release_notes/linuxsampler_2_1_0/01_linuxsampler_2_1_0.html

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    <meta name="author" content="Christian Schoenebeck">
    <title>Release Notes LinuxSampler 2.1.0</title>
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    <h1>LinuxSampler 2.1.0</h1>
    <p>
      LinuxSampler 2.1.0 and friends were released on November 25th 2017.
      Two years have passed since the last release of LinuxSampler.
      Here is a summary about what's new.
    </p>

    <h3>Real-Time Instrument Scripts</h3>
    <p>
      In the <a href="01_linuxsampler_2_0_0.html">previous release</a> a major
      new feature called <i>Real-Time Instrument Scripts</i> was added, which
      are essentially small programs that may be bundled with sound files to extend the
      sampler with custom behavior specifically intended for individual sounds.
      <a href="instrument_scripts.html">Find out more ...</a>
    </p>
    <p>
      These programs are written by sound designers in a script language called
      <a href="01_nksp.html">NKSP</a>.
      In this release a large amount of extensions and improvements have been
      added for this real-time instrument scripting support of LinuxSampler.
      For example 48 new built-in NKSP functions and 21 new built-in NKSP
      variables have been added.
      <a href="01_nksp_reference.html">Find out more ...</a>
    </p>
    <p>
      Also the NKSP language and the underlying engine itself was extended.
      Most notably the script engine now has an execution scheduler which is
      the basis for many of the timing relevant new NKSP features in this
      release, like programmatically suspending and resuming scripts for an
      exact duration or at an exact point of time or triggering or killing notes
      at very precise times (all with microsecond accuracy).
      You can now even launch new threads in your NKSP scripts by
      calling the new built-in function <code lang="nksp">fork()</code>.
      Furthermore
      <a href="01_nksp.html#boolean_operators">bitwise operators</a>
      have been added to NKSP, as well as support for
      read only built-in variables,
      <a href="01_nksp.html#synchronized_blocks">"synchronized" code blocks</a>
      , as well as
      <a href="01_nksp.html#user_functions">user declared functions</a>
      and user declared const array variables have been added to the NKSP language,
      and finally automatic suspension of RT threatening scripts by the RT script engine
      has been implemented. The latter ensures that the sampler remains stable,
      and does not cause audio dropouts, even while you are working on heavy and
      extremely buggy scripts.
      Also syntax error messages with NKSP scripts have
      been improved to output more clear and user friendly error messages, as
      well as the NKSP editor API has been improved which brings handy new features
      to gigedit's NKSP script editor, which will further be described below,
      along with gigedit's new features.
    </p>

    <h3>SFZ Engine</h3>
    <p>
      The SFZ engine now supports <code lang="sfz">&lt;global&gt;</code>,
      <code lang="sfz">&lt;master&gt;</code> sections,
      <code lang="sfz">#define</code> statement and <code lang="sfz">set_ccN</code>
      opcode. And finally the SFZ engine now supports NKSP real-time
      instrument scripts as well by adding a new
      <code lang="sfz">script</code> opcode for this purpose. So NKSP scripts
      are no longer limited to our Giga engine.
    </p>

    <h3>New GigaStudio format features</h3>
    <p>
      The equally named software on Windows has gone years ago,
      but the format lives on with LinuxSampler and this release adds
      yet some more new extensions to the gig format. Most notably you
      now have options to control envelope generators' state machines.
      For example you can now define whether a certain EG state should
      either be aborted or continued to its end when a note off arrived.
      These controls are especially useful for certain kinds of sounds
      like percussive instruments.
    <p>
    <img src="gigedit_state_machine_options.png" caption="EG State Machine Options (Gigedit)">
    </p>
      Accordingly you will now find new check boxes for this in gigedit.
      As these are extensions of the original format, setting these options
      will only work with LinuxSampler and would be ignored with the
      original GigaStudio software.
    </p>

    <h3>Instruments DB</h3>
    <p>
      Also the Instruments Database feature has received important maintenance
      fixes. Before this release, the instrument DB feature was barely usable
      for quite some time. Fundamental instruments DB issues have been fixed in
      this release to finally consider this feature stable again as well.
    </p>


