The split failure region of disk model is larger with the smaller pore radii distribution parameters.
随着孔径分布控制参数的减小，圆盘劈裂破坏区域增大且更加分散。
Using the disk model, DRBD exports a special device (/dev/drbdX) that you can use just like a regular disk.
使用磁盘模式，DRBD输出一个特殊设备（/dev/drbdX），您可以像使用一个普通磁盘那样使用它。
The pore radii distribution has some influences on tensile strength of disk model with smaller porosity.
当孔隙率较小时孔径分布对抗拉强度有一定的影响；
The conclusion is: the short term variability behavior provides a strong support to the thick accretion disk model of AGN.
这些讨论表明，活动星系核的短时标光变特征对厚吸积盘模型提供了强有力的支持。
The radiation pressure supported thick accretion disk model has been studied more extensively, and it seems to have some difficulties.
辐射压支持的流体厚吸积盘模型已经得到比较多的研究，看来存在一些难以解决的问题。
The N-S equations with adoption of an actuator disk model are used to simulate the effect of turbo-propeller slipstream on high-lift systems.
螺旋桨模型简化为一个激励盘，即一个无厚度可穿透的圆盘，以给定的圆盘拉力载荷，即压强差来模拟螺旋桨滑流的效果。
The different kinds of think accretion disk models, the accretion disk model for ultraviolet excess and the self-gravitating accretion disk model in QSOs axe briefly reviewed.
本文对类星体的各种厚吸积盘模型，紫外超现象的吸积盘模型及自引力吸积盘模型作了简扼评述。
The whole ABS models are established for the simulation requirement, including tire-road model, vehicle dynamic model, brake disk model, hydraulic system model and the controller model.
针对ABS仿真计算的需要，对整个防抱系统进行了建模，包括轮胎模型、车辆模型、制动器模型、液压系统模型和控制器模型；
Notwithstanding the previous guidelines, purchase at least one spare hard disk for each model hard disk you deploy.
尽管有前面的指导方针，但为您部署的每个模型硬盘购买至少一个备用硬盘。
First, convert your constraint model — presumably a file on disk somewhere — into a format that JAXP can use.
首先，将约束模型(可能是某个磁盘上的文件)转化为JAXP可以使用的格式。
Also, if a fragment is modified on disk, only the modified fragment is reloaded, not the entire model.
同样，如果您在硬盘上更改一个片段时，只有变更的片段会得到重新载入，而不是整个模型。
The model then integrated the two pictures to paint a fuller portrait of the dusty disk.
计算完成以后，模型将这两个方面合并到一起，描绘出尘埃盘整体形象。
A key part of this process is to map the requirements of the application model (operating system, architecture, disk, memory) to parts provided by plug-ins.
该流程的一个重要部分是将应用程序模型的要求(操作系统、架构、磁盘、内存)映射到插件提供的组件。
As with adding the virtual disk and network connection units, this dependency link augments the model with extra information to describe the configuration of the virtual image.
添加虚拟化硬盘与网络链接单元之后，这种依赖性链接就会判断额外的信息，以描述虚拟镜像的配置了。
Although you never write the file to disk and never bother about the XML syntax, the document is without doubt an XML document because it conforms to the data model.
虽然从未将文件写入磁盘，也从未使用xml语法，但毫无疑问，该文档是XML文档，因为它符合该数据模型。
The new model also holds that the companion object is a so-called "B star" circled by a dusty disk.
这个新模型依然坚持的观点是那个被称为“B星”的伴星被星尘带所环绕。
In this model, the disk thins out faster than it pushes planets inward.
在这个模型里，盘状物变得愈来愈稀薄的速度要比它把原行星向内推的速度要快。
For instance, QEMU's emulated hard disks return a model string of "QEMU HARDDISK" rather than a real hard disk manufacturer and model.
例如，QEMU的模拟硬盘会返回“QEMUHARDDISK”的模式字符串，与真实的硬盘驱动器不同。
The test environment used a System i Model 520 with two processors, 32 GB of memory, and 98 disk drives with RAID-5 protection.
这个测试环境??用一台SystemiModel 520，有两个处理器、32GB内存和 98 个磁盘驱动器（带 RAID-5保护）。
The other model, 'fragmentation', suggests that small clumps of a gaseous disk form directly into planets over 10,000 years.
另一个模型——碎化模型则认为大量聚集的气体盘在10000多年间直接形成了气体行星。
The other model, 'fragmentation', suggests that small clumps of a gaseous disk form directly into planets over 10, 000 years.
另一个模型——碎化模型则认为大量聚集的气体盘在10000多年间直接形成了气体行星。
For example, a model that grows to 30 MB on disk becomes very difficult to work with day-to-day on a 1 GB RAM machine.
举例来说，达到30MB的模型对于1gb内存的机器来说将变得非常难以处理。
As a virtual disk, DRBD provides a flexible model that a variety of applications can use (from file systems to other applications that can rely on a raw disk, such as a database).
作为一个虚拟磁盘，DRBD提供一个供各种应用程序使用的灵活模型(从文件系统到依赖于一个原始磁盘的其他应用程序，比如数据库)。
A more complex model should take into account other inputs, such as disk usage for processes that are disk-intensive, rather than CPU-intensive.
而更复杂的模型应该考虑到其他因素，比如过程的磁盘使用量，而这些过程往往是大量使用磁盘而不是CPU。
In this model, gas flows from the large red giant companion star into a disk and then onto the White Dwarf.
这个模型是指气体从大型红巨星伴星流到白矮星的吸积盘上然后被吸进白矮星中。
Disks are allocated from an Enterprise Storage Server (2105 model 800) array, with each disk configured as a 3390 model 3.
所有的磁盘都是从一个EnterpriseStorageServer (2105model 800)磁盘阵列中分配的，其中每个阵列都配置为一个3390 model 3。
Select the manufacturer and model of your device. If you have an installation disk, click have disk.
选择设备的厂商和型号。如果有安装磁盘，请单击“从磁盘安装”。
All disks are allocated from an Enterprise Storage Server (2105 model 800) array with each disk configured as a 3390 model 3.
所有的磁盘都是从EnterpriseStorageServer(2105型号800)阵列分配的，每一个磁盘都配置为3390型号3。
All disks were allocated from an Enterprise Storage Server (2105 model 800) array, with each disk configured as a 3390 model 3.
所有的磁盘都是从EnterpriseStorageServer(2105型号800)阵列分配的，每一个磁盘都配置为3390型号3。
All disks were allocated from an Enterprise Storage Server (2105 model 800) array, with each disk configured as a 3390 model 3.
所有的磁盘都是从EnterpriseStorageServer(2105型号800)阵列分配的，每一个磁盘都配置为3390型号3。
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