At the CommunityOne West keynote last June a demo of Crossbow was given using a tool called Virtual Wire. If you haven't seen the demo before, you can watch a 10 minute replay of it here:

Since that time a lot of folks have asked for access to the tool that was used in the demo. Browsing the Crossbow project page recently I noticed the Crossbow Virtual Wire Demo Tool has now been made available.

I'll warn you in advance that I view the tool as alpha quality as it doesn't have some basic functionalities like undo. However, as the names implies, it's perfect for demos (and learning a lot about zones and networking).

When you extract the tool you'll find a couple of screencasts, which I've also made available here. There's no audio, but they do give you the basic idea of the capabilities of the tool.

Demo 1: Creating and Connecting 2 Private Networks

This demo uses the Crossbow Virtual Wire Demo Tool to create 2 private networks. One network contains a web server (192.168.2) while the client is connecting from a separate network (193.168.3). A router is set up to forward packets between the 2 networks. This is a self-contained private network. The demo concludes by using a network load generator along with DTrace to show how easy it is to monitor and configure bandwidth to the server. The details on how to reproduce this demo have been documented here.

Demo 2: Creating a Private Network Connected to the Public Network

This demo uses the Crossbow Virtual Wire Demo Tool to create a private network containing a web server behind a firewall. The IP routing is configured to access the server from the global zone. The demo concludes by using a network load generator along with DTrace to show how easy it is to monitor and configure bandwidth to the server. The details on how to reproduce this demo have been documented here.

I've read that the best way to learn DTrace is to study existing D scripts. However, upon doing so I quickly find myself asking "where is that documented?" And it turns out, with tens of thousands of probes, as is often the case, it's not. So I'd love to hear what others with more DTrace experience do, but these are the steps I seem to have stumbled upon.

As an example, let's take the script /opt/DTT/Proc/rwbytype.d, which shows the bytes read and written by process by vnode type. Here's an example of the output:

bleonard@opensolaris:/opt/DTT/Proc$ rwbytype.d 
Tracing... Hit Ctrl-C to end.
^C
PID    CMD               VTYPE  DIR     BYTES
21124  gnome-terminal      chr    W         1
10523  gnome-power-mana   sock    W         4
10565  gnome-netstatus-   fifo    R         7
10547  gnome-netstatus-   fifo    W         8
4817   conky              fifo    R         9
10634  firefox-bin        fifo    R         9
10634  firefox-bin        fifo    W         9
15379  whoami             fifo    W         9
10547  gnome-netstatus-   fifo    R        20
10565  gnome-netstatus-   fifo    W        20
15377  dtrace              chr    W        31
10412  Xorg                chr    R        32
10469  gnome-settings-d   sock    R        32
10523  gnome-power-mana   sock    R        32
21124  gnome-terminal      chr    R        33
10472  metacity           sock    W        56
10472  metacity           sock    R       200
21124  gnome-terminal     sock    R       220
15379  conky               reg    R       529
15379  ksh93               reg    R       529
4817   conky              sock    R      2720
10412  Xorg               sock    W      3204
4817   conky               reg    R      6696
21124  gnome-terminal     sock    W      6852
4817   conky              sock    W     37952
10412  Xorg               sock    R     44864

And here's the D script that produces that output:

typedef struct vtype2str {
	string code;
};

translator struct vtype2str < int T > {
	/* the order has been picked for performance reasons */
	code =
	    T == 1 ? "reg"   :
	    T == 9 ? "sock"  :
	    T == 4 ? "chr"   :
	    T == 6 ? "fifo"  :
	    T == 8 ? "proc"  :
	    T == 2 ? "dir"   :
	    T == 3 ? "blk"   :
	    T == 5 ? "lnk"   :
	    T == 7 ? "door"  :
	    T == 10 ? "port" :
	    T == 11 ? "bad"  : "non";
};

dtrace:::BEGIN
{
	printf("Tracing... Hit Ctrl-C to end.\n");
}

fbt::fop_read:entry,
fbt::fop_write:entry
{
	self->type = xlate <struct vtype2str *>(args[0]->v_type)->code;
	self->size = args[1]->uio_resid;
	self->uiop = args[1];
}

fbt::fop_read:return
/self->uiop/
{
	this->resid = self->uiop->uio_resid;
	@bytes[pid, execname, self->type, "R"] = sum(self->size - this->resid);
	self->type = 0;
	self->size = 0;
	self->uiop = 0;
}

