怎样查找big文件

⑴ big文件是什么怎样使用

big文件一般是游戏中的文件，比较常见的用途是装载游戏的音乐、声音等文件。很多人游戏背景音乐都是从big文件中提取的，使用XCC
Mixer
软件就可以轻松办到，但最好只提取文件，千万不要乱改其中的内容，不然就bug了。

⑵ 红警3big文件放哪里有效

都有效
在桌面“红警3”图标上单击右键，属性
在目标那一栏后加上-ui（注意-ui前要有空格）
然后启动运行，会出现一个窗口 选择Select Language（好像是，反正有一个Language），然后选择Chinese（T），就OK

⑶ 请问如何打开.big文件

复制到FIFA2006安装目录下的相同文件就可以了
参考资料：http://hi..com/coolplay

⑷ 跪求`! . Big 文件格式打开方法`

Arial Audio Converter V2.3.6┊专业的音频格式批量转换工具┊汉化绿色特别版 一款专业的音频转换工具。 它可以在P3, WMA,OGG,MP2,WAV( PCM, DSP, GSM, ADPCM ), G721, G723, G726, VOX, ALAW, ULAW等声音格式之间相互转换。 使用这款非常易用的软件你可以批量转换文件而不必理会它们的源文件格式和目标文件格式。 Arial Audio Converter通过其内置播放器也支持播放功能。 http://www.greendown.cn/soft/2660.html天天音频转换专家 V5.61 绿色下载站专用破解免安装贵宾版‘天天音频转换专家’是一款专业的音频转换工具。 支持MP2, MP3, AAC, AC3, WMA, OGG, AMR, WAV( PCM, DSP, GSM, ADPCM ), G721, G723, G726, G729, VOX, ALAW, ULAW等常见的音频格式之间的转换。 可以批量转换文件而不必理会它们的源文件格式和目标文件格式。 内置播放器支持多种格式的播放功能。 主要特点： ★在MP2, MP3, AAC, AC3, WMA, OGG, WAV( PCM, DSP, GSM, ADPCM), G721, G723, G726, G729, VOX, ALAW, ULAW等声音格式之间按不同的设置进行相互转换； ★支持3G音频格式--AMR； ★支持同一种音频格式在不同压缩率下的转换； ★支持批量音频文件转换； ★支持ID3标签显示和编辑； ★内置播放器支持流行的音乐格式播放； ★用户界面友好，非常易于使用。随意注册即可用法：运行“绿化.exe”即可正常使用。运行“卸除.exe”即可卸除绿化时加到系统的东西。 http://www.greendown.cn/soft/2840.html

⑸ 如何打开.big文件

你安装一个虚拟光驱软件，加载.big文件就能打开了

⑹ BIG格式的文件怎么打开 谢了

听过JEPG 和GIF的图片格式但是没听过BIG格式的 你确定是这个格式？ 可能只是文件名字而已，你把后缀名隐藏了，点击上面的文件选项 显示后缀名再看看

⑺ 请问用什么软件可以解压提取后缀名为big的文件

.big是种游戏里面的音乐格式文件吧，要取得音乐文件，三个步骤：

1、提取音乐文件

2、将 aifc 转换为 wav 格式

3、因为 wav 格式文件很大，再将其转为其他各式（如MP3）。

一、提取音乐文件

1、下载HW2MusicTools.zip。

2、解压之后有两个 ZIP 包，一个是 HW2ICArchive.zip，用于读取和解压 big 文件。另一个 In_Aif.zip 是 WinAmp 的解码插件，用于播放 aifc 格式的音乐。

3、解压 HW2ICArchive.zip，运行当中的 HW2ICArchive.exe。如果出现错误，你就需要先将同目录下的另外两个 .dll 文件注册。

4、这个工具的用法我就不多说了，大家稍微摸索一下就能明白的。用它把 Music.big 中的所有文件解压出来，然后将所有的 .fda 文件重命名为 .aifc 格式。 .lua 的文件不管他，删掉。

