they are free from the influence of much of the fluid motion that is bound to be present in
the Sun, have been shown by helioseismology to represent the spherically averaged structure of the Sun amazingly well. This
state of affairs has come about after painstaking refinements by a great many people of the pertinent microphysics, including
that which controls the equation of state, the opacity, the nuclear reaction rates and the diffusion that inhibits gravitational
segregation of chemical elements. It has instilled confidence in the modellers in being able to predict the composition of
the solar interior. But there are consequences of the flow, related particularly to redistribution of chemical species, that
can be difficult to identify observationally, yet which may degrade any inferences we might make. Their potential presence
must at least be acknowledged by anyone who tries to asses the reliability of the models. This report summarizes the discussions
in the preceding pages of this volume of the current theoretical and observational status of the subject, pointing to many
of the caveats that have been raised, and attempting at the same time to put them into a seemingly coherent discourse in the
context of our present understanding of the workings of the solar interior.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
517.
针对二维欧拉方程研究了一类高分辨正性保持波尔兹曼型差分格式,首先分析了波尔兹曼方程和欧拉方程之间的关系;然后,利用一种特殊的插值技术构造了一类高分辨波尔兹曼型差分格式.最后通过数值实验验证了格式的实用性和有效性. 相似文献
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The Hopkinson pressure bar tests for base metal and friction stir jointing(FSJ) jointed region of 7022 a- luminum alloy are carried out at different temperatures and strain rates. The temperature is 30--400 ℃ and the strain rate is 1 200-5 000 s 1. High strain rate for base metal and FSJ jointed region of 7022 aluminum alloy are studied. The corresponding stress-strain curves are obtained. The results show that the flow stresses of base metal and FSJ jointed region of 7022 aluminum alloy decline with the increase of temperature and increase with the in- crease of strain rate. Furthermore, the constitutive equation for base metal and FSJ jointed region of 7022 alumi- num alloy at high temperature and high strain rate is obtained based on Johnson-Cook model. 相似文献
520.