Free 7.25 inches in mm software for linux

Print Plug-In provides a basic printing capability for The GIMP.
The current release supports PostScript, PCL (HP LaserJet and DeskJet), and ESC/P2 (EPSON Stylus Color) printers. The PostScript printer drivers handle PPD (PostScript Printer Description) files if you have them.
Using the Print Plug-In:
The Printer option provides selections for many common printers. Currently the print plug-in supports the following printers:
- PostScript printers
- HP DeskJet 500, 500C, 520, 540C, 600C, 660C, 68xC, 69xC, 850C, 855C, 855Cse, 855Cxi, 870Cse, 870Cxi, 1100C, 1120C, 1200C, and 1600C printers
- HP LaserJet II, III, IIIp, IIIsi, 4, 4L, 4P, 4V, 4Si, 5, 5FS, 5L, 5P, 5SE, 5Si, 6L, 6P printers
- EPSON Stylus Color, Color Pro, Color Pro XL, Color 400, Color 500, Color 600, Color 800, Color 1500, Color 1520, and Color 3000.
The Output Type option controls whether the printed output is in color or B&W (grayscale). This option is silently forced to B&W for grayscale images and B&W-only printers.
The Media Size option controls the size of the output. By default images are printed to fit the page and are automatically rotated to fill the largest area possible.
The Media Type option tells the printer what type of media is being used (Plain, Coated, etc). Not all printers support the media type option.
The Media Source option tells the printer which paper tray to print from. Not all printers support the media source option.
The Resolution option controls the resolution of the output. Not all printers support the resolution option.
The Orientation option controls whether the output is automatically rotated for maximum page coverage (Auto) or set to a specific orientation (Portrait or Landscape).
The Scaling option controls how large the printed image is. The default is to scale to a percentage of the printable area of the page. You can also specify an image resolution in pixels-per-inch (PPI) by clicking on the PPI radio button. The image is centered by default, however you can adjust the position of the image on the page by dragging the preview image.
The Brightness option controls the overall printed image brightness. A brightness of 100 is usually good for most B&W and PostScript printers, while most inkjet printers need a brightness between 100 and 120 for acceptable results.
Printing to a File
If you want to print to a file, select File from the Printer list. A file chooser dialog is displayed when you press the Print button. Warning, when you print to a file any existing file will be silently overwritten by this release of the plug-in!
Layered Images
Like most plug-ins, the print plug-in only reads the image from the active layer. If you want to print a composite of all visible layers you need to merge the layers (CTRL-M) and then print.
Supported Printers/Features
Most of the printer drivers in the print plug-in use the highest supported resolution for a printer, with the following exceptions:
- EPSON Stylus Color 600, 800, 1520, and 3000 - Currently the driver only supports 720 DPI printing in "compatibility" mode. This makes the drivers extremely slow compared to the Windows and Mac drivers. Unfortunately, I cannot provide optimized drivers (nor drivers for 1440x720) because of our NDA with EPSON.
- EPSON Stylus Photo, Photo Ex, Photo 700 - Currently the driver only supports 720 DPI printing in "compatibility" mode. This makes the drivers extremely slow compared to the Windows and Mac drivers, and you dont get the use of the light cyan and magenta inks (again, because of NDA restrictions.)

Music::Scales can supply necessary notes / offsets for musical scales.

SYNOPSIS

use Music::Scales;

my @maj = get_scale_notes(Eb); # defaults to major
print join(" ",@maj); # "Eb F G Ab Bb C D"
my @blues = get_scale_nums(bl); # bl,blu,blue,blues
print join(" ",@blues); # "0 3 5 6 7 10"
my %min = get_scale_offsets (G,mm,1); # descending melodic minor
print map {"$_=$min{$_} "} sort keys %min; # "A=0 B=-1 C=0 D=0 E=-1 F=0 G=0"

Given a keynote A-G(#/b) and a scale-name, will return the scale, either as an array of notenames or as a hash of semitone-offsets for each note.