/* this is delibrately redundant code for performance reasons */
fbt::fop_write:return
/self->uiop/
{
	this->resid = self->uiop->uio_resid;
	@bytes[pid, execname, self->type, "W"] = sum(self->size - this->resid);
	self->type = 0;
	self->size = 0;
	self->uiop = 0;
}

dtrace:::END
{
	printf("%-6s %-16s %6s %4s %9s\n",
	    "PID", "CMD", "VTYPE", "DIR", "BYTES");
	printa("%-6d %-16s %6s %4s %@9d\n", @bytes);
}

First of all, this D script is only enabling 6 probes:

dtrace:::BEGIN
dtrace:::END
dtrace::fop_read:entry
dtrace::fob_read:return
dtrace::fob_write:entry
dtrace::fob_write:return

The BEGIN and END clauses are self-explanatory. Where I get tripped up is looking at the 2nd clause:

fbt::fop_read:entry,
fbt::fop_write:entry
{
	self->type = xlate <struct vtype2str *>(args[0]->v_type)->code;
	self->size = args[1]->uio_resid;
	self->uiop = args[1];
}

First, I see that we're setting 3 thread-local variables, type, size and uiop. All of these variables are set using probe arguments, and this is where things start to get confusing - where are these arguments defined? I can run the following dtrace command to get verbose information on a probe:

bleonard@opensolaris:/opt/DTT/Proc$ dtrace -lv -n fbt::fop_read:entry
   ID   PROVIDER            MODULE                          FUNCTION NAME
17725        fbt           genunix                          fop_read entry

	Probe Description Attributes
		Identifier Names: Private
		Data Semantics:   Private
		Dependency Class: Unknown

	Argument Attributes
		Identifier Names: Private
		Data Semantics:   Private
		Dependency Class: ISA

	Argument Types
		args[0]: vnode_t *
		args[1]: uio_t *
		args[2]: int
		args[3]: cred_t *
		args[4]: caller_context_t *

So I learn that the data semantics of the argument attributes are private, which means this probe is accessing private implementation details of the kernel, but that's the case with most DTrace kernel probes. Of more interest is the argument list:

args[0]: vnode_t *
args[1]: uio_t *
args[2]: int
args[3]: cred_t *
args[4]: caller_context_t 

So I can see there are 5 total arguments available for this probe and I know my clause is accessing args[0] and args[1]. But what now? What exactly is vnode_t and uio_t? As far as I know, there's no further dtrace command to drill down into these data types. At this point I turn to the OpenSolaris Source Browser.

I begin by searching on the probe function fop_read, which returns 2 results, the vnode.h header file and the vnode.c source file:

Searched refs:fop_read (Results 1 -2 of 2) sorted by null

/onnv/onnv-gate/usr/src/uts/common/sys/
vnode.h	[all...]
/onnv/onnv-gate/usr/src/uts/common/fs/
vnode.c	3177 fop_read( function     [all...]