    <h2>Gigedit 1.1.0</h2>
    <p>
      Also <i>Gigedit</i>, our instrument editor for the GigaStudio/Gigasampler
      format, had been enhanced quite a lot. The most important new features are
      summarized next.
    </p>

    <h3>Script Editor</h3>
    <p>
      Gigedit's integrated instrument script editor supports now tight coupling
      directly with LinuxSampler's actual real-time instrument script backend.
      That provides several improvements for the script editor.
    </p>
    <p>
      <img src="nksp_editor_error_tooltip.png" caption="NKSP Error Tooltips">
      For example
      colored syntax highlighting of scripts is now always displayed correctly and
      simply looks much better now. Previously there was some small hard coded
      script parser code on Gigedit's side which however was buggy and simply
      did no great job. Now all the heavy lifting of handling all the details
      of the numerous NKSP language aspects are handled by the sampler instead,
      which also provides the following new script editor features.
    </p>
    <p>
      Due to that direct coupling with LinuxSampler's
      script backend, gigedit's script editor now shows all issues related to the script (errors
      and warnings) directly within the script editor in real-time while you are
      typing. The actual erroneous locations of the script are automatically
      highlighted with red background color, locations of the script with
      warnings are automatically highlighted with yellow background color, and
      when you move your mouse over the respective code location, the precise
      error/warning message is displayed as a tooltip. And last but not least
      there is a summary of issues displayed in the status bar of the script
      editor. Since LinuxSampler's instrument script backend is actually doing
      all the work for the script editor, all aspects of the language, all
      details about built-in functions and variables, and all potential issues
      with their precise cause and messages are automatically covered by the
      script editor now.
      That way you immediately know whether or whether not your script
      is OK with every character you are typing, and without requiring to
      actually load the script with an instrument into the sampler.
    </p>
    <p>
      <img src="nksp_editor_strike_through.png" caption="NKSP Disabled Code Blocks">
      Additionally when clicking on the
      script editor's "Apply" button or using Ctrl+S keyboard shortcut, then
      the script is automatically reloaded by the sampler. So you no longer
      have to reload the respective instrument manually while you are
      developing instrument scripts. There are also visual enhancements for the
      script editor, for example the line numbers are now shown on the left,
      the font size can be altered by the user, and unused code portions (i.e.
      disabled by <a href="">NKSP preprocessor statements</a>)
      are automatically striked through. That way you can immediately see
      which code portions of your scripts are actually used, and which are not.<br>
      <br>
      As as side note, you may have noticed a handy new built-in preprocessor
      condition in LinuxSampler 2.1.0 which can be enabled with
      <code lang="nksp">SET_CONDITION(NKSP_NO_MESSAGE)</code> and allows you
      to quickly disable <code lang="nksp">message()</code> function calls,
      i.e. to conviently switch your scripts between a debug and release mode.
      <a href="01_nksp.html#disable_messages">Find out more ...</a>
    </p>

    <h3>Macros</h3>
    <p>
      Another major new feature in this release are macros.
      A macro is a set of changes that should be applied to currently selected instrument.
    </p>
    <p>
      <img src="gigedit_macros_setup.png" caption="Macro List (Gigedit)">
      Such macros can be reviewed and edited, and they can be saved permanently for
      example as templates for common instrument creation tasks. Macros can be
      assigned to F keys on the keyboard so that they can be quickly triggered,
      you can transfer them over the OS clipboard and you can write comments
      to your macros so that you never forget what kind of purpose you had in
      mind for them. The macro features are based on libgig's new
      "Serialization" framework (described below) and accordingly you need at
      least libgig 4.1.0 for using these macro features.
    </p>
    <p>
      <img src="gigedit_macro_editor.png" caption="Macro Editor (Gigedit)">
      This is an example of editing a macro. Usually you may start creating a
      new macro by simply taking all parameters of a selected dimension region.
      Then in the macro editor you usually multi-row select (i.e. by Ctrl clicking
      items in the list) just the parameters you want this macro to alter, then
      click on "Inverse Delete" to just keep those few selected parameters in
      that macro. As a result, when you are going to apply this macro during your
      upcoming work, only those few parameters are modifed by this macro and all
      other ones are left untouched.
      Of course you can also alter the individual parameter values in
      this editor as well. 
    </p>