METHODS

get_scale_nums($scale[,$descending])

returns an array of semitone offsets for the requested scale, ascending/descending the given scale for one octave. The descending flag determines the direction of the scale, and also affects those scales (such as melodic minor) where the notes vary depending upon the direction. Scaletypes and valid values for $scale are listed below.

get_scale_notes($notename[,$scale,$descending,$keypref])

returns an array of notenames, starting from the given keynote. Enharmonic equivalencies (whether to use F# or Gb, for instance) are calculated based on the keynote and the scale. Basically, it attempts to do the Right Thing if the scale is an 8-note one, (the 7th in G harmonic minor being F# rather than Gb, although G minor is a flat key), but for any other scales, (Chromatic, blues etc.) it picks equivalencies based upon the keynote. This can be overidden with $keypref, setting to be either # or b for sharps and flats respectively. Cruftiness abounds here.

get_scale_offsets($notename[,$scale,$descending,$keypref])

as get_scale_notes(), except it returns a hash of notenames with the values being a semitone offset (-1, 0 or 1) as shown in the synopsis.

get_scale_MIDI($notename,$octave[,$scale,$descending])

as get_scale_notes(), but returns an array of MIDI note-numbers, given an octave number (-1..9).

get_scale_PDL($notename,$octave[,$scale,$descending])

as get_scale_MIDI(), but returns an array of PDL-format notes.

is_scale($scalename)

returns true if $scalename is a valid scale name used in this module.

kEchoSub is a small script lets You create subtitles "from scrath". When You want to make a translation for a movie and there are no subtitles available on the net even in other languages You can use this script.

Since version 0.2 it can also convert time stamps to hh:mm:ss with add zeros button. For example it can convert a timestamps like 1:22:3 to 01:22:03 format making it readable for some stupid video players which cant rad 1:22:3 format.

Since version 0.2 it can also add minumum time to read a subtitle line - different for long lines and short lines. You cna set the options "Characters per lon g line" to indicate how much characters doesn the line have to have to be considered LONG in Your opinion.

Ths script will then calculate the time spaces in seconds beteween the lines and it its too short itll put a | mark instead of timestampt so the video player will display the second time without erasing the preaviouse line from the screen.

online.php analyses /var/log/ppp-usage and displays connection statistics. It also prints some information about your current PPP connection.
Well, I was inspired by the script Onlinecalc by Michael Schlenstedt (Michael@adsl4linux.de). His script is heavily based upon "calc" by Ulrich Schmitz.
Since Onlinecalc did not fit my needs, I did a complete rewrite in php.
Main features:
- reads /var/log/ppp-usage and prints a table with a row for each month.
- also calculates the values of the current connection.
- completely written in PHP.
- display connect-time as dd:hh:mm:ss
- display volumes as 123 456 789,12 MB
- displays chronologically (maybe I will change the sorting later to reverse)

Games::Mastermind is a simple framework for MasterMind games.

SYNOPSIS

use Games::Mastermind;

# the classic game
$mm = Games::Mastermind->new;

# make a guess
$marks = $game->play(qw( Y C W R ));

# results
print "You win!n" if $marks->[0] == $mm->holes();

# the game history is available at all times
$history = $mm->history();
$last_turn = $mm->history()->[-1];

# reset the game
$mm->reset();

Games::Mastermind is a very simple framework for running Mastermind games.

IDS::Algorithm::MM is a Perl module created to learn or test using a first-order Markov Model (MM).

SYNOPSIS

A usage synopsis would go here. Since it is not here, read on.
In section 4.2 in Kruegel and Vignas paper, they ignored the probability information that the MM provided, and produced a binary result. In effect, they were using the constructed MM as a {N,D}FA.

Someday more will be here.

Ideally, we would be using the algorithm from stolcke94bestfirst. Constructing a DFA rather than a NFA in effect has performed most of the state merging that stolcke93hidden do.

Consider also a java or C/C++ implementaion: http://www.ghmm.org/ http://www.run.montefiore.ulg.ac.be/~francois/software/jahmm/

Useful information: http://www.cs.brown.edu/research/ai/dynamics/tutorial/Documents/HiddenMarkovModels.html http://www.comp.leeds.ac.uk/roger/HiddenMarkovModels/html_dev/main.html L R Rabiner and B H Juang, `An introduction to HMMs, IEEE ASSP Magazine, 3, 4-16.

printvcg

printvcg(filehandle)

Print in a form usable by VCG for printing the DFA.

If the filehandle is specified, print there; otherwise, print to STDOUT.
This code was stolen from DFA, and does not know about the probabilities.
load(filehandle)

Load a MM from a file; this is the inverse of "print", and the format we expect is that used in $self->print.

test(tokensref, string, instance)

Test the string of tokens and calculate the probability of the string being seen. At each stage, we get a p in [0,1]. The result is the product of these probabilities.
Note that if a transition cannot be made, we return a 0 probability.

add(tokensref, string, instance)

The collection of tokens (in the list referenced by tokensref) is a complete example of a list that should be accepted by the DFA.

string and instance are IDS::Test framework arguments that we ignore because we do not need them.

