1 /*
2  * CDDL HEADER START
3  *
4  * The contents of this file are subject to the terms of the
5  * Common Development and Distribution License, Version 1.0 only
6  * (the "License").  You may not use this file except in compliance
7  * with the License.
8  *
9  * You can obtain a copy of the license at usr/src/OPENSOLARIS.LICENSE
10  * or http://www.opensolaris.org/os/licensing.
11  * See the License for the specific language governing permissions
12  * and limitations under the License.
13  *
14  * When distributing Covered Code, include this CDDL HEADER in each
15  * file and include the License file at usr/src/OPENSOLARIS.LICENSE.
16  * If applicable, add the following below this CDDL HEADER, with the
17  * fields enclosed by brackets "[]" replaced with your own identifying
18  * information: Portions Copyright [yyyy] [name of copyright owner]
19  *
20  * CDDL HEADER END
21  */
22 /*
23  * Copyright 2005 Sun Microsystems, Inc.  All rights reserved.
24  * Use is subject to license terms.
25  *
26  * This D script is used as an example in the Solaris Dynamic Tracing Guide
27  * wiki in the "profile Provider" Chapter.
28  *
29  * The full text of the this chapter may be found here:
30  *
31  *   http://wikis.sun.com/display/DTrace/profile+Provider
32  *
33  * On machines that have DTrace installed, this script is available as
34  * restest.d in /usr/demo/dtrace, a directory that contains all D scripts
35  * used in the Solaris Dynamic Tracing Guide.  A table of the scripts and their
36  * corresponding chapters may be found here:
37  *
38  *   file:///usr/demo/dtrace/index.html
39  */
40 
41 profile-5000
42 {
43 	/*
44 	 * We divide by 1,000,000 to convert nanoseconds to milliseconds, and
45 	 * then we take the value mod 10 to get the current millisecond within
46 	 * a 10 millisecond window.  On platforms that do not support truly
47 	 * arbitrary resolution profile probes, all of the profile-5000 probes
48 	 * will fire on roughly the same millisecond.  On platforms that
49 	 * support a truly arbitrary resolution, the probe firings will be
50 	 * evenly distributed across the milliseconds.
51 	 */
52 	@ms = lquantize((timestamp / 1000000) % 10, 0, 10, 1);
53 }
54 
55 tick-1sec
56 /i++ >= 10/
57 {
58 	exit(0);
59 }
60