Linux-audio-dev

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7535 discussions

[LAD] Denemo is searching for a student for the Google Summer of Code (5000$)

by Nils

Hello list! Google Summer of Code (GSoC) is a global program that offers student developers stipends to write code for various open source software projects. A participating student gets 5000$ for ca. three months of work. [Link 1] Denemo is participating and we would like to encourage possible students to contact us through our mailinglist [see attached link 2] or #denemo on irc.freenode.org. Our top priority project is the following, but we are also ready for student ideas. "Make midi/audio output realtime-capable Denemo creates MIDI messages to use them with its internal Fluidsynth-sampler or send them out via the Jack Audio Connection Kit. This procedure is not realtime-safe yet. Graphical computation and controlling Denemo during playback creates playback-glitches. In order to fix this the midi/audio subsystem should run in its own realtime-thread and get priority. Needed student skills: Programming in C, experience in threads and realtime programming. Useful: Knowledge of MIDI and the Jack Audio Connection Kit." Links: [0] http://www.denemo.org [1] http://www.google-melange.com/ [2] http://www.denemo.org/index.php/Community [3] http://www.gnu.org/software/soc-projects/ideas-2011.html#denemo P.S. If you are not a student feel free do contact us anyway and help Denemo like the rest of the team :)

14 years, 10 months

[LAD] NASPRO 0.2.90 released

by Stefano D'Angelo

Hi all, I'm glad to announce the release of NASPRO 0.2.90. NASPRO (http://naspro.atheme.org/) is meant to be a cross-platform sound processing software architecture built around the LV2 plugin standard (http://lv2plug.in/). The goal of the project is to develop a series of tools to make it easy and convenient to use LV2 for sound processing on any (relevant) platform and for everybody: end users, host developers, plugin developers, distributors and scientists/researchers. This release is a total redesign/rewrite that more or less reimplements the features of the previous release, but in a much cleaner and maintainable way. It includes: * NASPRO core: the portable runtime library at the bottom of the architecture; * NASPRO Bridge it: a little helper library to develop insert-your-API-here to LV2 bridges; * NASPRO bridges: a collection of bridges to LV2 which, once installed, allow you to use plugins developed for other plugin standards in LV2 hosts. In particular, the NASPRO bridges collection includes two bridges: a LADSPA (http://www.ladspa.org/) 1.1 and a DSSI (http://dssi.sourceforge.net/) 1.0.0/1.1.0 bridge. All of the code is released under the LGPL 2.1 (http://www.gnu.org/licenses/lgpl-2.1.html) license. More information is available on the project's website. Enjoy! Stefano D'Angelo

14 years, 11 months

[LAD] [ANN] first release of flarps

by Lieven Moors

I would like to announce the release of flarps-0.1.0 Flarps is an arpeggiator for Linux. It uses JACK MIDI to generate melodies, and it can be controlled live by editing a text file in a simple text-editor. Flarps is designed around the notion of 'steps'. A step describes the relative distance between two MIDI notes, and has a horizontal and a vertical component. Vertically, a difference in pitch is specified, and horizontally a distance in time (rhythm). You can find a lot more information about flarps here: http://flarps.sourceforge.net/ You can download it directly at: http://sourceforge.net/projects/flarps/files/flarps-0.1.0.tar.bz2/download Or you can clone the git repository with: git clone git://flarps.git.sourceforge.net/gitroot/flarps/flarps For bug reports, feature requests, support requests etc., please use the facilities at the sourceforge project site. New ideas or patches for this project are very welcome. If you want to collaborate on this project, you can find me on the linux-audio-dev mailing list. lievenmoors

14 years, 11 months

[LAD] QT3 and KDE3 removal in Debian

by Adrian Knoth

Hi! I guess this could be important for some of you: Debian is currently dropping QT3 and KDE3 from unstable. This in turn means that apps depending on those libs either need to be ported to QT4/KDE4 or will also be removed. As always, saying Debian sooner or later also means Ubuntu and derivatives. Of course, all software remains installable from squeeze (current release) for the next few years (let me lie: 5?). I know that fmit and creox use QT3, probably some other audio software, too. The creox author has no time for porting, so if somebody feels bored or is looking for a little project, you might want to consider this. Cheers -- mail: adi(a)thur.de http://adi.thur.de PGP/GPG: key via keyserver