The fop_read function is defined on line 3177 of vnode.c and I can click on that link to be taken directly to the source. Sure enough, the arguments to the fop_read function in vnode.c match what I was told by dtrace:

   3176 int
fop_read(
	vnode_t *vp,
	uio_t *uiop,
	int ioflag,
	cred_t *cr,
	caller_context_t *ct)

Now I can click on vnode_t to see its definition and this returns 3 results - the logical one being the vnode.h header file returned by our first search:

/onnv/onnv-gate/usr/src/uts/common/sys/ vnode.h 257 } vnode_t; typedef in typeref:struct:vnode 800 int (*vop_open)(vnode_t **, int, cred_t *, \ 802 int (*vop_close)(vnode_t *, int, int, offset_t, cred_t *, \ 804 int (*vop_read)(vnode_t *, uio_t *, int, cred_t *, \ 806 int (*vop_write)(vnode_t *, uio_t *, int, cred_t *, \ 808 int (*vop_ioctl)(vnode_t *, int, intptr_t, int, cred_t *, \ 810 int (*vop_setfl)(vnode_t *, int, int, cred_t *, \ 812 int (*vop_getattr)(vnode_t *, vattr_t *, int, cred_t *, \ 814 int (*vop_setattr)(vnode_t *, vattr_t *, int, cred_t *, \ 816 int (*vop_access)(vnode_t *, int, int, cred_t *,     [all...]

Here we see that vnode_t is defined on line 257, which you can click to navigate directly to that section of the source. Our D script above is referencing args[0]->v_type, and we can see v_type is an enum:

typedef struct vnode {
	kmutex_t	v_lock;		/* protects vnode fields */
	uint_t		v_flag;		/* vnode flags (see below) */
	uint_t		v_count;	/* reference count */
	void		*v_data;	/* private data for fs */
	struct vfs	*v_vfsp;	/* ptr to containing VFS */
	struct stdata	*v_stream;	/* associated stream */
	enum vtype	v_type;		/* vnode type */
	dev_t		v_rdev;		/* device (VCHR, VBLK) */

Which you can also click on to see the type definition:

/*
 * vnode types.  VNON means no type.  These values are unrelated to
 * values in on-disk inodes.
 */
typedef enum vtype {
	VNON	= 0,
	VREG	= 1,
	VDIR	= 2,
	VBLK	= 3,
	VCHR	= 4,
	VLNK	= 5,
	VFIFO	= 6,
	VDOOR	= 7,
	VPROC	= 8,
	VSOCK	= 9,
	VPORT	= 10,
	VBAD	= 11
} vtype_t;

Which matches up perfectly to the struct at the beginning of our D script. So, now I've got a better handle of exactly what's going on with this D script.

Now, as a test, see if you can follow the same procedure to find the documented comment in the OpenSolaris source code for arg[1]->uio_resid :-). 

Sun ISV engineer and DTrace evangelist Angelo Rajadurai has just authored a new quick start guide to DTrace. The guide is based on his "Observing Applications with DTrace" presentation (slides, video) at CommunityOne West and focuses on tracing web applications. The examples from the book have also been added to a wiki page for easier copy & paste.

A hidden little gem that comes included with your installation of OpenSolaris is the DTrace Toolkit. You'll find it installed at /opt/DTT.

The DTrace Toolkit is a collection of tools written by volunteers of the DTrace community, led by Brendan Gregg. What I find most impressive is how well it has been put together. There are 230 executable DTrace scripts, each with their own man page. The scripts are organized by type (CPU analysis, I/O analysis, etc.) so they are easy to study, but they've all been symlinked into a Bin directory, so they are easy to put on your path. I've added the following to my ~/.bashrc file:

#
# DTrace Toolkit
#
PATH=$PATH:/opt/DTT/Bin
MANPATH=$MANPATH:/opt/DTT/Man

In addition to their man pages, all of the scrips have a -h help option, for example:

bleonard@os200906:~$ execsnoop -h
USAGE: execsnoop [-a|-A|-ehjsvZ] [-c command]
       execsnoop                # default output
                -a              # print all data
                -A              # dump all data, space delimited
                -e              # safe output, parseable
                -j              # print project ID
                -s              # print start time, us
                -v              # print start time, string
                -Z              # print zonename
                -c command      # command name to snoop
  eg,
        execsnoop -v            # human readable timestamps
        execsnoop -Z		# print zonename
        execsnoop -c ls         # snoop ls commands only

Note, if you want to run the DTrace scripts from your user account, run the following command to add the needed privileges, substituting in your user name:

pfexec usermod -K defaultpriv=basic,dtrace_user,dtrace_proc,dtrace_kernel <user>

To get started learning all that's available, I recommend reading the DTrace Tookkit page. Also, Stefan Parvu has an excellent presentation on DTrace and the toolkit that's worth a look.

