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8/20/2019 Unix Release Notes
1/76
Landmark Desktop-VIP
VIP 2003.3.0 UNIX/Linux Release Notes Page 1 December 2001
VIP Simulators 2003.4
UNIX and Linux Release Notes
Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7
System Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10
Enhancements and New Features . . . . . . . . . . . . . . . . . . . 15
Installation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .27
LAM License Manager . . . . . . . . . . . . . . . . . . . . . . . . . . . . .29
Setting the Environment . . . . . . . . . . . . . . . . . . . . . . . . . . . . 35
Appendices . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .39
Landmark/Asia Pacific
11th Floor Menara Tan & Tan
207 Jalan Tun Razak
50400 Kuala Lumpur
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Tel: 011-60-3-264-1121
Fax: 011-60-3-264-1135
Help Desk: 011-61-8-9481-4488
Email: [email protected]
Landmark/EAME
Benchmark House
203 Brooklands Road
Weybridge, Surrey KT13 ORH
England
Tel: 011-44-193-282-9999
Fax: 011-44-193-283-2000
Help Desk: 011-44-193-283-2100
Email: [email protected]
Landmark/The Americas
15150 Memorial Drive
Houston, Texas 77079
U.S.A.
Tel: 281-560-1000
Help Desk: 281-560-1200
Fax: 281-560-1168
Email: [email protected]
http://installnew.pdf/http://installnew.pdf/http://installnew.pdf/
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Table of Contents
Introduction
What’s New . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7
VIP Unix/Linux Users . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8
System Requirements
Sun Solaris Operating Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10
Tested Environment . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10Parallel Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10
Additional Software Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10
Additional Hardware Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10
IBM AIX Operating Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11
Tested Environment . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11Parallel Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11
Additional Software Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11
Additional Hardware Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11
SGI IRIX Operating Systems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12Tested Environment . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12Unique Parallel Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
Software Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12Hardware Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
Linux Operating System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13
Tested Environment . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13Unique Parallel Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13
Software Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13
Hardware Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13
Enhancements and New Features
Version R2003.4 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15
VIP-Executive . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15
General . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15 New Features . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15
Modified Features . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17VDB Database . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 18DeskTop-VIP User Interface . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19
VIP Job Submittal . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20Known Issues . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20
SimResults / SimResults+ . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21
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Known Issues . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21VIP Convert . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21
VIP Data Studio . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22VDS-CORE . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22VDS-EXEC . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22
Known Issue . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23Grid Calculator (GridCalc) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 24
Known Issue . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 24Region Calculator (RegCalc) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 24E2V . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25
GridGenr . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26
Installation
VIP Installation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 27
LAM License Manager
Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 29
Version Compatibility . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 29
Understanding the License Process . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 30
Using the License System with Third-Party Software . . . . . . . . . . . . . . . . . . . . . 30
LAM 2003.0 Guide -- Linux and Unix . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31
LAM System Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31Operating System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31
Hardware Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31Obtaining a Server License File . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31Installing LAM Server . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34Controlling the License Server . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 38
Starting and Stopping the License Server . . . . . . . . . . . . . . . . . . . . . . . . 39Setting the Environment Variable . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39Defining License Groups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39
LAM Technical Notes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41
If Applications Cannot Find License File . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41Overriding LM_LICENSE_FILE . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41Restricting the Use of FLEXlm Utilities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
Setting the Environment
Setting the User’s Environment . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 43Without OpenWorks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 43
Other Important Environment Variables . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44
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Appendix A: Parallel Computing
Getting Started with PARALLEL-VIP . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47Include File Configuration Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47Which Systems Will Parallel-VIP Run On? . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47
Where Should You Run From? . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48Running on IBM SP Workstations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48
Running on Shared Memory Silicon Graphics, Solaris, and LinuxWorkstations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48
File System Set Up . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48
.rhosts File . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 50Remote Shell Capabilities . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 50Testing for Valid rsh Performance . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51
Other Notes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
Appendix B: NFS Mounting Requirements for Parallel or Remote Submission
Manual Mounts . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 53Assumptions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 53Tests . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 53
Automount Mounts . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 54Assumptions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 54Tests . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 55
Environment Variables and Guidelines . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 55Rules . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56
Appendix C: Setup Instructions to Submit Jobs via Remote Shell
Overview . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57
Assumptions: About the User’s Network . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 58
Key Commands . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 59
Key Files . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 60
Job Submission Panels . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 67
Restrictions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 67
Appendix E: SP2 POE Checkout GuidelinesAppendix F: Modifying a Samba Server to Work with VIP Applications
Using Samba shares in Remote Windows VIP Submissions or Parallel Windows VIPSubmissions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73
Using Samba Versions 2.2.2 and Higher with VIP applications. . . . . . . . . . . . . . . . . . . 74
Example smb.conf File Used During Testing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 75
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Desktop-VIP 2003.4 Release Notes Page 7 Introduction
Introduction
These Release Notes provide the necessary information to correctly install
DESKTOP-VIP Release 2003.4 on Windows 2000 machines. They also containoperating system support levels and required third party software, as well as
instructions for setting up parallel configurations, network dependencies andtested hardware configurations. Instructions for uninstalling older versions ofDESKTOP-VIP and related third party software are also included in these
Release Notes.
What’s New
DESKTOP-VIP R2003.4 provides a graphical user interface that is certified onWindows 2000 Service Pack 1 and 2. It has also been tested on Windows XPProfessional, with no problems detected. VIP simulators are certified on
Windows 2000 SP1 and 2, as well as Solaris 8, IRIX 6.5.11m, and AIX 4.3.3,
and Linux Red Hat 7.2. VIP simulators have also been tested on Windows XPProfessional with no problems detected.
This release provides a wide range of enhancements, including the followingmajor changes to Windows-based user interface applications:
■ Desktop. The new JAVA-based Desktop has a Windows look-and-feel, with
features like docking/floating toolbars and mouse-over tooltips. Study/Case management and network access from the Desktop has beenimproved.
■ Job Submittal. The new JAVA-based Job Submittal application withemphasis placed on ease-of-use, job queueing, remote job submittal,and input/output/include file management.
■ SimResults and SimResults+. The SimResults plotting application takes
advantage of Windows-based features such as drag-and-drop to let you more
efficiently use those plotting capabilities that were available in PlotView.
SimResults+ (license required) also lets you create RTF plots, allows for
batch plotting, and provides a seamless interchange between Eclipse and VIP
data and .grf templates.