    <h3>Persistent Settings</h3>
    <p>
      All user settings of gigedit are now persistently saved and automatically
      restored. This also includes gigedit's windows' dimensions and positions.
    </p>

    <h3>Multi-Row Selection</h3>
    <p>
    <img src="gigedit_multi_row_action.png" caption="Multi Row Selection &amp; Actions (Gigedit)">
      Multi-row selection has been added to all list views now, so you can now
      more efficiently apply actions to multiple samples, instruments or scripts
      simultaneously at once, instead of requesting those actions for each item
      individually.
    </p>

    <h3>Multi-Zone Selection</h3>
    <p>
      <img src="gigedit_multi_dimreg_zone_actions.png" caption="Multi Zone Selection &amp; Actions (Gigedit)">
      Also modifying key features of several dimension region zones
      simultaneously is now supported. That means you can now delete, split and
      resize multiple dimension region zones at once. Oh yes, I forget, Ctrl+click
      selecting multiple dimension regions is supported now as well.
    </p>
    
    <h3>Feature Icons</h3>
    <p>
      <img src="gigedit_zone_icons.png" caption="Feature Icons (Gigedit)">
      You will also note that there are now icons displayed on the individual
      regions and dimension region zones. Those icons visualize common key
      features of regions and dimension region zones. For example if you forgot
      to assign any sample to one of them, then you will see a red dot on the
      respective region or dimension region zone. Another icon type is showing
      you whether a region or dimension region zone uses a sample loop.
      For example when you just imported a drum sample, you don't really want
      a loop to be on.
      This way
      you can immediately see and control the key features of all regions
      and their dimension region zones, without requiring to browse through all
      of them individually.
    </p>

    <h3>Keyboard Shortcuts</h3>
    <p>
     Various new keyboard shortcuts have been added so you can work more
     efficiently on your sounds. For example you can now use Ctrl+Left and
     Ctrl+Right to navigate through all regions of the currently selected
     instrument, and likewise you can use Alt+Left, Alt+Right, Alt+Up and
     Alt+Down to navigate through all dimension region zones of the currently
     selected region. Since there are many actions that can be either applied
     on instrument level, or on region level, or on dimension region level, as
     a general rule, for all keyboard shortcuts:
     <ul>
       <li><b>Shift</b> key is used for actions on instrument level</li>
       <li><b>Ctrl</b> key is used on region level</li>
       <li><b>Alt</b> key is used by gigedit for actions on dimension region level</li>
     </ul>
     So as another example you may copy all parameters of the currently
     selected dimension region zone by hitting Alt+C, then you might select
     another dimension region zone, or another instrument and then use Alt+V
     to apply the parameters from the clipboard. While the parameters are
     (as macro actually) on the clipboard you can also review, edit and
     delete the individual parameters before applying them. As a final
     example for new important shortcuts you may now use Shift+Up and
     Shift+Down for switching between instruments.
    </p>

    <h3>Combine Tool Improvements</h3>
    <p>
      <img src="gigedit_combine_tool_reorder.png" caption="Combine Tool (Gigedit)">
      Also the Combine Tool has been improved. You can now simply select the
      (multiple) instruments you want to combine directly from the applications
      main window, i.e. by Ctrl or Shift clicking them from the instruments
      list view, and then right click to call the combine tool on that
      selection. The Combine Tool now also shows you as preview the order in
      which the selected instruments are going to be combined. This is
      especially useful when combining instruments with certain dimension
      types where the order matters for the actual resulting sound; for example
      when using the velocity dimension. Simply use drag n drop to reorder
      the previously selected instruments before combining them.
    </p>

    <h3>Search Filter</h3>
    <p>
      <img src="gigedit_search_filter.png" caption="Search Filter (Gigedit)">
      And last but not least a filter option field had been added to the
      instruments list and samples list, which allows you to find specific
      samples and instruments very quickly by typing search key words, which is
      especially very helpful in case you are working on gig files which contain
      a very large amount of samples or instruments in a single gig file
      (like this one, which apparently has far more than 400 instruments).
    </p>

    <h2>libgig 4.1.0</h2>
    <p>
      Our fundamental file access C++ library
      <a href="http://download.linuxsampler.org/doc/libgig/api/">libgig</a>
      has also received some major improvements, which are outlined next.
    </p>