14 years, 11 months

Re: [LAD] FFT 1D real

by Alfs Kurmis

Citējot *Fons Adriaensen <fons(a)linuxaudio.org> [1]*: > > How from ...1024 or 2048 or 4096... FFT return values i > calculate > > power magnitudes for all bands, > > and finally values for visual 10-20 hopping bars, like in > Winamp , > > XMMS , QMMP ... ? > > If you want such a display the FFT is not a good way to do it. > It's possible but not simple if you want a correct result. What is good/best way to calculate values for visual 10-20 hopping bars like in GUI audio players ? > > 43303.2715 + 796.7285 = 44100 or 44100 - 43303.2715 = > 796.7285> > > Why Frequency 796.7285 is mirrored as Frequency 43303.2715 , > and magnitude for both Frequencies is divided by 2 ???? > > Because you are using a complex FFT, and the imaginary part > of your signal is zero. That means that the spectrum must be > symmetric. > > > Is here way direct calculate full magnitude and without > Frequency > > mirroring , in band 0 Hz ... FSampl/2 ONLY , > > Use an FFT operating on real data instead of complex. Can U gimme pointers to such functions ? What about all Radix algorithms ? Tnx in advance Alf ---------- Pārsūtītās vēstules beigas ---------- Links: ------ [1] mailto:fons@linuxaudio.org