■
Enhancements to VIP Data Studio. This efficient, wizard-driven applicationhas been expanded to let you create VIP-CORE as well as VIP-EXEC data
files.
■ VIP Convert. This powerful conversion application now lets you export and
import Rescue geocellular model data.
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■ RegCalc (Region Calculator). This new application lets you quickly obtain
pressure, saturation, and fluids in place at any timestep for both your
IREGIONS and any arbitrary I,J,K area (not defined as an IREGION).
DESKTOP-VIP R2003.4 provides numerous enhanced simulation capabilities,
including:
■ Enhanced Surface Pipeline Network, including optimization of well and
gaslift gas rates, and multiple output streams from nodes.
■ A basic implementation of injection networks in addition to production
networks.
■ Version independent restarts from R2003.4 forward. (A utility is provided to
convert from R2003.0 to R2003.4)
■ Option for control of gas re-solution rate. (DRSDT)
■ Support for multiple water PVT regions, including optional propertyvariations with salinity.
■ Optimization of gaslift gas utilization at all targeting levels.
■ Threshold pressure option for fault flow.
■ Simultaneous bottomhole and tubinghead pressure constraints.
All new and enhanced functionality is described in the Enhancements and New
Features section of this document.
VIP Unix/Linux Users
Desktop-VIP graphical user interface applications are only available onWindows 2000. Except as noted below for Geolink and 3DView, only Unix andLinux simulators are provided and can be found on separate CDs. You can use
the Desktop-VIP on Windows 2000 to submit remote simulation jobs (serial or parallel) to Unix/Linux machines. GeoLink certified on Solaris and IRIX platforms is part of the Stratamodel R2003.0 offering. A certified version of
3DView for Solaris and IRIX is part of the OpenVision R2003.0 offering. Atested version of 3DView for Linux is part of the OpenVision R2003.3 offering.
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System Requirements
The minimum hardware requirements are a UNIX or Linux workstation with 200
MB of free disk space to store the VIP simulation software, as well as a CD drive
either local or mounted across the network for unloading the software from the
installation CD.
The amount of memory and swap space necessary to run VIP is dependent on the
size of the model. However it is recommended that you have at least the following
minimum configuration. This allows a model with approximately 100,000 grid
blocks to be run.
Minimum RAM: 256 Megabytes
Minimum Swap: 512 Megabytes
Minimum tmp: 512 Megabytes
Minimum Disk: 4 GB system/ 9GB user space
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Sun Solaris Operating Systems
Serial and parallel VIP executables are available for Solaris operating systems.
Tested Environment
VIP R2003.4 was tested on Solaris 8 (SunOS Release distributed October 10, 2000).
Parallel Requirements
Parallel-VIP was tested on Solaris 8 running on shared memory Solaris
workstations. For additional information on parallel computing requirements,
refer to Appendix A.
Additional Software Requirements
The Message Passing Interface (MPI) Version 1.1.0 is required and is supplied on
the VIP installation media.
Additional Hardware Requirements
Shared memory Solaris workstation with two or more CPUs in a single machine.
It is recommended that sufficient disk space is added to provide adequate swap,
tmp, and storage space. The executables for Paralled-VIP to run in a distributed
cluster across two or more separate Solaris machines are not provided.
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IBM AIX Operating Systems
Serial and Parallel VIP executables are available on AIX operating systems.
Tested Environment
VIP R2003.4 was tested on AIX 4.3.3.
Parallel Requirements
SP platforms running IBM’s Parallel Operating Environment. A distributed
version, running MPI, is not available. For additional information on parallel
computing requirements refer to Appendix A.
Additional Software Requirements
• Parallel Operating Environment (POE) 2.4
• Parallel System Support Program (PSSP) 3.1.1
Additional Hardware Requirements
It is recommended that sufficient disk is added on each node to minimally provide
swap space and tmp space that is two times larger than real memory. Other disks
should be added locally to the SP to store user files.
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SGI IRIX Operating Systems
Serial and Parallel VIP executables are available on IRIX operating systems.
Tested Environment
VIP R2003.4 was tested under IRIX 6.5.11m.
Unique Parallel Requirements
Parallel-VIP runs on a 64-bit SGI Shared Memory workstation (8000 or greater;
i.e. Power Challenge, Origin, Octane) that has two or more CPUs. For additional
information on parallel computing requirements refer to Appendix A.
Software Requirements
The Message Passing Interface (MPI) Version 1.1.0 is required and is supplied on
the VIP installation media.
Hardware Requirements
Shared memory SGI workstation with two or more CPUs in a single machine. It is
recommended that sufficient disk is added to provide adequate swap, tmp, and
storage space. The executables for Paralled-VIP to run in a distributed cluster
across two or more separate Solaris machines are not provided.
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Linux Operating System
Serial and parallel VIP executables are available on Linux operating systems.
Tested Environment
VIP R2003.4 was tested under Linux Red Hat Version 7.2.
Unique Parallel Requirements
Parallel-VIP runs on a Linux Distributed Memory workstation that has two or
more CPUs. For additional information on parallel computing requirements refer
to Appendix A.
Software Requirements
The Message Passing Interface (MPI) Version 1.1.0 is required and is supplied on
the VIP installation media.
Hardware Requirements
Distributed memory Linux workstation with two or more CPUs in a single
machine. It is recommended that sufficient disk is added to provide adequate
swap, tmp, and storage space. Parallel-VIP will run in a distributed cluster across
two or more distinctively separate Linux machines.
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Enhancements and New Features
Version R2003.4
This release of DESKTOP-VIP provides the following new and modifiedfeatures for both the Unix/Linux and Windows versions.
VIP-Executive
The following notes describe features which were added or modified in VIP-
EXECUTIVE. Some of these features offer new capabilities and others offer better efficiency. Features that are pertinent only to VIP-CORE or VIP-EXECare listed separately.
General
1. Change bars specific to version R2003.4 have been retained in the CORE and
EXEC user manuals to aid the user in quickly locating new/modified
information.
2. Note: VDB and map files have always been required to have ROOT as the
root grid name. If the root grid is renamed in VIP-CORE (LGR ROOTGRID
option), all input data is required to use this name and output files will reflect
this name, but applications such as 3DView that read from the VDB will show
the root grid as ROOT.