    <h3>Files larger than 2 GB</h3>
    <p>
      libgig 4.1.0 adds support for files much larger than 2 GB for GigaStudio /
      Gigasampler (.gig), DLS, as well as for RIFF files in general. This file size
      limitation existed for a very long time due to the RIFF format's historical,
      internal 32 bit file offsets. To circumvent this file size limitation the
      concept of so called "extension files" was added in the past to the
      GigaStudio format, which means that the GigaStudio instrument editor
      (the original one on Windows) splitted
      the respective overall instrument file into a set of files (.gig, .gx01,
      .gx02, ...), each being max. 2 GB in size, and all of them were expected to be
      located in the same directory for the sampler to load the entire large
      instrument successfully. libgig always supported only reading such gig
      extension files, however libgig never supported to create .gig files with
      extension files, nor did it support modifying existing ones.
    <p>
    </p>
      In this release
      it was necessary to finally get rid of this overall file size limitation in
      libgig. Now when that concept of extension files was introduced years ago, it
      made sense at that point, because there were still many systems out there
      which still had no support for large files (on either OS or file system
      level). However today even on low end mobile devices support for large files
      is already a broad standard. Accordingly instead of adding write support for
      extension files in libgig, the problem was addressed at its root by
      transparently using appropriate, automatic file offset sizes. So when writing
      .gig/DLS/RIFF files smaller than 2 GB there are still 32 bit file offsets
      being used by libgig. Accordingly such files are still backward compatible
      with older software. However if the overall file size to be written is 2 GB or
      larger, then 64 bit file offsets are automatically used by libgig instead.
      Note though that due to that circumstance such files &#8807; 2 GB are not backward
      compatible with older versions of libgig, nor could they be loaded with the
      original GigaStudio software.
    </p>
    
    <h3>Serialization API</h3>
    <p>
      Another major new feature in this libgig release is the entirely new
      <a href="http://download.linuxsampler.org/doc/libgig/api/namespaceSerialization.html">Serialization API</a>
      which provides a powerful and easy way
      to serialize and deserialize an arbitrary set of native C++ objects into an
      abstract data stream. Which means you can simply save the entire runtime state
      of an application to a file or send it as data over "wire" (i.e. over network
      or to another process) and restore that runtime state from that data there at
      any time. In contrast to other C++ serialization frameworks out there, this
      framework provides two major benefits:
      <ol>
        <li>
          This serialization framework is designed to be very robust regarding
          potential versioning changes of the native C++ classes being
          (de)serialized. So even if the C++ classes have seen massive software
          changes between the point where they were serialized and the point where
          they are to be deserialized; for example if class member variables of
          serialized C++ objects were renamed in meantime, or if variable offsets, or
          variables' data types had been changed, then the deserialization algorithm
          can still cope with such common software changes automatically in many
          cases, that is as long as the deserialization algorithm can "guess" what
          the changes were exactly. If the serialization framework is unable to
          automatically detect the precise software changes, then it will abort the
          deserialization task with an exception and an error message stating that
          the software versions are incompatible.
        </li>
        <li>
          This serialization framework supports "partial" deserialization. That
          means it not only allows to restore an entire runtime state, but it also
          allows to only restore an arbitrary desired subset of information
          from the previously serialized data stream, while leaving all other data
          of the running C++ objects untouched. The serialization framework also
          incorporates a reflection API which allows applications to implement
          convenient editors on top of such serialized data, i.e. allowing end users
          to pick or alter specific information within the serialized data.
        </li>
      </ol>
      This new Serialization framework is already embedded into the gig classes of
      libgig, and it is used as basis for the new powerful macro features in the
      gigedit instrument editor, like already outlined above.
    </p>