With this toolkit there's probably little need to write a DTrace script from scratch - it's literally a treasure chest of material that I've only begun to explore.

There are (at least) 2 big Linux conferences this weekend, the Ontario Linux Fest and the Florida Linux Show. The good news is that you'll find OpenSolaris represented at both of them. In Ontario Canada, Toronto OpenSolaris User Group leader Steven Acres will deliver Why OpenSolaris? In Orlando, Florida, I'll be delivering What's So Cool About OpenSoalaris Anyhow?

If you happen to be nearby (or willing to travel), please stop by and say hello.

When I edit a text file in vi, I find it much easier to read if the syntax is color highlighted. There are 2 steps to enabling this. First, add an alias for vi (or vim) to your ~/.bashrc file as follows:

#
# Enable color support for vi
#
alias vi='TERM=xtermc vim'

You can read the gory details about why this needs to be done in bug 1641 - xterm terminfo entry doesn't support color.

You also need to tell vi to use syntax coloring. Adding the following to your ~/.vimrc file (create one if it doesn't yet exist):

syntax on

Much nicer:

Netperf is a cool little utility that I discovered while working with Crossbow. It's technically a network benchmarking tool, but it's fun to use to hammer your network with load and test out Crossbow's bandwidth control features.

Simply click the link to install netperf , which will launch the Package Manager Web Installer:

To verify the installation, first start the benchmark server:

bleonard@opensolaris:~$ netserver
Starting netserver at port 12865
Starting netserver at hostname 0.0.0.0 port 12865 and family AF_UNSPEC

Then run netperf, which will run a TCP_STREAM test of 10 seconds over the loopback interface:

bleonard@opensolaris:~$ netperf
TCP STREAM TEST from ::ffff:0.0.0.0 (0.0.0.0) port 0 AF_INET to opensolaris (127.0.0.1) port 0 AF_INET
Recv   Send    Send                          
Socket Socket  Message  Elapsed              
Size   Size    Size     Time     Throughput  
bytes  bytes   bytes    secs.    10^6bits/sec  

 49152  49152  49152    10.00    4895.46  

Now that we know Netperf is set up correctly, we can use it to test bulk data transfer performance between 2 hosts (or 2 zones). TCP stream performance is the default test type and it's simply performed by running the command:

netperf -H <remotehost>

which will run a 10 second test between the local and remote system.

So I'm going to use netperf to run some tests between the global zone and a local zone, which has been set up to use a Crossbow virtual NIC exclusively. To create such a configuration on your own, see the blog entry Zones and Crossbow.

The local zone, myzone, is currently up and running:

bleonard@opensolaris:~$ zoneadm list -cv
  ID NAME             STATUS     PATH                           BRAND    IP    
   0 global           running    /                              native   shared
   - myzone           running    /zones/myzone                  ipkg     excl 

The first thing I'm going to do is copy the netserver program over to the local zone:

pfexec cp /opt/csw/bin/netserver /zones/myzone/root/var/tmp/.

And then start the netserver:

bleonard@opensolaris:~$ pfexec zlogin myzone /var/tmp/netserver
en_US.UTF-8: unknown locale
en_US.UTF-8: unknown locale
Starting netserver at port 12865
Starting netserver at hostname 0.0.0.0 port 12865 and family AF_UNSPEC

Now let's test the connection between the global and local zone:

bleonard@opensolaris:~$ netperf -H 10.0.1.25
TCP STREAM TEST from ::ffff:0.0.0.0 (0.0.0.0) port 0 AF_INET to ::ffff:10.0.1.25 (10.0.1.25) port 0 AF_INET
Recv   Send    Send                          
Socket Socket  Message  Elapsed              
Size   Size    Size     Time     Throughput  
bytes  bytes   bytes    secs.    10^6bits/sec  