WE add the transition from the last token to the (ACCEPT) state.

add_transition(from, token)

Add a transition from one state to another when the specified token is received. It is not an error to try to add an existing transition. In that event, this function quietly returns. If no such transition exists, we look for a transition on the token; if so, we add an edge to the destination node for the existing edge. Finally, if there is no other choice, we create a new state and add the edge.

generalize()

Reduce the number of states in the model.

Our building a DFA rather than a NFA has in effect performed most of the state merging that would have occurred.

XXX We should still be doing some checks for additional merge possibilities.
XXX A proof that the DFA is effectively the NFA with merged states would be useful.

Math::NumberCruncher Perl module contains a collection of useful math-related functions.

SYNOPSIS

It should be noted that as of v4.0, there is now an OO interface to Math::NumberCruncher. For backwards compatibility, however, the previous, functional style will always be supported.

# OO Style

use Math::NumberCruncher;

$ref = Math::NumberCruncher->new();

# From this point on, all of the subroutines shown below will be available # through $ref (i.e., ( $high,$low ) = $ref->Range( @array )). For the sake # of brevity, consult the functional documentation (below) for the use # of specific functions.

# Functional Style

use Math::NumberCruncher;

($high, $low) = Math::NumberCruncher::Range(@array);
$mean = Math::NumberCruncher::Mean(@array);
$median = Math::NumberCruncher::Median(@array [, $decimal_places]);
$odd_median = Math::NumberCruncher::OddMedian(@array);
$mode = Math::NumberCruncher::Mode(@array);
$covariance = Math::NumberCruncher::Covariance(@array1, @array2);
$correlation = Math::NumberCruncher::Correlation(@array1, @array2);
($slope, $y_intercept) = Math::NumberCruncher::BestFit(@array1, @array2 [, $decimal_places]);
$distance = Math::NumberCruncher::Distance($x1,$y1,$z1,$x2,$y2,$z2 [, $decimal_places]);
$distance = Math::NumberCruncher::Distance($x1,$y1,$x1,$x2 [, $decimal_places]);
$distance = Math::NumberCruncher::ManhattanDistance($x1,$y1,$x2,$y2);
$probAll = Math::NumberCruncher::AllOf(0.3,0.25,0.91,0.002);
$probNone = Math::NumberCruncher::NoneOf(0.4,0.5772,0.212);
$probSome = Math::NumberCruncher::SomeOf(0.11,0.56,0.3275);
$factorial = Math::NumberCruncher::Factorial($some_number);
$permutations = Math::NumberCruncher::Permutation($n);
$permutations = Math::NumberCruncher::Permutation($n,$k);
$roll = Math::NumberCruncher::Dice(3,12,4);
$randInt = Math::NumberCruncher::RandInt(10,50);
$randomElement = Math::NumberCruncher::RandomElement(@array);
Math::NumberCruncher::ShuffleArray(@array);
@unique = Math::NumberCruncher::Unique(@array);
@a_only = Math::NumberCruncher::Compare(@a,@b);
@union = Math::NumberCruncher::Union(@a,@b);
@intersection = Math::NumberCruncher::Intersection(@a,@b);
@difference = Math::NumberCruncher::Difference(@a,@b);
$gaussianRand = Math::NumberCruncher::GaussianRand();
$ways = Math::NumberCruncher::Choose($n,$k);
$binomial = Math::NumberCruncher::Binomial($attempts,$successes,$probability);
$gaussianDist = Math::NumberCruncher::GaussianDist($x,$mean,$variance);
$StdDev = Math::NumberCruncher::StandardDeviation(@array [, $decimal_places]);
$variance = Math::NumberCruncher::Variance(@array [, $decimal_places]);
@scores = Math::NumberCruncher::StandardScores(@array [, $decimal_places]);
$confidence = Math::NumberCruncher::SignSignificance($trials,$hits,$probability);
$e = Math::Numbercruncher::EMC2( "m512", "miles" [, $decimal_places] );
$m = Math::NumberCruncher::EMC2( "e987432" "km" [, $decimal_places] );
$force = Math::NumberCruncher::FMA( "m12", "a73.5" [, $decimal_places] );
$mass = Math::NumberCruncher::FMA( "a43", "f1324" [, $decimal_places] );
$acceleration = Math::NumberCruncher::FMA( "f53512", "m356" [, $decimal_places] );
$predicted_value = Math::NubmerCruncher::Predict( $slope, $y_intercept, $proposed_x [, $decimal_places] );
$area = Math::NumberCruncher::TriangleHeron( $a, $b, $c [, $decimal_places] );
$area = Math::NumberCruncher::TriangleHeron( 1,3, 5,7, 8,2 [, $decimal_places] );
$perimeter = Math::NumberCruncher::PolygonPerimeter( $x0,$y0, $x1,$y1, $x2,$y2, ... [, p$decimal_places]);
$direction = Math::NumberCruncher::Clockwise( $x0,$y0, $x1,$y1, $x2,$y2 );
$collision = Math::NumberCruncher::InPolygon( $x, $y, @xy );
@points = Math::NumberCruncher::BoundingBox_Points( $d, @p );
$in_triangle = Math::NumberCruncher::InTriangle( $x,$y, $x0,$y0, $x1,$y1, $x2,$y2 );