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1	schoenebeck	3376	<html>
2			<head>
3			<meta name="author" content="Christian Schoenebeck">
4			<title>Release Notes LinuxSampler 2.1.0</title>
5			<navpath>LinuxSampler 2.1.0</navpath>
6			<meta name="description" content="Release notes for LinuxSampler 2.1.0.">
7			<link rel="stylesheet" href="http://doc.linuxsampler.org/css/preview.css">
8			<script type="text/javascript" src="http://doc.linuxsampler.org/js/preview.js"></script>
9			</head>
10			<body>
11			<h1>LinuxSampler 2.1.0</h1>
12			<p>
13			LinuxSampler 2.1.0 and friends were released on November 25th 2017.
14			Two years have passed since the last release of LinuxSampler.
15			Here is a summary about what's new.
16			</p>
17
18			<h3>Real-Time Instrument Scripts</h3>
19			<p>
20			In the <a href="01_linuxsampler_2_0_0.html">previous release</a> a major
21			new feature called <i>Real-Time Instrument Scripts</i> was added, which
22			are essentially small programs that may be bundled with sound files to extend the
23			sampler with custom behavior specifically intended for individual sounds.
24			<a href="instrument_scripts.html">Find out more ...</a>
25			</p>
26			<p>
27			These programs are written by sound designers in a script language called
28			<a href="01_nksp.html">NKSP</a>.
29			In this release a large amount of extensions and improvements have been
30			added for this real-time instrument scripting support of LinuxSampler.
31			For example 48 new built-in NKSP functions and 21 new built-in NKSP
32			variables have been added.
33			<a href="01_nksp_reference.html">Find out more ...</a>
34			</p>
35			<p>
36			Also the NKSP language and the underlying engine itself was extended.
37			Most notably the script engine now has an execution scheduler which is
38			the basis for many of the timing relevant new NKSP features in this
39			release, like programmatically suspending and resuming scripts for an
40			exact duration or at an exact point of time or triggering or killing notes
41			at very precise times (all with microsecond accuracy).
42			You can now even launch new threads in your NKSP scripts by
43			calling the new built-in function <code lang="nksp">fork()</code>.
44			Furthermore
45			<a href="01_nksp.html#boolean_operators">bitwise operators</a>
46			have been added to NKSP, as well as support for
47			read only built-in variables,
48			<a href="01_nksp.html#synchronized_blocks">"synchronized" code blocks</a>
49			, as well as
50			<a href="01_nksp.html#user_functions">user declared functions</a>
51			and user declared const array variables have been added to the NKSP language,
52			and finally automatic suspension of RT threatening scripts by the RT script engine
53			has been implemented. The latter ensures that the sampler remains stable,
54			and does not cause audio dropouts, even while you are working on heavy and
55			extremely buggy scripts.
56			Also syntax error messages with NKSP scripts have
57			been improved to output more clear and user friendly error messages, as
58			well as the NKSP editor API has been improved which brings handy new features
59			to gigedit's NKSP script editor, which will further be described below,
60			along with gigedit's new features.
61			</p>
62
63			<h3>SFZ Engine</h3>
64			<p>
65			The SFZ engine now supports <code lang="sfz"><global></code>,
66			<code lang="sfz"><master></code> sections,
67			<code lang="sfz">#define</code> statement and <code lang="sfz">set_ccN</code>
68			opcode. And finally the SFZ engine now supports NKSP real-time
69			instrument scripts as well by adding a new
70			<code lang="sfz">script</code> opcode for this purpose. So NKSP scripts
71			are no longer limited to our Giga engine.
72			</p>
73
74			<h3>New GigaStudio format features</h3>
75			<p>
76			The equally named software on Windows has gone years ago,
77			but the format lives on with LinuxSampler and this release adds
78			yet some more new extensions to the gig format. Most notably you
79			now have options to control envelope generators' state machines.
80			For example you can now define whether a certain EG state should
81			either be aborted or continued to its end when a note off arrived.
82			These controls are especially useful for certain kinds of sounds
83			like percussive instruments.
84			<p>
85			<img src="gigedit_state_machine_options.png" caption="EG State Machine Options (Gigedit)">
86			</p>
87			Accordingly you will now find new check boxes for this in gigedit.
88			As these are extensions of the original format, setting these options
89			will only work with LinuxSampler and would be ignored with the
90			original GigaStudio software.
91			</p>
92
93			<h3>Instruments DB</h3>
94			<p>
95			Also the Instruments Database feature has received important maintenance
96			fixes. Before this release, the instrument DB feature was barely usable
97			for quite some time. Fundamental instruments DB issues have been fixed in
98			this release to finally consider this feature stable again as well.
99			</p>
100
101
102			<h2>Gigedit 1.1.0</h2>
103			<p>