 49152  49152  49152    10.00    1130.01   

Here we can see the throughput between my zones is 1130 Mbit/s. Now let's reduce the max bandwidth of the virtual NIC to 500 Mbit/s and try the test again:

bleonard@opensolaris:~$ pfexec dladm set-linkprop -p maxbw=500 myzone0
bleonard@opensolaris:~$ dladm show-vnic
LINK         OVER         SPEED  MACADDRESS           MACADDRTYPE         VID
myzone0      e1000g0      500    2:8:20:59:0:b5       random              0
bleonard@opensolaris:~$ netperf -H 10.0.1.25
TCP STREAM TEST from ::ffff:0.0.0.0 (0.0.0.0) port 0 AF_INET to ::ffff:10.0.1.25 (10.0.1.25) port 0 AF_INET
Recv   Send    Send                          
Socket Socket  Message  Elapsed              
Size   Size    Size     Time     Throughput  
bytes  bytes   bytes    secs.    10^6bits/sec  

 49152  49152  49152    10.00     486.22   

Or at a ridiculously low 2 Mbit/s:

bleonard@opensolaris:~$ pfexec dladm set-linkprop -p maxbw=2 myzone0
bleonard@opensolaris:~$ netperf -H 10.0.1.25
TCP STREAM TEST from ::ffff:0.0.0.0 (0.0.0.0) port 0 AF_INET to ::ffff:10.0.1.25 (10.0.1.25) port 0 AF_INET
Recv   Send    Send                          
Socket Socket  Message  Elapsed              
Size   Size    Size     Time     Throughput  
bytes  bytes   bytes    secs.    10^6bits/sec  

 49152  49152  49152    10.25       1.09   

Good stuff.

I've just scratched the surface of Netperf, but this simple introduction suits my purposes for testing Crossbow. For more fun check out the Netperf manual.

I've had my local IPS repository mirror running for about 1 month now and I find it extremely beneficial. So much so that I've gone ahead and produced a short 6 minute screencast on the process of creating it (although it takes much longer than that to set up as you need to wait for files to download and copy - the joys of editing screencasts).

 Click the image to play the screencast

Not surprisingly, Sun is a big sponsor at this year's fast approaching Oracle OpenWorld . I used to think JavaOne was a big event, but OOW draws about 3 times the attendance. And with Oracle's renewed focus on Sun, you can bet Solaris has a big presence. For your convenience, we've put together a landing page with all things Solaris at Oracle OpenWorld. At a minimum, if you plan to be in the Bay Area the week of October 11th, consider the Discover package. For $75 ($125 on-site) it gets you access to the keynote sessions as well as the exhibit hall where me and my team will be hanging out all week showing off Solaris.

NetBeans 6.7, released earlier this summer, has a pretty nifty Python editor. To give it a spin a decided to set up a project for the Image Packaging System. If you want to try it yourself, here's the steps I took:

Install NetBeans

bleonard@os200906:~$ pfexec pkg install netbeans
DOWNLOAD                                    PKGS       FILES     XFER (MB)
Completed                                  19/19   5638/5638 165.54/165.54 

PHASE                                        ACTIONS
Install Phase                              6756/6756 
Deleting content cache

Install the NetBeans Python Plugin

Start NetBeans (Applications > Developer Tools) and install the Python plugin (Tools > Plugins):

Create the IPS Project

The IPS Python sources are in /usr/lib/python2.4/vendor-packages/pkg, with the exception of the pkg script, which is in /usr/bin. To keep the NetBeans project simple, I copied the pkg script from /usr/bin to /usr/lib/python2.4/vendor-packages/pkg. I also renamed the script to pkg2.py. Adding the .py extension allows it to be recognized as a Python script by NetBeans. Changing the name to pkg2 prevents it from conflicting with the existing script in /usr/bin:

 pfexec cp /usr/bin/pkg /usr/lib/python2.4/vendor-packages/pkg/pkg2.py

In NetBeans select File > New Project and then select Python Project with Existing Sources:

Give the project a name such as PKG or IPS and set the Python Platform to Python 2.4.4:

Then add /usr/lib/python2.4/vendor-packages/pkg as a source root folder:

To give the project a quick test drive, right-click it and select Properties. Then set the Main Module to pkg2.py and the Application Arguments to something like 'info netbeans':

Then select Run > Run Main Project. You'll see the result in the Output window:

Editor Features

Now that we've got the project set up, let's look at some of the features provided by the editor.

Syntax Highlighting 

The code is easy to read.

Code completion

Ctrl+Space to activate.

Hover Documentation and Hyperlink Navigation

Holding down the control key and hovering over Classes and methods will also show you the documentation:

And clicking on the hyper-link will take you to the class or method.

Navigator Window

Also, the Navigator window is a quick way to find your way around a script:

Go to Type

And Go to Type (Ctrl + O) will quickly take you to any type:

Debugger

And finally, one of the coolest features is the debugger. Select Debug > Debug Main Project to start it:

Variables view:

You can find a summary of features on the NetBeans Python Wiki. Please file issues you find with the NetBeans Python Editor.

As I continued to experiment with my local repository mirror, I noticed downloads from the remote repository were running as quickly as from the local repository. Well, I was actually installing and uninstalling the same package to compare speeds and it turns out the files were not actually being downloaded from either repository, but rather copied from a local cache in /var/pkg/download. 

You see, the first time you install a package, it is first copied from the repository to your /var/pkg/download folder and then installed from there. Over time, the size of this folder can grow pretty big. For example, mine was over 3 gigabytes:

bleonard@os200906:~$ du -hs /var/pkg/download/
3.3G    /var/pkg/download/

Note, because there's so many files, the du command takes several minutes to complete.

Fortunately, this cache can be disabled through a property setting. To see the image's current properties, run pkg property:

bleonard@os200906:~$ pkg property
PROPERTY                       VALUE
send-uuid                      True
preferred-publisher            opensolaris.org
require-optional               False
flush-content-cache-on-success False
display-copyrights             True
pursue-latest                  True

Setting the flush-content-cache-on-success property to true will delete your cache on the next successful IPS command:

bleonard@os200906:~$ pfexec pkg set-property flush-content-cache-on-success true
bleonard@os200906:~$ pfexec pkg install SUNWgnome-hex-editor
DOWNLOAD                                    PKGS       FILES     XFER (MB)
Completed                                    1/1       28/28     0.21/0.21 

PHASE                                        ACTIONS
Install Phase                                  83/83 
Deleting content cache

After which you will no longer even have a download directory in /var/pkg.

Note, if you're turning off the cache to save space (as I am), you'll also need to delete the cache from any other boot environments you may have. In those cases, assuming you are not actively using those boot environments, you can just delete the /var/pkg/download directory.

The best way to judge the success of any project, open source or not, is the strength of the development community supporting it. Thats why I was happy to come across Murray Blakeman's site today, Solaris Multimedia. Murry runs his own IPS repository with much of the popular multimedia tools the community's been clamoring for. I was hesitant to advertise it here for a couple of reasons. First, Murray only has a 384 kbps link so I'm not sure how much more publicity his site could handle. Second, I don't want to see Murray to suffer the same fate as the the Life with Solaris guys. Ultimately, I decided since he's already out there promoting his site, a little cross-promotion was acceptable. Plus, as I've said, I'm really thankful to the contribution he's making to the OpenSolaris community.

If you decided to try the repository, read his 2009.06 Multimedia Repository post first on how to most effectively use it.

In my previous entry I wrote about creating a portable version of the repository using a USB stick. That option is great for taking the repository on the road and even sharing it with folks at conferences where the Internet connection usually sucks.

However, a more practical use of this repository image to many of you may be setting up a local mirror. In this situation, you get the best of both words - fast access to the repository with continued access to updates as they become available.