New Features
1. Version-independent restart files: The restart files have been restructured
to enable the flexibility of version-independent restart files. For all future
versions, VIP-EXEC will be able to restart from any prior restart files,
eliminating any requirement to rerun the entire study when moving to a new
version. A utility program is provided to convert current R2003.x restart files
to the new structure, enabling R2003.4 to restart from converted R2003.x
restart files.
Converting Restart Files:
Modify script for VIPHOME. Using your text editor (such as Notepad orvi), open the script file (rstconv.bat on Windows or rstconv.ksh on Unix/
Linux) located in your VIP directory path /vip/dtvip/cvrst. On the followingline, edit the file to point to your VIPHOME location.
set VIPHOME=net/machinename/vip
Save and close the file.
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Run the conversion. In the case file directory, type the following at the
command line prompt:
rstconv
You need only specify the base restart file name (filenamei.rst) for a CORE
run and base output restart file name (filenamer.rst) for an EXEC run. Thescript will then read and convert multiple restart files: filenamei.rst,
filenamei.rst0, filenamei.rst1, ... , where a numbered file is expected for each
grid.
2. Control of gas re-solution rate: In conjunction with the new extended form
of the black-oil PVT tables (BOETAB, etc.), a new DRSDT variable has been
added which enables the user to limit the rate of increase of the solution gas-
oil ratio, Rs.
3. Multiple water properties regions: Enables the user to specify different
water PVT regions, with different properties in each region, in a manner
analogous to the specification of different hydrocarbon PVT regions.
4. Water properties variation with salinity: Allows the user to specify the
variation in water properties as a function of salinity for any water PVT
region, enabling more precise modelling of fresh water injection. The salinity
of the injected water can be specified for each water injection well.
VIP-CORE
1. Aquifer connections to LGRs: Enables aquifers to be connected to any
gridblock within any grid, rather than being limited to the base grid, only.
2. Limits removed for the reference depth for the initial pressure in anequilibrium region which has an active gas-oil contact: The reference
depth for the initial pressure in an equilibrium region involving an active gas
cap is now allowed to be outside of the oil leg, since the phase pressure
profiles will be based on the saturation pressure at the GOC.
3. XREG values can be read for each gridblock . XREG data can also be read using a value for each gridblock in the window. Previously,
only one value could be applied to the whole window.
Known Issue:
1. The CORE keyword VDB filename.vdb only works for local runs.
VIP-EXEC
1. Enhancements to the production Surface Pipeline Network (SPN) option:
A number of enhancements have been made to the production SPN. These
include the following:
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a. Optional well rate and gaslift gas rate optimization.
b. Pseudo well option for satellite field modelling.
c. Allow multiple output streams from nodes.
d. Simplified heat-transfer analysis extended from wells to nodes.
2. Basic implementation of an SPN for injection wells: Enables a separate
network to be defined and used for the injection system.
3. Optimization of gaslift gas utilization at all targeting levels: Enables the
user to solve for the minimum gaslift gas required to make the production
targets at any level, outside of SPN.
4. IMPWEL now available with OPTMBL and Crossflow: The implicit well
option with the IMPES formulation can now be used in conjunction with both
OPTMBL and the wellbore crossflow options.
5. Threshold pressure option for fault flow: Enables the flow across aspecified fault to be blocked until the pressure potential exceeds the specified
threshold. When exceeded, the potential is reduced by the value of the
threshold, and flow is allowed based on the adjusted potential.
Modified Features
VIP-CORE
1. Automatically connect analytical aquifers to only gridblocks below the
water-oil contact: In previous versions, connections were made to all
gridblocks specified, irrespective of whether they were above or below thecontact.
Fixed Problems
1. MULT PLUS data now propagates correctly to children LGRs.
2. MULTFL now works correctly with LGR or DECOMPOSE and no longer
results in convergence failures in EXEC.
3. Some pinchouts across LGRs with OMITs could be missed.
4. Multi level LGR or DECOMPOSE grids no longer have corrupted map filesthat cannot be loaded into 3DView.
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VIP-EXEC
1. Support for both previous algorithm and iterative damping for
OPTMBL: In the R2003.0 release, iterative damping was introduced with no
ability to request the old algorithm. Now the old algorithm is the default, and
iterative damping may be requested by specifying DAMP on the OPTMBL
card.
2. Support simultaneous THP and BHP constraints for wells: The simulator
will now allow and utilize both THP and BHP constraints for a well
simultaneously, honoring the more restrictive of the two. Previous versions
would use only the last one entered, negating either of the two previously
entered.
3. Make-up gas rate and composition of injected gas: The actual required
rate of make-up gas to satisfy the gas reinjection requirement is now correctly
calculated and reported, as well as the correct injection gas composition
involving the produced gas plus required make-up gas.
4. Default for the automatic solver cutback changed to OFF: In the R2003.0
release, a new feature was introduced within the solver to attempt to
determine either very slow convergence or divergence, and terminate the
solution effort, with the idea being to save the excess CPU time of continuing
to maximum iterations and then cutting the timestep. After finding several
models in which this hurt the overall performance, the default is changed to
OFF, and the user must explicitly turn it on if deemed necessary.
5. Enhanced convergence and constraints on the welbore gradient methods:
Enhanced convergence criteria and tighter constraints within the iterative
wellbore gradient calculations now yield much better performance for a few
special cases wherein the previous versions produced premature shut in ofsome wells.
6. Numerous additions to the various output files: Significant additions have
been made to the output capabilities of the spreadsheet, plot, and map files.
Fixed Problem
1. Excessive memory utilization in the solver for inactive gridblocks.
VDB Database
The following notes describe features which were added or modified in the VDBdatabase.
1. New structure implemented: A new VDB directory structure has been
implemented to replace the single-file VDB model. This new structure:
❑ Allows for faster data access
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❑ Allows more simulation runs for a single study without hitting the 2GB
file size limit
❑ Eliminates the need for VDB defragmentation
The new VDB structure is described in detail in the Starting and Using
Desktop-VIP chapter of the Getting Started manual.
Convert old VDBs by running this command at the command-line prompt
from within the directory containing the old VDB:
vdbconverter
All DeskTop-VIP applications can easily handle both old and new style VDB
files. The command-line executable will also convert from the new to the old
format.
2. VDB control file provided: An XML control file has been provided in the
top-level directory of the new VDB allows users to easily see the list of cases
and parent-child relationships among them
3. Simultaneous VDB access: Multiple VIP simulation jobs can now access the
VDB simultaneously.