104			Also <i>Gigedit</i>, our instrument editor for the GigaStudio/Gigasampler
105			format, had been enhanced quite a lot. The most important new features are
106			summarized next.
107			</p>
108
109			<h3>Script Editor</h3>
110			<p>
111			Gigedit's integrated instrument script editor supports now tight coupling
112			directly with LinuxSampler's actual real-time instrument script backend.
113			That provides several improvements for the script editor.
114			</p>
115			<p>
116			<img src="nksp_editor_error_tooltip.png" caption="NKSP Error Tooltips">
117			For example
118			colored syntax highlighting of scripts is now always displayed correctly and
119			simply looks much better now. Previously there was some small hard coded
120			script parser code on Gigedit's side which however was buggy and simply
121			did no great job. Now all the heavy lifting of handling all the details
122			of the numerous NKSP language aspects are handled by the sampler instead,
123			which also provides the following new script editor features.
124			</p>
125			<p>
126			Due to that direct coupling with LinuxSampler's
127			script backend, gigedit's script editor now shows all issues related to the script (errors
128			and warnings) directly within the script editor in real-time while you are
129			typing. The actual erroneous locations of the script are automatically
130			highlighted with red background color, locations of the script with
131			warnings are automatically highlighted with yellow background color, and
132			when you move your mouse over the respective code location, the precise
133			error/warning message is displayed as a tooltip. And last but not least
134			there is a summary of issues displayed in the status bar of the script
135			editor. Since LinuxSampler's instrument script backend is actually doing
136			all the work for the script editor, all aspects of the language, all
137			details about built-in functions and variables, and all potential issues
138			with their precise cause and messages are automatically covered by the
139			script editor now.
140			That way you immediately know whether or whether not your script
141			is OK with every character you are typing, and without requiring to
142			actually load the script with an instrument into the sampler.
143			</p>
144			<p>
145			<img src="nksp_editor_strike_through.png" caption="NKSP Disabled Code Blocks">
146			Additionally when clicking on the
147			script editor's "Apply" button or using Ctrl+S keyboard shortcut, then
148			the script is automatically reloaded by the sampler. So you no longer
149			have to reload the respective instrument manually while you are
150			developing instrument scripts. There are also visual enhancements for the
151			script editor, for example the line numbers are now shown on the left,
152			the font size can be altered by the user, and unused code portions (i.e.
153			disabled by <a href="">NKSP preprocessor statements</a>)
154			are automatically striked through. That way you can immediately see
155			which code portions of your scripts are actually used, and which are not.<br>
156			<br>
157			As as side note, you may have noticed a handy new built-in preprocessor
158			condition in LinuxSampler 2.1.0 which can be enabled with
159			<code lang="nksp">SET_CONDITION(NKSP_NO_MESSAGE)</code> and allows you
160			to quickly disable <code lang="nksp">message()</code> function calls,
161			i.e. to conviently switch your scripts between a debug and release mode.
162			<a href="01_nksp.html#disable_messages">Find out more ...</a>
163			</p>
164
165			<h3>Macros</h3>
166			<p>
167			Another major new feature in this release are macros.
168			A macro is a set of changes that should be applied to currently selected instrument.
169			</p>
170			<p>
171			<img src="gigedit_macros_setup.png" caption="Macro List (Gigedit)">
172			Such macros can be reviewed and edited, and they can be saved permanently for
173			example as templates for common instrument creation tasks. Macros can be
174			assigned to F keys on the keyboard so that they can be quickly triggered,
175			you can transfer them over the OS clipboard and you can write comments
176			to your macros so that you never forget what kind of purpose you had in
177			mind for them. The macro features are based on libgig's new
178			"Serialization" framework (described below) and accordingly you need at
179			least libgig 4.1.0 for using these macro features.
180			</p>
181			<p>
182			<img src="gigedit_macro_editor.png" caption="Macro Editor (Gigedit)">
183			This is an example of editing a macro. Usually you may start creating a
184			new macro by simply taking all parameters of a selected dimension region.
185			Then in the macro editor you usually multi-row select (i.e. by Ctrl clicking
186			items in the list) just the parameters you want this macro to alter, then
187			click on "Inverse Delete" to just keep those few selected parameters in
188			that macro. As a result, when you are going to apply this macro during your
189			upcoming work, only those few parameters are modifed by this macro and all