$area = Math::NumberCruncher::PolygonArea( 0, 1, 1, 0, 2, 0, 3, 2, 2, 3 [, p$decimal_places] );
$area = Math::NumberCruncher::CircleArea( $diameter [, $decimal_places] );
$circumference = Math::NumberCruncher::Circumference( $diameter [, $decimal_places] );
$volume = Math::NumberCruncher::SphereVolume( $radius [, $decimal_places] );
$surface_area = Math::NumberCruncher::SphereSurface( $radius [, $decimal_places] );
$years = Math::NumberCruncher::RuleOf72( $interest_rate [, $decimal_places] );
$volume = Math::NumberCruncher::CylinderVolume( $radius, $height [, $decimal_places] );
$volume = Math::NumberCruncher::ConeVolume( $lowerBaseArea, $height [, $decimal_places] );
$radians = Math::NumberCruncher::deg2rad( $degrees [, $decimal_places] );
$degrees = Math::NumberCruncher::rad2deg( $radians [, $decimal_places] );
$Fahrenheit = Math::NumberCruncher::C2F( $Celsius [, $decimal_places] );
$Celsius = Math::NumberCruncher::F2C( $Fahrenheit [, $decimal_places] );
$cm = Math::NumberCruncher::in2cm( $inches [, $decimal_places] );
$inches = Math::NumberCruncher::cm2in( $cm [, $decimal_places] );
$ft = Math::NumberCruncher::m2ft( $m [, $decimal_places] );
$m = Math::NumberCruncher::ft2m( $ft [, $decimal_places] );
$miles = Math::NumberCruncher::km2miles( $km [, $decimal_places] );
$km = Math::NumberCruncher::miles2km( $miles [, $decimal_places] );
$lb = Math::NumberCruncher::kg2lb( $kg [, $decimal_places] );
$kg = Math::NumberCruncher::lb2kg( $lb [, $decimal_places] );
$RelativeStride = Math::NumberCruncher::RelativeStride( $stride_length, $leg_length [, $decimal_places] );
$RelativeStride = Math::NumberCruncher::RelativeStride_2( $DimensionlessSpeed [, $decimal_places] );
$DimensionlessSpeed = Math::NumberCruncher::DimensionlessSpeed( $RelativeStride [, $decimal_places] );
$DimensionlessSpeed = Math::NumberCruncher::DimensionlessSpeed_2( $ActualSpeed, $leg_length [, $decimal_places]);
$ActualSpeed = Math::NumberCruncher::ActualSpeed( $leg_length, $DimensionlessSpeed [, $decimal_places] );
$eccentricity = Math::NumberCruncher::Eccentricity( $half_major_axis, $half_minor_axis [, $decimal_places] );
$LatusRectum = Math::NumberCruncher::LatusRectum( $half_major_axis, $half_minor_axis [, $decimal_places] );
$EllipseArea = Math::NumberCruncher::EllipseArea( $half_major_axis, $half_minor_axis [, $decimal_places] );
$OrbitalVelocity = Math::NumberCruncher::OrbitalVelocity( $r, $a, $M [, $decimal_places] );
$sine = Math::NumberCruncher::sin( $x [, $decimal_places] );
$cosine = Math::NumberCruncher::cos( $x [, $decimal_places] );
$tangent = Math::NumberCruncher::tan( $x [, $decimal_places] );
$arcsin = Math::NumberCruncher::asin( $x [, $decimal_places] );
$arccos = Math::NumberCruncher::acos( $x [, $decimal_places] );
$arctan = Math::NumberCruncher::atan( $x [, $decimal_places] );
$cotangent = Math::NumberCruncher::cot( $x [, $decimal_places] );
$arccot = Math::NumberCruncher::acot( $x [, $decimal_places] );
$secant = Math::NumberCruncher::sec( $x [, $decimal_places] );
$arcsec = Math::NumberCruncher::asec( $x [, $decimal_places] );
$cosecant = Math::NumberCruncher::csc( $x [, $decimal_places] );
$arccosecant = Math::NumberCruncher::acsc( $x [, $decimal_places] );
$exsecant = Math::NumberCruncher::exsec( $x [, $decimal_places] );
$versine = Math::NumberCruncher::vers( $x [, $decimal_places] );
$coversine = Math::NumberCruncher::covers( $x [, $decimal_places] );
$haversine = Math::NumberCruncher::hav( $x [, $decimal_places] );
$grouped = Math::NumberCruncher::Commas( $number );
$SqrRoot = Math::NumberCruncher::SqrRoot( $number [, $decimal_places] );
$square_root = Math::NumberCruncher::sqrt( $x [, $decimal_places] );
$root = Math::NumberCruncher::Root( 55, 3 [, $decimal_places] );
$root = Math::NumberCruncher::Root2( 55, 3 [, $decimal_places] );
$log = Math::NumberCruncher::Ln( 100 [, $decimal_places] );
$log = Math::NumberCruncher::log( $num [, $decimal_places] );
$num = Math::NumberCruncher::Exp( 0.111 [, $decimal_places] );
$num = Math::NumberCruncher::exp( $log [, $decimal_places] );
$Pi = Math::NumberCruncher::PICONST( $decimal_places );
$E = Math::NumberCruncher::ECONST( $decimal_places );
( $A, $B, $C ) = Math::NumberCruncher::PythagTriples( $x, $y [, $decimal_places] );
$z = Math::NumberCruncher::PythagTriplesSeq( $x, $y [, $decimal_places] );
@nums = Math::NumberCruncher::SIS( [$start, $numbers, $increment] );
$inverse = Math::NumberCruncher::Inverse( $number [, $decimal_places] );
@constants = Math::NumberCruncher::CONSTANTS( all [, $decimal_places] );
$bernoulli = Math::NumberCruncher::Bernoulli( $num [, $decimal_places] );
@bernoulli = Math::NumberCruncher::Bernoulli( $num );