Setting Up the Local Repository

If you haven't already, download the ISO image of the repository (about 7 GB). After the download completes, mount the ISO:

pfexec mount -F hsfs `pfexec lofiadm -a ~/Download/osol-repo-0906-full.iso` /mnt

In order for the mount to persist across reboots, we'll move it to a new file system, which we first need to create:

pfexec zfs create -o compression=on rpool/repo

Then copy the repository to the file system (this will take a little over an hour to complete):

bleonard@opensolaris:~$ pfexec rsync -aP /mnt/repo /rpool/repo
...
repo/updatelog/2009071315
       67506 100%  150.17kB/s    0:00:00 (xfer#304859, to-check=1/609926)
repo/updatelog/2009071316
       24956 100%   55.26kB/s    0:00:00 (xfer#304860, to-check=0/609926)

sent 6669164656 bytes  received 8537336 bytes  1368521.77 bytes/sec
total size is 6630966532  speedup is 0.99

Configure the package server to use the local repository:

svccfg -s application/pkg/server setprop pkg/inst_root=/rpool/repo/repo
svccfg -s application/pkg/server setprop pkg/readonly=true

You can also choose a port number different from the default of 80, which I did because I'm running Apache on port 80:

svccfg -s application/pkg/server setprop pkg/port=81

Edit the repo/cfg_cache file, changing the origins property from http://pkg.opensolaris.org/release  to http://<domainname>:<port>, where <domainname> is network accessible and <port> is needed if you used something other than the default of 80. For example:

origins = http://opensolaris:81

Then refresh the package server service to pick up the configuration changes and start it:

svcadm refresh application/pkg/server
svcadm enable application/pkg/server

Accessing the Local Repository

Now all those wishing to use the local package server simply need to make the following change:

pfexec pkg set-publisher -m http://opensolaris:81 opensolaris.org

Which will result in the following:

bleonard@opensolaris:~$ pkg publisher
PUBLISHER                             TYPE     STATUS   URI
opensolaris.org          (preferred)  origin   online   http://pkg.opensolaris.org/release/
opensolaris.org          (preferred)  mirror   online   http://opensolaris:81/

If you only want to use the local repository, first remove the mirror:

pfexec pkg set-publisher -M http://opensolaris:81 opensolaris.org 

Then:

pfexec pkg set-publisher -O http://opensolaris:81 opensolaris.org

For more information see the README.

A snapshot of the OpenSolaris release repository has been made available for download as an ISO image, where it can be mounted directly or transfered to a USB stick. This will certainly come in handy if you plan to travel somewhere with limited network access but would like access to the repository. In this entry I'll review setting up a USB stick, which gives you a portable repository. In a follow-up entry I'll look at creating a mirror on local file system, which would greatly improve IPS performance for users on a local network.

Putting the Repository on the USB Stick

Download the repository image, which is just over 7 GB. Obviously you'll need at least an 8 GB USB stick. Once plugged in run rmformat to get its device name:

bleonard@opensolaris:~$ rmformat
Looking for devices...
     1. Logical Node: /dev/rdsk/c4t0d0p0
        Physical Node: /pci@0,0/pci1179,1@1d,7/storage@3/disk@0,0
        Connected Device: MATSHITA DVD-RAM UJ-844S  1.11
        Device Type: CD Reader
	Bus: USB
	Size: <Unknown>
	Label: <Unknown>
	Access permissions: <Unknown>
     2. Logical Node: /dev/rdsk/c6t0d0p0
        Physical Node: /pci@0,0/pci1179,1@1a,7/storage@1/disk@0,0
        Connected Device: Verbatim STORE N GO       5.00
        Device Type: Removable
	Bus: USB
	Size: 7.6 GB
	Label: <Unknown>
	Access permissions: Medium is not write protected. 