190			other ones are left untouched.
191			Of course you can also alter the individual parameter values in
192			this editor as well.
193			</p>
194
195			<h3>Persistent Settings</h3>
196			<p>
197			All user settings of gigedit are now persistently saved and automatically
198			restored. This also includes gigedit's windows' dimensions and positions.
199			</p>
200
201			<h3>Multi-Row Selection</h3>
202			<p>
203			<img src="gigedit_multi_row_action.png" caption="Multi Row Selection & Actions (Gigedit)">
204			Multi-row selection has been added to all list views now, so you can now
205			more efficiently apply actions to multiple samples, instruments or scripts
206			simultaneously at once, instead of requesting those actions for each item
207			individually.
208			</p>
209
210			<h3>Multi-Zone Selection</h3>
211			<p>
212			<img src="gigedit_multi_dimreg_zone_actions.png" caption="Multi Zone Selection & Actions (Gigedit)">
213			Also modifying key features of several dimension region zones
214			simultaneously is now supported. That means you can now delete, split and
215			resize multiple dimension region zones at once. Oh yes, I forget, Ctrl+click
216			selecting multiple dimension regions is supported now as well.
217			</p>
218
219			<h3>Feature Icons</h3>
220			<p>
221			<img src="gigedit_zone_icons.png" caption="Feature Icons (Gigedit)">
222			You will also note that there are now icons displayed on the individual
223			regions and dimension region zones. Those icons visualize common key
224			features of regions and dimension region zones. For example if you forgot
225			to assign any sample to one of them, then you will see a red dot on the
226			respective region or dimension region zone. Another icon type is showing
227			you whether a region or dimension region zone uses a sample loop.
228			For example when you just imported a drum sample, you don't really want
229			a loop to be on.
230			This way
231			you can immediately see and control the key features of all regions
232			and their dimension region zones, without requiring to browse through all
233			of them individually.
234			</p>
235
236			<h3>Keyboard Shortcuts</h3>
237			<p>
238			Various new keyboard shortcuts have been added so you can work more
239			efficiently on your sounds. For example you can now use Ctrl+Left and
240			Ctrl+Right to navigate through all regions of the currently selected
241			instrument, and likewise you can use Alt+Left, Alt+Right, Alt+Up and
242			Alt+Down to navigate through all dimension region zones of the currently
243			selected region. Since there are many actions that can be either applied
244			on instrument level, or on region level, or on dimension region level, as
245			a general rule, for all keyboard shortcuts:
246			<ul>
247			<li><b>Shift</b> key is used for actions on instrument level</li>
248			<li><b>Ctrl</b> key is used on region level</li>
249			<li><b>Alt</b> key is used by gigedit for actions on dimension region level</li>
250			</ul>
251			So as another example you may copy all parameters of the currently
252			selected dimension region zone by hitting Alt+C, then you might select
253			another dimension region zone, or another instrument and then use Alt+V
254			to apply the parameters from the clipboard. While the parameters are
255			(as macro actually) on the clipboard you can also review, edit and
256			delete the individual parameters before applying them. As a final
257			example for new important shortcuts you may now use Shift+Up and
258			Shift+Down for switching between instruments.
259			</p>
260
261			<h3>Combine Tool Improvements</h3>
262			<p>
263			<img src="gigedit_combine_tool_reorder.png" caption="Combine Tool (Gigedit)">
264			Also the Combine Tool has been improved. You can now simply select the
265			(multiple) instruments you want to combine directly from the applications
266			main window, i.e. by Ctrl or Shift clicking them from the instruments
267			list view, and then right click to call the combine tool on that
268			selection. The Combine Tool now also shows you as preview the order in
269			which the selected instruments are going to be combined. This is
270			especially useful when combining instruments with certain dimension
271			types where the order matters for the actual resulting sound; for example
272			when using the velocity dimension. Simply use drag n drop to reorder
273			the previously selected instruments before combining them.
274			</p>
275
276			<h3>Search Filter</h3>
277			<p>
278			<img src="gigedit_search_filter.png" caption="Search Filter (Gigedit)">
279			And last but not least a filter option field had been added to the
280			instruments list and samples list, which allows you to find specific
281			samples and instruments very quickly by typing search key words, which is
282			especially very helpful in case you are working on gig files which contain
283			a very large amount of samples or instruments in a single gig file
284			(like this one, which apparently has far more than 400 instruments).
285			</p>
286
287			<h2>libgig 4.1.0</h2>
288			<p>