DeskTop-VIP User Interface
The following notes describe features which were added or modified in theDesktop.
1. GUI redesign and new features: The DeskTop user interface has been re-
written in Java, eliminating all dependencies on Tk/Tcl. It now has aWindows look-and-feel, with features including docking/floating toolbars,
mouse-over tooltips, etc.
2. Improved study/case management: The new DeskTop user interface allows
the user to load multiple VIP studies onto the Desktop and easily switch back
and forth between active studies/cases. The VDB study/case hierarchy is now
visible to the user on the Desktop, and studies/cases can be added, deleted, or
modified from the Desktop. Data types contained in the study/case are easily
visible to the user at all times.
3. Study/case comments can be added: The user now has the ability to add
study/case comments which can easily be viewed.
4. Persistence of user preferences: Changes/preferences set by the user are
persisted from session to session.
5. Improved network access. The network can be now accessed from the file
selection dialog box.
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VIP Job Submittal
The following notes describe features which were added or modified in VIP JobSubmittal.
1. GUI redesign and new features: The VIP Job Submittal interface has been
totally redesigned, with the emphasis placed on ease-of-use, job queueing,
and remote job submittal.
2. Input, output, and include files shown:. The Job submittal panel now
displays all input files, output files, and include files associated with a given
VIP job.
3. Improved simulation messages: The feedback to the user while jobs are
executing has been improved.
4. More control over the run: Jobs can now be run as a background process
and multiple jobs can run simultaneously. The user can now choose which
simulator version to use for each run.
5. Real-time plotting: A user-configurable feature has been added for real-
time plotting of simulation results while a job is running.
6. Local or remote queueing: Jobs can be queued to run either locally or
remotely.
7. Batch plotting for automatically-generated plots: Batch plotting has been
improved for automatically generating plots of simulation results. Output can
be sent to the default printer, to Microsoft Word document, Excel document,
Powerpoint document, or HTML files.
Known Issues
1. For remote runs using this release version, the directory that is one level
above the Study directory is reserved for remote copy procedures. Therefore,
no primary data files ( i.dat and r.dat ) or restart files ( i.rst and r.rst ) may exist
in the directory immedi-ately above the Study Directory. If they do, they will
be copied to the directory immediately above the remote working directory.
The simulator will not be able to find them during the remote run and the
simulation will fail
2. When specifying the location of include files, it is recommended that the user
always specify fully qualified paths. Relative paths will only work one levelhigher (../) and one level lower (./); however there are situations where they
will not work at all.
3. The VDB option in CORE is not supported for remote jobs submitted from
Desktop-VIP, if the *.vdb file is to be automatically copied to the remote
machine. However, if the user manually copies the *.vdb file to the working
directory on the remote machine, the VDB option will function properly.
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SimResults / SimResults+
A new Windows-based plotting package has been added to Desktop-VIP toreplace PlotView. (PlotView has been retained on the Desktop for this release.)
1. SimResults drag-and-drop GUI: SimResults provides all the functionality
that was available in plotview, within a drag-and-drop user interface for
creating X/Y plots and 2D maps.
2. SimResults+ enhanced functionality: SimResults+ provides additional
functionality, including:
❑ Full batch plotting support via GRF scripting language
❑ RFT plotting
❑ User definable derived quantities
❑ 2D map display for VIP map data
Known Issues
1. If you have a new Windows 2000 machine, Microsoft Office must be installed
in order to run SimResults.
2. If you are a new user or have a new Windows 2000 machine, then the
message prompting for Office 2000 SR-1 disk is produced if SimResults (or
any application that has been compiled using Visual Studio) is run.
Work-around: This issue can be solved by running any office application
once, e.g. start Word then close it down.
VIP Convert
The following notes describe features which were added or modified in the VIP
Convert conversion utility.
1. Additional export capability: VIP Map, VIP CORE, Landmark Active
Field Surveillance (AFS) and Rescue files can now be exported from the
VDB study/case.
2. Additional import capability: RESCUE models can now be imported into aVDB file.
3. VDB viewing from the VIP Convert application: A new VDB “View”
panel has been added to allow the numerical data contained in a VDB study/
case to be viewed.
4. Improved status reporting. Status reporting to the user while VIP Convert is
processing files has been improved.
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VIP Data Studio
The following notes describe features which were added or modified in VIP-Data Studio. Features that are pertinent only to VDS-CORE or VDS-EXEC arelisted separately.
1. External data can now be imported or entered: Data can be be parsed,
and unrecognized parsed data is now saved as an include file for import.
2. Summary (error) page provided: A summary page of the model is now
displayed to the user before the data set is generated. The summary provides
basic error checking (missing data, obvious errors).
3. Color-coded icons: Icons have now been added to each data type in the
options tree. A green icon indicates that all required data has been entered. A
yellow icon indicates that no data has been entered but none is required. A
red icon indicates that mandatory data is missing.
VDS-CORE
A user interface has been added to create basic CORE initialization files. It letsthe user parse an existing initialization file and import tables from existingdatasets. It also provides a creation wizard to quickly generate the basic
requirements for an initialization file from scratch.
Data Studio CORE supports the following data:
• Basic utility data• Local grid refinement
• Limited support for advanced utility features (Dual, Therm, etc.)• Equilibrium tables• Rock tables (relative permeability and compaction)
• PVT tables for black-oil, water-oil, gas-water, EOS• Basic correlations to generate relative permeability tables and black-oil/
water-oil, gas-water PVT
• EOS separators• Grid data – through view for simple grid arrays or as include file• Grid Array functions
• Grid Modifiers• Aquifers
VDS-EXEC
• New production data options available. The Production Data panel nowsupports:
• Active Field Surveillance (AFS) file import• User-defined conversion factors through the import wizard
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• Class header definition for export to OBS format through the import wiz-ard
• Appending of imported pressure data after importing rates/volumes,allowing different time frequency for pressure measurements
• Generation of types and rate constraints from raw production data (no
averaging required)
• New output options available: The Output panel now supports:
• RFT output (well selection)
• SSSUM option• Compositional MAPX/Y/Z and OUTX/Y/Z options
• New well perforations options available: The Well Perforations panel now provides:
• An import wizard to generate VIP PERF cards from a simulation gridwithin a VDB and some basic well data• Ability to filter displayed perfs by well, date, and/or well name
• New well constraints options available: The user can now view all con-straints for a well. The Well Constraints panel now supports the following
constraints:
• Hydraulic table assignment
• Gas Producer THP table assignment• Tubing length
• Tubing diameter friction factor • Crossflow model activation• Minimum rate scale-back for targeting
• New well hierarchy option available: Basic injection and production tar-geting plus hierarchy ontime factors is now supported.