14 years, 11 months

[LAD] FFT 1D real

by Alfs Kurmis

Hi Experts. I am Physics student, and i wanna write referat about Fourier transformations, also about FFT 1D real case. Hope this is best place for ask this, and here are best experts. I wanaa demonstrate how diverse window functions changes measured spectrum, how much CPU ressources take diverse FFT algorithms ... Yet i understand [i hope so] how works windowing . Is somewhere available copy-paste self contained C example functions or makros for diverse FFT algorithms FFT, QFT, Goertzel, radix-2, radix-4, split-radix, mixed-radix ... ? Which variables in FFT function must/should be defined as static, register ... for best performance ? What typical comes in to FFT function ? Pointer to already windowed array of samples ? What return FFT ? What exact physical dimensions return FFT , if input function dimensions was - voltage depends from (time) U=U(t) ? How from ...1024 or 2048 or 4096... FFT return values i calculate power magnitudes for all bands, and finally values for visual 10-20 hopping bars, like in Winamp , XMMS , QMMP ... ? If i exact know my FFT window size [for example 4096 samples] and window type , and it will be constant forever, is it possible to calculate window(,sine,cosine,) and store all values in constant array, so that in runtime it do not need be calculated , but i can just take values form array ? I have google_d about FFT and have found such proggie [see below] I have it little bit remixed , i generate pure sine frekwenz = 796.7285 HZ , and in output file i got so what : [ 71] 764.4287 Hz: Re= 0.0000000011142182 Im= 0.0000002368905824 M= 0.0000002368932028 [ 72] 775.1953 Hz: Re= 0.0000000011147694 Im= 0.0000003578625618 M= 0.0000003578642981 [ 73] 785.9619 Hz: Re= 0.0000000011164234 Im= 0.0000007207092628 M= 0.0000007207101275 [ 74] 796.7285 Hz: Re=-0.0000022785007614 Im=-0.5000000048748561 M= 0.5000000048800476 [ 75] 807.4951 Hz: Re= 0.0000000011098065 Im=-0.0000007304711756 M= 0.0000007304720186 [ 76] 818.2617 Hz: Re= 0.0000000011114605 Im=-0.0000003676273975 M= 0.0000003676290776 [ 77] 829.0283 Hz: Re= 0.0000000011120118 Im=-0.0000002466579503 M= 0.0000002466604569 ... ... ... [4019] 43270.9717 Hz: Re= 0.0000000011120118 Im= 0.0000002466579503 M= 0.0000002466604569 [4020] 43281.7383 Hz: Re= 0.0000000011114605 Im= 0.0000003676273975 M= 0.0000003676290776 [4021] 43292.5049 Hz: Re= 0.0000000011098065 Im= 0.0000007304711756 M= 0.0000007304720186 [4022] 43303.2715 Hz: Re=-0.0000022785015510 Im= 0.5000000048748419 M= 0.5000000048800334 [4023] 43314.0381 Hz: Re= 0.0000000011164234 Im=-0.0000007207092628 M= 0.0000007207101275 [4024] 43324.8047 Hz: Re= 0.0000000011147694 Im=-0.0000003578625618 M= 0.0000003578642981 [4025] 43335.5713 Hz: Re= 0.0000000011142182 Im=-0.0000002368905824 M= 0.0000002368932028 Where 43303.2715 + 796.7285 = 44100 or 44100 - 43303.2715 = 796.7285 Why Frequency 796.7285 is mirrored as Frequency 43303.2715 , and magnitude for both Frequencies is divided by 2 ???? Is here way direct calculate full magnitude and without Frequency mirroring , in band 0 Hz ... FSampl/2 ONLY , and not in full band - 0 Hz ... FSampl ?? In this case - how do i calculate corresponding frequency of each band that returns FFT, if sample frequency is 32K, 44K or 48K ? Pleaz do not point me to FFTW[3] and such libs , i must self write/combine code . Except FFTW has best short self contained 1D functions for copy-paste :) Each pointer and example is welcomed. Tnx in advance @ all. Alfs Kurmis. ==== #include <stdio.h> #include <stdlib.h> #include <string.h> #include <ctype.h> #include <math.h> #define BUFFER 4096 //2048 //#define BUFFER 256 # define M_PI_LD 3.1415926535897932384626433832795029L /* pi */ //void readwave(const char *filename, double *tr); short FFT(short int dir, long m, double *x, double *y); double fstep; int main (int argc, char *argv []) { int i; double f = 0.0; double amplitude = 0.; double samplerate = 44100., frekwenz=796.7285; double xarg=0. , argplus = 0. , pti ; double real[BUFFER], img[BUFFER]; // ==== ===== argplus = ( frekwenz *2.0*M_PI )/samplerate; //printf("Reading %d bytes from %s.rn", BUFFER, argv[1]); for(i=0;i<BUFFER;i++) { // xarg=0.0; argplus=0.2; floarArg =0.0001; pti = sin ( xarg ) /* * 32767.0*/ ; /*if ( kante>0 ) { if( pti > 0.0 ){ pti = 23767.0; }else{pti = -23767.0;} } /**/ xarg = xarg +argplus;//+floarArg; if ( xarg > (4.0*M_PI) ) xarg = xarg - (4.0*M_PI); real[i] = pti; } printf("F= %7.2f Hz nn", (samplerate*argplus)/(2*M_PI) ); memset(img, 0, sizeof(img)); /* Fill all the imaginary parts with zeros */ //fstep = (double) samplerate / (double) (BUFFER*2); fstep = (double) samplerate / (double) (BUFFER); printf("Frequency step : %10.6frn", fstep); FFT(1, /*11*/ 12, real, img); /* Fast Fourier Transform with 2^11 bins */ // FFT(1, 7, real, img); /* Fast Fourier Transform with 2^11 bins */ /* Write fourier transformed data to stdio */ i = 0; while(i < BUFFER) { amplitude = sqrt((real[i]*real[i]) + (img[i]*img[i])); //printf("(%4d) %.2f Hz: Re=%f Im=%f P=%frn", i, f, real[i], img[i], amplitude); printf("[%4d] %8.4f Hz: Re=%22.16f Im=%22.16f M=%22.16fn", i, f, real[i], img[i], amplitude); i++; f += fstep; } return 0 ; } // main /* This computes an in-place complex-to-complex FFT x and y are the real and imaginary arrays of 2^m points. dir = 1 gives forward transform dir = -1 gives reverse transform */ short FFT(short int dir, long m, double *x, double *y) { long n,i,i1,j,k,i2,l,l1,l2; double c1,c2,tx,ty,t1,t2,u1,u2,z; /* Calculate the number of points N = M ^2 */ n = 1; for (i=0;i<m;i++) n *= 2; printf("FFT -->> (n) 2 ^ %ld = %ldn", m, n); /* Do the bit reversal */ i2 = n >> 1; j = 0; for (i=0;i<n-1;i++) { if (i < j) { tx = x[i]; ty = y[i]; x[i] = x[j]; y[i] = y[j]; x[j] = tx; y[j] = ty; } k = i2; while (k <= j) { j -= k; k >>= 1; } j += k; } // for (i=0;i<n-1;i++) /* Compute the FFT */ c1 = -1.0; c2 = 0.0; l2 = 1; for (l=0;l<m;l++) { l1 = l2; l2 <<= 1; u1 = 1.0; u2 = 0.0; for (j=0;j<l1;j++) { for (i=j;i<n;i+=l2) { i1 = i + l1; t1 = u1 * x[i1] - u2 * y[i1]; t2 = u1 * y[i1] + u2 * x[i1]; x[i1] = x[i] - t1; y[i1] = y[i] - t2; x[i] += t1; y[i] += t2; } z = u1 * c1 - u2 * c2; u2 = u1 * c2 + u2 * c1; u1 = z; } c2 = sqrt((1.0 - c1) / 2.0); if (dir == 1) c2 = -c2; c1 = sqrt((1.0 + c1) / 2.0); } /* Scaling for forward transform */ if (dir == 1) { for (i=0;i<n;i++) { x[i] /= n; y[i] /= n; } } return(1); //return(TRUE); } ----