289			Our fundamental file access C++ library
290			<a href="http://download.linuxsampler.org/doc/libgig/api/">libgig</a>
291			has also received some major improvements, which are outlined next.
292			</p>
293
294			<h3>Files larger than 2 GB</h3>
295			<p>
296			libgig 4.1.0 adds support for files much larger than 2 GB for GigaStudio /
297			Gigasampler (.gig), DLS, as well as for RIFF files in general. This file size
298			limitation existed for a very long time due to the RIFF format's historical,
299			internal 32 bit file offsets. To circumvent this file size limitation the
300			concept of so called "extension files" was added in the past to the
301			GigaStudio format, which means that the GigaStudio instrument editor
302			(the original one on Windows) splitted
303			the respective overall instrument file into a set of files (.gig, .gx01,
304			.gx02, ...), each being max. 2 GB in size, and all of them were expected to be
305			located in the same directory for the sampler to load the entire large
306			instrument successfully. libgig always supported only reading such gig
307			extension files, however libgig never supported to create .gig files with
308			extension files, nor did it support modifying existing ones.
309			<p>
310			</p>
311			In this release
312			it was necessary to finally get rid of this overall file size limitation in
313			libgig. Now when that concept of extension files was introduced years ago, it
314			made sense at that point, because there were still many systems out there
315			which still had no support for large files (on either OS or file system
316			level). However today even on low end mobile devices support for large files
317			is already a broad standard. Accordingly instead of adding write support for
318			extension files in libgig, the problem was addressed at its root by
319			transparently using appropriate, automatic file offset sizes. So when writing
320			.gig/DLS/RIFF files smaller than 2 GB there are still 32 bit file offsets
321			being used by libgig. Accordingly such files are still backward compatible
322			with older software. However if the overall file size to be written is 2 GB or
323			larger, then 64 bit file offsets are automatically used by libgig instead.
324			Note though that due to that circumstance such files ≧ 2 GB are not backward
325			compatible with older versions of libgig, nor could they be loaded with the
326			original GigaStudio software.
327			</p>
328
329			<h3>Serialization API</h3>
330			<p>
331			Another major new feature in this libgig release is the entirely new
332			<a href="http://download.linuxsampler.org/doc/libgig/api/namespaceSerialization.html">Serialization API</a>
333			which provides a powerful and easy way
334			to serialize and deserialize an arbitrary set of native C++ objects into an
335			abstract data stream. Which means you can simply save the entire runtime state
336			of an application to a file or send it as data over "wire" (i.e. over network
337			or to another process) and restore that runtime state from that data there at
338			any time. In contrast to other C++ serialization frameworks out there, this
339			framework provides two major benefits:
340			<ol>
341			<li>
342			This serialization framework is designed to be very robust regarding
343			potential versioning changes of the native C++ classes being
344			(de)serialized. So even if the C++ classes have seen massive software
345			changes between the point where they were serialized and the point where
346			they are to be deserialized; for example if class member variables of
347			serialized C++ objects were renamed in meantime, or if variable offsets, or
348			variables' data types had been changed, then the deserialization algorithm
349			can still cope with such common software changes automatically in many
350			cases, that is as long as the deserialization algorithm can "guess" what
351			the changes were exactly. If the serialization framework is unable to
352			automatically detect the precise software changes, then it will abort the
353			deserialization task with an exception and an error message stating that
354			the software versions are incompatible.
355			</li>
356			<li>
357			This serialization framework supports "partial" deserialization. That
358			means it not only allows to restore an entire runtime state, but it also
359			allows to only restore an arbitrary desired subset of information
360			from the previously serialized data stream, while leaving all other data
361			of the running C++ objects untouched. The serialization framework also
362			incorporates a reflection API which allows applications to implement
363			convenient editors on top of such serialized data, i.e. allowing end users
364			to pick or alter specific information within the serialized data.
365			</li>
366			</ol>
367			This new Serialization framework is already embedded into the gig classes of
368			libgig, and it is used as basis for the new powerful macro features in the
369			gigedit instrument editor, like already outlined above.
370			</p>
371
372			</body>
373			</html>