Known Issue
1. When launching 3DView from the VIP Data Studio perforation wizard, the
3DView main window sometimes locks due to an Exceed problem.
Workaround: close the DOS command window that comes up whenlaunching 3DView from the perforation wizard. (This will also close the
current 3DView without killing Exceed). Then relaunch 3DView from the
perforation wizard.
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Grid Calculator (GridCalc)
The following notes describe features which were added or modified theGridCalc utility.
1. GUI redesign: The user interface has been redesigned with a Windows
look-and-feel.
2. New trigonometric functions added: Sine, cosine, tangent, and square-root
functions have been added to the calculator pad.
3. Summation capabilities added: The user can now perform summations by
time or by layer.
4. Temporary variables can be created: The user can now create temporary
variables as building blocks for more complex permanent variables. The
temporary variables are deleted at the end of the session.
5. Improved error-checking and messages: The application now performsmore complete error-checking and provides better error messages to the user.
Known Issue
1. In GridCalc expressions, the program only recognizes VDB and Case names
that start with an alpha character. For example "name2" is a recognized VDB
or Case name in an expression, but "2name" is not. Workaround: if you
want to use a VDB or Case name that does not begin with an alpha character
in an expression, select it as the active Project and Case. Then create the
expression without specifying a Project or Case. When not specified, the
program assumes the current Project and Case by default.
Region Calculator (RegCalc)
The following notes describe features which were added or modified theRegCalc utility, which replaces MapCalc.
1. GUI redesign: The user interface has been redesigned with a Windows
look-and-feel.
2. New features to aid in transfer of data to spreadsheet: A new Copy
feature lets the user easily copy data to the Clipboard to paste into a
spreadsheet application. A new Export feature lets the user quickly create atab-delimited file for import into a spreadsheet application.
3. Improved report options: Multiple timesteps can now be included in a single
report. New Print Preview and Column Layout control has been added to give
the user more control over the report hardcopy.
4. Improved error-checking and messages: The application now performs
more complete error-checking and provides better error messages to the user.
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E2V
The following notes describe features which were added or modified the E2Vutility.
1. Extended black oil table data converted: Extended black oil table (e.g.
BOETAB) data is now converted to VIP format.
2. Multiplication data now converted: Data for multiplying named faults
(MULTFL) and multiplying transmissibilities between reservoir regions
(MULTIR) is now converted into VIP format.
3. Observed file can now be created: An option has been added to create an
observed data file (*.obs) during the conversion process.
4. Eclipse BHP reference depth can be converted: The default BHP reference
depth (depth to top perforation) from Eclipse has been added as an option.
5. Well scheduling data can now be created: Well scheduling data can now becreated in a compressed format based upon user selection.
6. Conversion improvements have been made: A variety of bug fixes have
been added to make the conversions more complete and reliable.
Known Issues
1. For Eclipse data sets containing non-monotonic PVT data, the converted data
set may report errors when run in VIP. In some cases, E2V slightly modifies
the data to cause monotonic behavior, but in other cases the data is not
adjusted.
2. The conversion of Eclipse gas and oil viscosity in the PVT tables cannot be
guaranteed. You should manually check and verify this data.
3. The conversion of MULTZ data in Eclipse to TMZ data in VIP may have
errors.
4. When Eclipse data has UTM coordinates, you must choose the right-handed
option in order to ensure the correct results. The left-handed option (default)
is not guaranteed to work correctly.
5. For VIP, the matrix and fracture systems must have the same equilibration
region specified by the IEQUIL array; there is no IEQUILF array. Eclipseallows the matrix and fracture systems to have different equilibration region
specification for each grid block.
6. GASWATER and WATEROIL options are not allowed in VIP-DUAL.
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GridGenr
The GridGenr model size limitations were retested with the following results:
1. Grid points per zone. The maximum number of grid points per zone
increased from 60,000 to 300,000.
2. Mesh size. The maximum size of a mesh increased from 500,000 to
1,000,000.
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Installation
The VIP simulator installation CDs are written in standard Landmark Graphics
CD Release Manager (CDINSTALL) format. They are used to install VIP on all
supported UNIX and Linux platforms.
This install media contains the shell script “setup” and the necessary tools to
extract the application from CD and transcribe the application to disk.
For UNIX, the CDINSTALL packs the application in such a manner that the
application itself cannot be run from CD. It must first be transcribed to disk, then
invoked from disk. This is accomplished by running the Release Manager. For
Linux, an auto-mount is provided. Once the CD is inserted, you need only cd to
the directory /mnt/cdrom/install.
The CD Release Manager program provides a consistent GUI-based interface for
installing VIP. After you specify the programs to be installed and the directories in
which to install them, the program provides a graphical status display of theinstallation’s progress. Do not use the upgrade option as it is not functional.
Please refer to the next chapter for procedures on mounting and managing the
license server.
VIP Installation
After inserting the VIP CD into your local CD drive, login in as “root” and change
directories to your CD drive. Change directories to the “install” directory and type
the following command:
./setup
The following message appears:
|----------------------------------------------------|
| Landmark Graphics Corporation |
| Release Manager |
|----------------------------------------------------|
Log files are written to CDINSTALL_LOG
CDINSTALL_LOG is set to : /tmp
Is this correct [y]?
OWHOME must be set: A full path is required Please enter path:
If you have OpenWorks, enter the full pathname to your OpenWorks 2003 home
directory. This pathname is used to determine where to locate the VIP installation.
For example, if your OpenWorks area is located under /usr/apps, the full
pathname should be entered as /usr/apps/OpenWorks.
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If the environment variable OWHOME is defined before starting the CD install
procedure, then the question above never appears and the pre-defined OWHOME
directory path is used as the installation location. VIP will be installed in a
directory relative to the installation location. For example, if the installation
location is /usr/apps/OpenWorks, VIP is typically installed in /usr/apps/
OpenWorks/vip.
If you do not have OpenWorks, similar rules apply, except that you supply a full
directory pathname the location on your file system where you want VIP
installed. For example, if the pathname you supply is /usr/apps, VIP is installed
in /usr/apps/vip.