14 years, 11 months

[LAD] Normalize and Cut Wav

by Alfs Kurmis

Hi experts. I have started my small project - mp3 database for radio. http://martini.pudele.com/radio/mp3_database/mp3_database.html How do i normalize by peak [not RMS] and trim silences in begin and end of WAV files ? Silences somewhere in middle of file i wanna leave untouched. I wanna in first step detect MAX sample in whole WAV file. For example we gotta MAX sample 10 000, then Apmliefier_coefficient will be 32 000/10 000 = 3,2 . In second step i wanna trim silences at begin and below -80 dB [or 2 bit noise] For this in same file each sample multiple by Apmliefier_coefficient , and see - result is over -80 dB or not. If not, then first N samples will not written in trimmed file, but first sample that is over -80 dB [in any channel] , and all further samples written in new file. Now we must just follow which sample [in any channel] is over -80 dB. After write is complete, we can just truncate after last sample that was over -80 dB, and write header. So far i have found SOX vanna reverse da file for end silence trim, and for each step produce tmp file. Is here C API , program, script, way to do so what without any temporary files ? I have written script for normalize, but what ir best way for normalize ? What about mp3 and ogg automatic normalize and frames trim ? Tnx in advance Alf ==== #!/bin/bash for i in *.wav; do val=${i%.wav} echo "** Check peak for $i **" ampl=`sox "$i" -t wav /dev/null stat -v 2>&1` waveaus=${i%.wav}.wave wert1="1.1"; wert2=$ampl; wahr=$(echo "$wert1 > $wert2" | bc) if [ $wahr = 1 ]; then echo " $wert1 > $wert2 , Do Nuthin" else echo " $wert1 <= $wert2 , Do process" echo "** Amplifying volume by -=$ampl=- to fake a normalize $val.wav -- $waveaus" ampl2=$(echo $ampl*0.9995 | bc -l) echo "ampl2 = $ampl2" sox -v $ampl2 "$i" -t wav "$waveaus" fi echo "" done ----

