怎樣查找big文件

⑴ big文件是什麼怎樣使用

big文件一般是游戲中的文件，比較常見的用途是裝載游戲的音樂、聲音等文件。很多人游戲背景音樂都是從big文件中提取的，使用XCC
Mixer
軟體就可以輕松辦到，但最好只提取文件，千萬不要亂改其中的內容，不然就bug了。

⑵ 紅警3big文件放哪裡有效

都有效
在桌面「紅警3」圖標上單擊右鍵，屬性
在目標那一欄後加上-ui（注意-ui前要有空格）
然後啟動運行，會出現一個窗口 選擇Select Language（好像是，反正有一個Language），然後選擇Chinese（T），就OK

⑶ 請問如何打開.big文件

復制到FIFA2006安裝目錄下的相同文件就可以了
參考資料：http://hi..com/coolplay

⑷ 跪求`! . Big 文件格式打開方法`

Arial Audio Converter V2.3.6┊專業的音頻格式批量轉換工具┊漢化綠色特別版 一款專業的音頻轉換工具。 它可以在P3, WMA,OGG,MP2,WAV( PCM, DSP, GSM, ADPCM ), G721, G723, G726, VOX, ALAW, ULAW等聲音格式之間相互轉換。 使用這款非常易用的軟體你可以批量轉換文件而不必理會它們的源文件格式和目標文件格式。 Arial Audio Converter通過其內置播放器也支持播放功能。 http://www.greendown.cn/soft/2660.html天天音頻轉換專家 V5.61 綠色下載站專用破解免安裝貴賓版『天天音頻轉換專家』是一款專業的音頻轉換工具。 支持MP2, MP3, AAC, AC3, WMA, OGG, AMR, WAV( PCM, DSP, GSM, ADPCM ), G721, G723, G726, G729, VOX, ALAW, ULAW等常見的音頻格式之間的轉換。 可以批量轉換文件而不必理會它們的源文件格式和目標文件格式。 內置播放器支持多種格式的播放功能。 主要特點： ★在MP2, MP3, AAC, AC3, WMA, OGG, WAV( PCM, DSP, GSM, ADPCM), G721, G723, G726, G729, VOX, ALAW, ULAW等聲音格式之間按不同的設置進行相互轉換； ★支持3G音頻格式--AMR； ★支持同一種音頻格式在不同壓縮率下的轉換； ★支持批量音頻文件轉換； ★支持ID3標簽顯示和編輯； ★內置播放器支持流行的音樂格式播放； ★用戶界面友好，非常易於使用。隨意注冊即可用法：運行「綠化.exe」即可正常使用。運行「卸除.exe」即可卸除綠化時加到系統的東西。 http://www.greendown.cn/soft/2840.html

⑸ 如何打開.big文件

你安裝一個虛擬光碟機軟體，載入.big文件就能打開了

⑹ BIG格式的文件怎麼打開 謝了

聽過JEPG 和GIF的圖片格式但是沒聽過BIG格式的 你確定是這個格式？ 可能只是文件名字而已，你把後綴名隱藏了，點擊上面的文件選項 顯示後綴名再看看

⑺ 請問用什麼軟體可以解壓提取後綴名為big的文件

.big是種游戲裡面的音樂格式文件吧，要取得音樂文件，三個步驟：

1、提取音樂文件

2、將 aifc 轉換為 wav 格式

3、因為 wav 格式文件很大，再將其轉為其他各式（如MP3）。

一、提取音樂文件

1、下載HW2MusicTools.zip。

2、解壓之後有兩個 ZIP 包，一個是 HW2ICArchive.zip，用於讀取和解壓 big 文件。另一個 In_Aif.zip 是 WinAmp 的解碼插件，用於播放 aifc 格式的音樂。

3、解壓 HW2ICArchive.zip，運行當中的 HW2ICArchive.exe。如果出現錯誤，你就需要先將同目錄下的另外兩個 .dll 文件注冊。

4、這個工具的用法我就不多說了，大家稍微摸索一下就能明白的。用它把 Music.big 中的所有文件解壓出來，然後將所有的 .fda 文件重命名為 .aifc 格式。 .lua 的文件不管他，刪掉。

⑻ 怎樣打開*.big文件

你安裝一個虛擬光碟機軟體，載入.big文件就能打開了

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

⑼ 提取BIG文件

推薦使用XCC系列軟體~~~

⑽ 有關big文件的提取問題。

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.