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Understanding the License Process
The license process is described in detail in the LAM Guide that was
included in the R2003.0 release. Refer to the Guide for a detailedexplanation of licensing.
Using the License System with Third-Party Software
Because Landmark’s License System uses FLEXlm from Globetrotter,administrators must be careful when installing other third-party
software that also uses FLEXlm (Sun’s compilers, Charisma, etc.).
When your environment contains Landmark applications (either VIP
only or in combination with other products such as OpenWorks) andother third-party software, there are two ways to manage the licensesystem:
• The first (and easiest) way produces separate license systems.Landmark applications reference one license system while third-
party software references the other license system.
• The second (more complicated) way produces a single license
system that is used by both Landmark applications and the third- party software.
Procedures for each type of license set-up are described in the LAMGuide. The Guide assumes that your license file is in the OpenWorks
environment. When reading these procedures, substitute your VIP path(or wherever FLEXlm is installed) for the OpenWorks path.
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LAM 2003.0 Guide -- Linux and Unix
Introduction
This chapter describes LAM on Linux and UNIX platforms and
contains the following major topics:
• “Obtaining a Server License File” on page 31
• “Installing LAM Server” on page 34
• “Controlling the License Server” on page 38
• “LAM Technical Notes” on page 41
LAM System Requirements
Operating System
AIX 4.3.3, IRIX 6.5.11m, Red Hat Linux 7.2, Solaris 2.8.
Hardware Requirements
The memory, disk storage, and bandwidth needed for the LicenseServer is minimal when compared with the capability of modernworkstations, servers, and networks. For instance, as a base the
FLEXlm daemon, lmgrd, uses about 160 KB of memory, and the
Landmark daemon, licsrv, uses about 180 KB; however, with a largelicense file and with a large number of users, both daemons may use
about six megabytes of memory.
The storage requirements remain relatively static, around eight or nine
megabytes.
Obtaining a Server License File
Before you begin, check “LAM Technical Notes” on page 41.
A license file must be obtained from Landmark Graphics Corporation
before you can start the license server and run the VIP applications.
1. Log on to the server that will run LAM Release 2003.0.
2. Enter one of the following commands in a terminal window to
display the host ID of the system where the LAM server executes.
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The number can be a hexadecimal number or a decimal number. Ifthe number is decimal, a numeral or pound sign ( # ) must
immediately precede the decimal number.
AIX
FLEXlm uses the machine ID as the host ID. To retrieve the
machine name, use the uname command. For example:
uname -m
The command returns a twelve digit number. For instance:
000276513100
The first two and last two digits are always zeros. Strip away thefirst two and last two digits, and used the middle eight digits as the
host ID. For example:
02765131
IRIX
anw% /etc/sysinfo -s
The sysinfo command display information similar to thefollowing:
1762857767
In the example above, the number that sysinfo produces is adecimal number, 1762857767 . For the LAM server, the host IDmust be provided in the following form: #1762857767 . To convert
it to a hexadecimal number, use the following commands:
echo DecimalNumber 16o p | dc
HexadecimalNumber
Machine ID May Change With Operating System Changes
The identifier returned by uname may change after the software levels
of the AIX operating system are changed. This change may affect the
validity of your Landmark license.
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For example, using the number from sysinfo provided above, thecommand sequence would provide the following:
anw% echo 1762857767 16o p | dc
69131327
Linux
In Linux, the ID of an Ethernet interface (or adapter) is used as thehost ID of the system. Use the ifconfig command to find the ID of
the interface. For example:
/sbin/ifconfig Device
where Device is the name of the interface driver (such as eth for anEthernet interface) with its device number. For example, the first
Ethernet adapter in the computer would be eth0 .
The command will display the ID of the Ethernet interface as the
hardware class address (HWaddr). This address is composed oftwelve hexadecimal digits separated into pairs by colons. Forexample:
01:32:09:F6:A5:F5
For the LAM server, the host ID is the number without the colons.For example, given the address above, the following would be the
ID of the Ethernet interface:
013209F6A5F5
Solaris
highpoint% sysdef -h
The sysdef command display information similar to the following:
*
* Hostid
*
7233926c
In the example above, the number that sysdef produces is ahexadecimal number, 7233926c .
3. Write the Host Name here: _________________________
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To retrieve the host name from the system, enter the following in aterminal window:
uname -n
4. Request the license file from the following address:
http://www.lgc.com/support/licensing
Provide Landmark Licensing with the host ID and the host name
as well as the type of license, number of users for the license,machine manufacturer and model, and operating system name andversion.
5. Copy the license file to a folder on the machine where the licenseserver runs and is accessible by the license server.
Typically, the pathname for the license file is $OWHOME/lam/license.dat . If you give the name any other pathname, you must
include the path name as a parameter in the command that startsthe license server. For example:
$OWHOME/lam/bin/startlmgrd -c /export/home/license/license.dat
Or, you must assign the LM_LICENSE_FILE environmentvariable to the pathname. For example:
setenv LM_LICENSE_FILE $OWHOME/lam/license.dat
Installing LAM Server
The steps to install LAM server are contained in this section.
The following procedure should also be used if you must reinstall theLicense Manager files.
Use the following steps to install LAM server.
1. Log on as root.
2. If you are logged in remotely to the system where you areinstalling LAM, do the following:
• On the remote system, set the DISPLAY environment variable:
setenv DISPLAY LocalMachineName:0.ScreenNumber
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• On the local system, allow the remote system access to the localsystem:
xhost + RemoteMachineName
3. Run the Setup program. For example, you may enter the
following:
/cdrom/CDInstall/install/setup
The Release Manager for R2003 begins running in the terminalwindow and will prompt for the location of log files.
4. Enter y to accept the default, /tmp .
Or, enter n , and enter another path for the log files.
5. If the OWHOME environment variable has not been set, you will be prompted to enter its path. The path must be a complete
pathname, such as:
/d01/programs/OpenWorks
Release Manager displays the location of the OpenWorks home
directory (contained in OWHOME) and asks you to confirmwhether it is correct.
6. Enter y to accept the setting of OWHOME.
Or, if the location is not correct, enter n , and enter anotherlocation for the OpenWorks home directory.
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7. If the location does not exist, the Release Manager will ask you toallow it to create the directory or subdirectories that do not exist.
Enter n to re-enter the OpenWorks home path or to stop theinstallation process.