14 years, 11 months

[LAD] Permafrost guitar amp, was Re: RDF libraries, was Re: [ANN] IR: LV2 Convolution Reverb

by Giuseppe Zompatori

From: Stefano D'Angelo <zanga.mail(a)gmail.com> Date: 2011/2/27 Subject: Re: [LAD] RDF libraries, was Re: [ANN] IR: LV2 Convolution Reverb To: Giuseppe Zompatori <siliconjoe(a)gmail.com> Cc: linux-audio-dev(a)lists.linuxaudio.org 2011/2/27 Stefano D'Angelo <zanga.mail(a)gmail.com>: > > > Ciao Giuseppe, > Ciao Stefano, Taking this email to a new thread. >Well... they seem to have a lot of stuff there. :-) > >However, I wonder how they do it... I think they are probably using >some black box modeling, since multiple nonlinearities+feedback in a >single system is very hard to model. > They are very silent on this sadly, don't know what they are doing. > >The kind of stuff I'm trying to do is accurately model a class A amp >with a single triode using white box techniques... to give you an idea >of what it sounds like see this: >http://www.youtube.com/watch?v=cdNtmaIdLdo - it is part of my MSc >thesis presentation (100.000 lire guitar, dated and slow laptop, cheap >speaker and cheap camera... only the sound card is good). > >I guess you speak Italian (at least your name suggests that), so enjoy >my weird southern accent. :-P > Very interesting, I tried compiling your thesis with permafrost to try this out (obtaining the source from the pdf has been hell BTW) but it bails with an "m_pi" undeclared input/output function... Anyway, are you limited to the simulation of a half triode with white box techniques? I think you should model at least both halves of a triode if you're after accuracy, a single triode amplifier won't even work in real life (I build tube amps, I know) ;) Also class A amplifiers aren't very popular amongst guitar players (mainly because of their clipping behavior). You also want a multi-stage preamp with different filtering/biasing points between stages. You might think I am crazy but that's what you'll discover yourself by observing schematics to popular guitar amps. Here's a simple (early Fender-like) amp topology: Tube n. 1 ------------------------------------------------------- Tube n. 2 Tube n. 3 and 4 | | | | 1st triode -> Tone stack -> post tone stack recovery triode -> P.I. (Phase inverter) triodes -> (at least 2) Pentodes -> O.T. (Output Transformer) -> Speakers ^ ^ | | Presence pot<--------------------------------negative-feedback--------------------------------------------- This is the easiest PP (Push Pull) class A/B amp I could come up with (sounds pretty darn good in real life). It has got a tone stack, 4 tubes (2 triodes and two pentodes) and an OT/speakers, do you think this is feasible computational-wise with permafrost? >Well, they say guitarix has improved, yet the last time I was all but >satisfied with it. You may want to take a look at invada plugins, if >you haven't already. Invada has a simple generic tube drive function AFAIK, I still prefer the CAPS* amp over it as it's at least based on a real amp. >Stammi bene, > >Stefano Anche tu! -Giuseppe

14 years, 11 months

[LAD] Finding Deadlock causes in multithreaded C++ using gdb

by Harry Van Haaren

Hey guys, I'm working on a mulithreaded version of my pet project, and I've now managed to deadlock one thread, which in turn makes the GUI thread wait for a mutex lock, and then finally segfaults the whole program :-) So I'm looking for pointers on how best to find a deadlock's cause using gdb? Other advice / good articles on the topic etc welcome! Thanks for reading, -Harry

14 years, 11 months

[LAD] Litmus RT kernel

by michael noble

hi all, I just came across this: http://www.cs.unc.edu/~anderson/litmus-rt/index.html. From the site: The LITMUSRT project is a soft real-time extension of the Linux kernel with > focus on multiprocessor real-time scheduling and synchronization. The Linux > kernel is modified to support the sporadic task model and modular scheduler > plugins. Both partitioned and global scheduling is supported. > It seems their latest patch is against 2.6.36. I realize this is not a plug and play alternative to Ingo's work by any means, but I was wondering if anyone more knowledgeable has some insight into what exactly the Litmus kernel may offer... -michael

14 years, 11 months

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Linux-audio-dev