Use the mount command to find the device instance:

bleonard@opensolaris:~$ mount | grep c6t0d0p0
/media/STORE N GO on /dev/dsk/c6t0d0p0:1 read/write/nosetuid/nodevices/hidden/nofoldcase/clamptime/noatime/timezone=18000/dev=9810d0 on Fri Jul 31 11:07:12 200

Then unmount it:

bleonard@opensolaris:~$ rmumount /dev/rdsk/c6t0d0p0:1
/dev/rdsk/c6t0d0p0:1 /dev/dsk/c6t0d0p0:1 unmounted

Now you can copy the ISO to the device:

bleonard@opensolaris:~/Download$ pfexec dd if=osol-repo-0906-full.iso of=/dev/rdsk/c6t0d0p0 ibs=32K obs=32K
234931+1 records in
234931+1 records out
7698249728 bytes (7.7 GB) copied, 759.871 s, 10.1 MB/s

You can see the operation took almost 13 minutes to complete. Optionally you can label the device:

rmformat -b 'repo0906' /dev/rdsk/c6t0d0p0

Using the USB Stick as a Repository

IPS is a network based packaging system, therefore we need to configure an IPS server on the local machine to look at the USB stick as its repository.

Plug the USB stick into the machine that needs access to the repository. It should be automatically mounted into your /media directory.

bleonard@opensolaris:~$ ls /media
0906FULL/

Next configure the local package server with the location of the repository (if you are interested in seeing the existing set of properties, run svccfg -s application/pkg/server listprop):

svccfg -s application/pkg/server setprop pkg/inst_root=/media/0906FULL/repo
svccfg -s application/pkg/server setprop pkg/readonly=true 

Optionally, change the pkg server's port number from the default of 80. I'm already running Apache on port 80, so I'll use 81 for the repository server:

svccfg -s application/pkg/server setprop pkg/port=81

Copy the repo/cfg_cache file to the local file system so it can be edited:

pfexec cp /media/0906FULL/repo/cfg_cache /etc/0906_cfg_cache

Edit the file and change the origins property from http://pkg.opensolaris.org/release  to http://localhost:81. Be sure to include the port number if you changed it (note, if you also want the repository accessible to other machines, then use an IP network-accessible domain name):

origins = http://localhost:81

Configure the package server service to use the local configuration file:

svccfg -s application/pkg/server setprop pkg/cfg_file=/etc/0906_cfg_cache

Refresh the package server service to pickup the configuration changes and then start it:

svcadm refresh application/pkg/server
svcadm enable application/pkg/server

At this point you should be able to browse the local repository at http://localhost:81:

The final step is to configure IPS to access the repository:

pfexec pkg set-publisher -O http://localhost:81 opensolaris.org

You're now free to install packages on a plane. 

For more information, see the README.

Reverting Back

It's simple to switch back to the default release repository:

pfexec pkg set-publisher -O http://pkg.opensolaris.org/release opensolaris.org

The next time you need the "repo on a stick", just plug in the USB and switch the publisher back to http://localhost.

pfexec pkg set-publisher -O http://localhost:81 opensolaris.org

Chime has a nifty little feature where you can run it in server mode and then monitor the system remotely using the Chime GUI.

On the server simply run:

bleonard@opensolaris:~$ chime server
Listening for remote DTrace consumers on port 5088
Press the Enter key to stop the server.

Then on the client point chime to the server:

chime 10.0.1.10

At least it's supposed to be that easy, however, there's a small issue with Java RMI that prevents this from working correctly.

I did some research on RMI and discovered you have two options to solve this problem.

Option 1 is to add your server's IP address to /etc/hosts as follows and restart the chime server.

127.0.0.1	opensolaris opensolaris.local localhost loghost
10.0.1.10	opensolaris

Alternatively, you can edit the /opt/OSOL0chime/bin/chime script on the server to include the following JVM property (Of course supplying the proper IP address):

JMX_FLAGS="${JMX_FLAGS} -Djava.rmi.server.hostname=10.0.1.10"

Choose either option and you should then be able to successfully monitor the remote system.