⑻ 怎样打开*.big文件

你安装一个虚拟光驱软件，加载.big文件就能打开了

下载
http://www.crsky.com/soft/1158.html

⑼ 提取BIG文件

推荐使用XCC系列软件~~~

⑽ 有关big文件的提取问题。

Big Bang theory of the main opinion is that our universe had a period from hot to cold evolutionary history. During this period, the universe is not a static system, but are constantly expanding, so that the density of matter from the dense to dilute to evolve. This from hot to cold, from dense to dilute the process as the outbreak of an enormous scale. According to Big Bang cosmology opinion, the big bang the whole process are: early in the universe, the temperature is extremely high at 10 billion degrees. Material density is likely to be considerable, the whole system of the universe balanced. The universe only neutrons, protons and electrons, photons and neutrinos and other elementary particles form the material. However, because the whole system continues to expand, the results of the temperature dropped quickly. When the temperature dropped to around one billion degrees, neutrons begin to lose the freedom of the conditions exist, it either happened decay, or with protons into deuterium, helium and other elements; chemical element is formed from the beginning of this period. Temperature further dropped to one million degrees, the early formation of chemical elements in the process of The End (see element synthesis theory). The universe's material is mainly of protons and electrons, photons, and some of the more lighter nuclei. When the temperature is reced to several thousand degrees, the radiation diminishes, the universe is mainly gaseous material, the gas graally unite into a gas cloud further the formation of various star systems, to become the universe we see today.
Gamow in 1948 from the hot set up since the concept of the Big Bang, through decades of efforts, the universe, scientists outline for us the history of such a universe:
Big Bang beginning about 137 million years ago, a very small volume, high density, high temperature.
Big Bang 10 ~ 43 seconds ago the universe emerged from the quantum background.
Big Bang the first 10 ~ 35 seconds with a broken down into strong, weak electric and gravitational force.
Big Bang 10 ~ 5 second 10 trillion degrees, the formation of protons and neutrons.
0.01 seconds after the Big Bang one hundred billion degrees, photon, electron, neutrino mainly accounted for only 10 billionths of a proton neutron, thermal equilibrium state, the rapid expansion of the system, temperature and density continues to drop.
0.1 seconds after the Big Bang 30 billion later, the neutron proton ratio dropped to 0.61 from 1.0.
One second after the Big Bang 10 billion later, the neutrinos escape outward, electron-positron annihilation reaction, nuclear power is still less than the neutron and proton bound.
13.8 seconds after the Big Bang 30 billion kwh, deuterium, helium nuclei stability category (chemical element) form.
35 minutes after the Big Bang, after three hundred million degrees, nuclear process to stop, can not form a neutral atom.
Big Bang 30 years after 3000, the chemical combination of the role of neutral atoms so that the formation of the universe, the main components of gaseous substances, and graally the gravitational effect of self-cohesion, high-density gas into the clouds, until the stars and stellar systems.
According to the Hubble constant can be estimated around 150 million years ago, the universe began in a singular point.
Wenger. Wave Miao said: "The explosion 1 / 100 second when the temperature was 100 billion degrees Celsius, the universe at its most simple state of thermal equilibrium. From a purely energy generated by the photon and electron-positron blend together, even the mirage-like micro - This son also soak in hot soup pots (what we call soup of elementary particles) Lane. photon and proton ratio of 10 to 1. exploded one second after the temperature has dropped to 10 billion degrees Celsius, neutrinos begin to escape from the heat balance extricate . 3 minutes is a epoch-making time, the temperature has dropped to one billion degrees Celsius, electron-positron annihilation finish. the universe, mainly by light, positive and negative component neutrino, nuclear particles represents a very small share of one of the ratio of hydrogen and helium for 73 : 27. The other is by the annihilation of many particles with the same nuclear electron scarce. since there is no major event happened 70 million years, until the temperature has dropped to 3000 degrees Celsius, the free electron graally have their own owners, and nuclear form of hydrogen and helium, material was hot out of radiation balance, beginning the universe transparent.