Or, enter y to allow the Release Manager to create directories. TheRelease Manager - Product Selection dialog opens, and the
Release Manager Release Notes dialog opens on top of theselection dialog. The Release Notes contain a list of the features ofOpenWorks 2003 and a list of the platforms on which it runs.
8. Click OK to close the dialog.
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The Release Manager - Product Selection dialog lists theLandmark products on the CD.
9. Select Install in the option menu for LAM.
10. Verify the installation location. If you need to change theinstallation location, click the Browse (!) button associated with
the product and navigate to the correct location.
11. Select Linux for the Linux operating system, SUNSV for theSolaris operating system, IRIX64 for the IRIX operating system,
or AIX for IBM’s AIX operating system, in the Target OS optionmenu.
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12. Click Start. The Product Installation Status dialog opens with theInstallation Status Window.
The Release Manager will display a series of status messages inthis dialog as it extracts the product.
After LAM installs, the Product Installation Status dialog indicates
its installation.
Next, the Product License Information dialog opens to remind you
to contact Landmark Graphics Corporation about the license foryour software.
13. Click OK in the Product License Information dialog.
14. Click OK in the Product Installation Status dialog.
15. Click Close in the Installation Status Window.
The Release Manager - Product Selection dialog redisplays,indicating that LAM has successfully installed.
16. Click Exit in the Release Manager - Product Selection dialog.
17. When prompted to confirming exiting CD Installer, click Yes.
A Warning dialog displays, asking you to determine whether tokeep the log files or not.
18. Click OK to delete the log files, or click Cancel to save the logfiles.
CD Installer stops running.
Controlling the License Server
After acquiring a license file for the software you have purchased, but before you use the software, you must start the license server. You can
start the license server manually, or you can configure the licenseserver to start when the system boots.
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Starting and Stopping the License Server
The system startup file on the license server is modified at installationtime to start up the license daemon. Use the following steps to start andstop the License Server.
1. To start the server manually, log in as root to the workstationcontaining the license server, change to the LAM bin directoryunder OpenWorks, and enter the startup command. For example:
telnet nova
login: root
setenv OWHOME /pa/OpenWorks (C Shell), or OWHOME=/pa/OpenWorks;export OWHOME (Bourne or Korn Shell)cd /pa/OpenWorks/lam/bin
./startlmgrd
2. To stop the License Server, use the same procedure as indicated inthe previous step, but substitute the following command:
./stoplmgrd
Setting the Environment Variable
The LM_LICENSE_FILE environment variable is an environmentvariable provided by the FLEXlm license server package. It performs
the following functions:
• Allows users to designate a license.dat file that the application will
use to attempt to check out a license
• Allows users to specify a list of license.dat files that the application
has available to use in checking out licenses.
LM_LICENSE_FILE has a syntax exactly like that of PATH. For
example, C shell users would use the following commands:
setenv LM_LICENSE_FILE $OWHOME/license1.dat
setenv LM_LICENSE_FILE $OWHOME/license1.dat:$OWHOME/license2.dat
Defining License Groups
A License Group is one or more workstations using a single LicenseSystem, including a license.dat file and one or more License Servers
(represented by SERVER lines in the license.dat file).
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Large sites may want to partition their workstations into distinctgroups. Each workstation group would have a License System
including:
• a license.dat file
• one or more workstations designated as License Servers.
The user defines LM_LICENSE_FILE to point to the license.dat filethat is to be used by applications running in the group.
Group License Sharing
Groups may “share” licenses with other groups through the use of the
LM_LICENSE_FILE environment variable:
• Each group has a copy of each license.dat file from the other groups(hopefully all named appropriately).
• The user environment contains the LM_LICENSE_FILE defining
the exact location of each of the above license.dat files. In addition,LM_LICENSE_FILE defines an order that the application will
follow when trying to check out a license from one of the groups.
Be aware of licenses common to one or more of the above license.dat
files and the problem associated with searching LM_LICENSE_FILE.An example of a LM_LICENSE_FILE variable setting for a group is
shown below:
setenv LM_LICENSE_FILE “/etc/license_g1.dat:/etc/license_g2.dat”
NOTE: Rollover in LAM version 2003.0 does not work properly. If a user runs out
of licenses in the license_gl,.dat file, LAM will not automatically rollover to
license_g2.dat.
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LAM Technical Notes
If Applications Cannot Find License File
As a default, License Application Manager (LAM) expects the license
file to have a pathname of $OWHOME/lam/license.dat .
Environment variables locating the license are normally set up by theinstallation program. The variable can contain either the full path to the
license file including the machine name on which it resides, or it cancontain the port number and machine name of the license server thatserves that license file. For example:
LM_LICENSE_FILE 2013@HostName
or
LM_LICENSE_FILE $OWHOME/lam/license.dat
FLEXlm performs background operations to speed-optimize access tothe license file when it is run from an application for the first time.
FLEXlm writes the path to the license file in either the user homedirectory or the root directory (depending on the platform andconfiguration) in a hidden file named .flexlmrc.
If it is necessary to change the location or name of the license file beingused, remove .flexlmrc in order to get FLEXlm to use the new license
file if the path has changed.
Overriding LM_LICENSE_FILE
Landmark generally makes use of the LM_LICENSE_FILEenvironment variable. Applications running for the first time mayincorrectly override the setting of the LM_LICENSE_FILE variable.
Set the environment variableFLEXLM_NO_CKOUT_INSTALL_LIC to 1.
Doing this will prevent the creation of $HOME/.flexlmrc. You shouldalso remove any existing $HOME/.flexlmrc to avoid overriding
LM_LICENSE_FILE.
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Restricting the Use of FLEXlm Utilities
The lmdown, lmremove, and lmreread utilities can be privileged,depending on the switches used when the lmgrd license server isstarted. When they are privileged, only a License Administrator can run
the utilities. A License Administrator is a member of the lmadmingroup, or if the lmadmin group does not exist, a License Administratoris a member of the group with ID 0.
To restrict who can run the utilities, lmgrd license server must bestarted with the -2 -p switch. For instance to start the server and restrict
the use of the utilities, you might enter the following:
$OWHOME/lam/bin/startlmgrd -c /export/home/license/license.dat -2 -p
If you want to disable the lmdown or lmremove utilities, so that even aLicense Administrator can not run them, the lmgrd license server can
be started with -x UtilityName . For example, you might enter one ofthe following commands:
$OWHOME/lam/bin/startlmgrd -c /export/home/license/license.dat -x lmdown
$OWHOME/lam/bin/startlmgrd -c /export/home/license/license.dat -x lmremove
$OWHOME/lam/bin/startlmgrd -c /export/home/license/license.dat -x lmdown -x lmremove
After disabling lmdown, you can only stop the lmgrd license serverwith the kill command, but you must not use the version of thecommand with the -9 switch.