iCal::Parser is a Perl module to parse iCalendar files into a data structure.

SYNOPSIS

use iCal::Parser

my $parser=iCal::Parser->new();
my $hash=$parser->parse($file);

$parser->parse($another_file);
my $combined=$parser->calendar;

my $combined=iCal::Parser->new->parse(@files);
my $combined=iCal::Parser->new->parse_files(@files);
my $combined=iCal::Parser->new->parse_strings(@strings);

This module processes iCalendar (vCalendar 2.0) files as specified in RFC 2445 into a data structure. It handles recurrences (RRULEs), exclusions (EXDATEs), event updates (events with a RECURRENCE-ID), and nested data structures (ATTENDEES and VALARMs). It currently ignores the VTIMEZONE, VJOURNAL and VFREEBUSY entry types.

The data structure returned is a hash like the following:

{
calendars=>[%cal, ...],
events=>{yyyy=>{mm=>{dd}=>{UID=>%event}}
todos=>[%todo, ...]
}

That is, it contains an array of calendar hashes, a hash of events key by year=>month=>day=>eventUID, and an array of todos.

Calendars, events and todos are "rolled up" version os the hashes returned from Text::vFile::asData, with dates replaced by DateTime objects.

During parsing, events in the input calendar are expanded out into multiple events, one per day covered by the event, as follows:
If the event is a one day "all day" event (in ical, the event is 24hrs long, starts at midnight on the day and ends a midnight of the next day), it contains no hour field and the allday field is set to 1.

If the event is a recurrence (RRULE), one event per day is created as per the RRULE specification.

If the event spans more than one day (the start and end dates are on different days, but does not contain an RRULE), it is expanded into multiple events, the first events end time is set to midnight, subsequent events are set to start at midnight and end at midnight the following day (same as an "allday" event, but the allday field is not set), and the last days event is set to run from midnight to the end time of the original multi-day event.

If the event is an update (it contains a RECURRENCE-ID), the original event is updated. If the referenced event does not exist (e.g., it was deleted after the update), then the event is added as a new event.
An example of each hash is below.