Windows系统下(Linux和MAC系统下请自行了解清楚)NI的各种软件、模块、工具包、驱动程序,使用NI许可证管理器来激活的,绝大部分的都可以使用NI Lincense Activator来激活,以下链接可下载:
NI序列号Serial Number生成激活工具NI License Activator,LabVIEW/VBAI/VDM/VAS等软件模块工具包破解工具不限版本
http://pcmv.cn/thread-490-1-1.html
视觉论坛的各种资源,除了视觉相关的模块有使用外,大部分的都不会使用,所以仅提供资源不能提供技术支持。资源的下载地址一般会同时提供NI官方地址和百度网盘的下载地址。某些工具包NI的地址失效或没有NI的下载地址,那视觉论坛也没有办法,只能尝试使用百度网盘地址下载;如果百度网盘的下载地址失效过期,可联系论坛客服更新。现在NI的下载服务器对我国IP地址不是很友好,有些时候速度很慢或大的资源下载很容易出错,这样会造成安装过程各种类型报错而无法安装。建议在下载完成后,对下载资源做校验和验证(NI一般会提供MD5或SHA256等),与官方或视觉论坛提供的校验和对比,一致就可以安装,如果不一致,则需要重新下载。视觉论坛早期下载的资源,那时候NI没有这么多限制,基本上都是正常下载的资源;后期下载的资源,都与NI的正确校验和对比过,保证是正确的资源才上传到百度网盘,所以百度网盘的资源基本上是正确的。校验和工具下载地址:
文件Hash计算器FHash,文件校验和验证下载文件正确性验证,MD5值计算、SHA1值计算、SHA256值计算、CRC32值计算
http://pcmv.cn/thread-26524-1-1.html
LabVIEW 2010 Advanced Signal Processing Toolkit x86WinEng LabVIEW2010高级信号处理工具包ASPT2010 32位Windows英语版
ASPT工具包,在2009到2017年版本之间,有64位的测试版,但是NI官方一直到APST2018才正式发布64位版本。我方视觉论坛提供了ASPT2009-APST2017的64位版本下载。具体的可在本论坛搜索相应的版本。
LabVIEW高级信号处理工具包是一组软件工具,可用于执行时频分析、时序分析和小波分析。
LabVIEW高级信号处理工具包是LabVIEW的一个附加软件,提供有时频分析、时序分析和小波分析工具。该附加工具内含LabVIEW数字滤波器设计工具包,您可单独购买这一工具包。为了有效地提取信号隐藏的信息,应选择适当的分析工具。您可以将时频分析工具用于具有缓慢变化的光谱内容的进化信号,用于静止信号的时间序列分析工具,以及用于描述短时事件的进化信号和瞬态信号的小波分析工具。您还可以将分析代码部署到NI实时嵌入式硬件。
百度网盘下载地址(限速,请开会员或使用破解限速工具):
EXE版和ZIP版内容一样,EXE为NI当年发行版,ZIP为NI后期重新压制版本。
EXE版:
链接: 请注册视觉论坛用户,登陆后购买附件下载查看,充值请联系在线客服提取码: 请注册登陆视觉论坛会员,购买附件查看
ZIP版:
链接: 请注册视觉论坛用户,登陆后购买附件下载查看,充值请联系在线客服 提取码: 请注册登陆视觉论坛会员,购买附件查看
NI官方下载地址(可能无效或无法下载完成):
EXE版:
请注册登陆视觉论坛会员,购买附件查看
ZIP版:
请注册登陆视觉论坛会员,购买附件查看
LabVIEW 2010 Advanced Signal Processing Toolkit x86WinEng LabVIEW2010高级信号处理工具包ASPT2010 32位Windows英语版
http://pcmv.cn/thread-24259-1-1.html?fromuid=9
(出处: 视觉论坛VISIONBBS|视觉之家VISIONHOME)
LabVIEW 2010 Advanced Signal Processing Toolkit Readme
Overview
New Features and Changes
This version includes the following new VIs:
TSA Bicoherence—Use this VI to compute the bicoherence of a univariate time series.
WA Set Coefficients of Discrete Wavelet Transform—Use this VI to set specific coefficients that you compute from the discrete wavelet transform.
WA Set Coefficients of Integer Wavelet Transform—Use this VI to set specific coefficients that you compute from the integer wavelet transform.
WA Set Coefficients of Undecimated Wavelet Transform—Use this VI to set specific coefficients that you compute from the undecimated wavelet transform.
WA Online Detrend—Use this VI to remove the trend from 1D streaming signals by setting the approximation coefficients to zeros.
WA Online Multiscale Peak Detection—Use this VI to detect peaks or valleys in a streaming signal.
This version includes the following changed VIs:
initialize? (F) specifies whether the input block of data is the first block.
averaging parameters specifies how this VI computes the averaging.
averaging done? returns whether the averaging process is complete.
length specifies the length of the sliding window that divides the time series into subsequences.
frequency bins specifies the number of frequency bins for which this VI computes the bispectrum.
TSA Bispectrum—This VI includes the following new or changed parameters that enable this VI to examine whether the phase components at specific frequencies are coupled.
TSA MUSIC—The default value for noise subspace is –1, which means this VI calculates an appropriate value for noise subspace.
WA Multiscale Peak Detection—Use this VI to detect peaks or valleys in an offline signal.
TFA Dual Window—In previous versions, this VI contains the transform info and expansion info outputs. In this version, these outputs are replaced by the analysis info and synthesis info outputs.
Dual Window—In previous versions, this Express VI contains the transform info and expansion info outputs. In this version, these outputs are replaced by the analysis info and synthesis info outputs.
TFA Read from File, TSA Read from File, and WA Read from File—These VIs contain the number of rows, start of read offset, and delimiters inputs. Use the number of rows input to specify the maximum number of rows in a spreadsheet text file. Use the start of read offset input to specify the position in the file, measured in rows, to begin reading. Use the delimiters input to specify an array of strings used to separate fields in a spreadsheet text file.
WA Arbitrary Path Reconstruction—In previous versions, this VI contains the source input. In this version, this input is replaced by the source coefficients input. Use the source coefficients input to specify the coefficients for reconstructing a time waveform.
System Requirements
200 MB free disk space
LabVIEW 2010 Full or Professional Development System
Windows 7 (32-bit and 64-bit)
Windows Vista (32-bit and 64-bit)
Windows XP (32-bit)
Windows Server 2003 R2 (32-bit)
Windows Server 2008 R2 (64-bit)
Installation Instructions
LabVIEW Release Notes, which are available in your LabVIEW software kit.
LabVIEW 2010 Platform DVDs Readme, which is available on the top-level of LabVIEW Platform DVD 1.
Note: If you purchased this product with an NI Software Suite or NI Product Bundle, use the installation media that shipped with your purchase to install this product.Activation Notice
Accessing the Help
Finding Examples
Known Issues
Bug Fixes
Bug ID | Fixed Issue |
148996 | The TSA MUSIC Spectrum VI returns incorrect results for a multiple-tone pure signal |
215043 | WA WP Best Tree VI does not return the best tree in some corner cases |
215835 | Control values in ASPT Express VIs are not shown with Contrast Black OS color scheme |
Important Information