For more information, see the FLEXlm documentation on theGLOBEtrotter Software website.
http://www.globetrotter.com/manual.htmContains the Table ofContents of the FLEXlm End User’s Guide.
http://www.globetrotter.com/IX.htm Contains the Index and a link todownload a PDF of the FLEXlm End User’s Guide.
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Setting the Environment
Setting the User’s Environment
The following should be done to set the user’s environment:
■ Create a user (if an appropriate user does not exist).
■ Set the default shell to csh (recommended).
Without OpenWorks
For users to submit simulation jobs from a Windows 2000 machine to a remote
UNIX or Linux machine, the location of the UNIX/Linux VIP installation and the
location of the License Manager must be known. This information is provided in
a .kviprc file that a user has in his home directory or the site administrator has
placed in /etc or /usr/local/etc directories. A template of this file is
located in the UNIX and Linux VIP installation and is found in the top VIP
directory.
If it is to be placed in the user’s home directory, make a copy of this file and
rename it to .kviprc (note the dot before the name). If the site administrator has
placed it in/etc or /usr/local/etc, the dot before the name is not required.
Edit the copied file and modify the location of the VIP UNIX or Linux installation
(VIPHOME) and the location of the License Manager’s license.dat file
(LM_LICENSE_FILE).
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Other Important Environment Variables
Simulator Selection Environment Variables - Default Executables
Starting DESKTOP-VIP for Windows 2000 will set the following simulator
default environment variables:
If a user chooses to use a different simulator, the particular simulator name can be
changed by setting the appropriate variable before starting DESKTOP-VIP. Or the
user can switch between simulator versions on the Job Submittal panel.
Note that the default simulator name version numbers are no longer different for
the Linux executables.
Variable Name Default Simulator Name Description Platform
VIPCOREDEF core2003r4.exe Defaulted name of VIP-CORE
executable
ALL
VIPEXECDEF exec2003r4.exe Defaulted name of VIP-EXEC
executable
ALL
VIPCORELOCALDEF pcore2003r4_local.exe Defaulted name of Parallel VIP-
CORE executable running local
IBM
VIPEXECLOCALDEF pexec2003r4_local.exe Defaulted name of Parallel VIP-
EXEC executable running local
IBM
VIPCOREDISTDEF pcore2003r4_dist.exe Defaulted name of Parallel VIP-
CORE executable running dis-
tributed
WINDOWS. SUN,
SGI, LINUX
VIPEXECDISTDEF pexec2003r4_dist.exe Defaulted name of Parallel VIP-
EXEC executable running dis-
tributed
WINDOWS. SUN,
SGI, LINUX
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If a user chooses to use a different simulator, he can change the particular
simulator name by setting one of the following environment variables in his
.krunvip file:
setenv VIPCOREDEF newcore.exe
setenv VIPEXECDEF newexec.exe
setenv VIPCORELOCALDEF newpcorelocal.exe
setenv VIPEXECLOCALDEF newpexeclocal.exe
setenv VIPCOREDISTDEF newpcoredist.exe
setenv VIPEXECDISTDEF newpexecdistexe
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Appendix A: Parallel Computing
Getting Started with PARALLEL-VIP
Setting up your system to run PARALLEL-VIP may require some changes to your basic system configuration. This section describes nomenclature and other
information to facilitate the installation.
Include File Configuration Requirements
Each possible parallel configuration has associated requirements for validinclude file locations and configuration requirements. Configurations andrequirements are detailed in the PDF document IncludeFileRules.pdf which can
be accessed from the Help menu (Help > Submit > Include Paths). Configurations are also provided in Excel spreadsheet format in the document BoulderSubmission.xls. Both documents can be found in
%VIPHOME%\doc\help.
Which Systems Will Parallel-VIP Run On?
PARALLEL-VIP will run on the following systems:
1. IBM SP workstations with a Power 2 architecture with or without a high
performance switch. This configuration is often referred to as a LOCAL
system. The IBM software POE and PSSP must be installed.
2. Shared Memory Silicon Graphics workstations (Power Challenge, Octane,
and Origin 2000). This configuration is often referred to as a
DISTRIBUTED system.
3. Shared memory SUN Solaris workstations. This configuration is often
referred to as a DISTRIBUTED system.
Parallel Computing Quick Guide
Refer to the Parallel Computing chapter of the Getting Started manual for a helpful
introduction to parallel computing.
Warning
Be sure to read the IncludeFileRules document carefully. This document provides a spreadsheetto help you find your configuration options and the setup rules that must be met.
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4. Linux Red Hat 7.2 cluster workstations. This configuration is often referred
to as a DISTRIBUTED system.
Where Should You Run From?
Running on IBM SP Workstations
A user can either:
1. Log in directly to one of the SP nodes and submit the run from the command
line.
2. Submit the run remotely from your Windows 2000 machine.
NOTE: IBM's Parallel Operating Environment (POE) must be running on the SP
system.
See “Appendix E: SP2 POE Checkout Guidelines” for SP POE checkout
guidelines and helpful hints.
Running on Shared Memory Silicon Graphics, Solaris, and Linux Worksta-
tions
A user can either:
1. Log onto the Silicon Graphics, Solaris, or Linux shared memory machine and
submit the run from the command line.
2. Submit the run remotely from your Windows 2000 Machine.
NOTE: MPI (Argonne N.L. Version 1.1) needs to be accessible from the submitting
machine. The code is provided with the Desktop-VIP installation.
File System Set Up
The directories containing the VIP installation and the VIP dataset need to be
cross-mounted with all the nodes that will be used to run the calculation. In
addition, the file systems where the VIP installation and the datasets to be runreside must each be mounted and accessible using the same full path name for all
the nodes.
For example, let’s assume that the VIP home directory ($VIPHOME) is located at
/mnt/vip on the first node. Then the same directory must be cross mounted and
named so it has the same full path name on all the remaining nodes. Any errors
you receive may not be very descriptive of the underlying problem if the file
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systems are not mounted correctly. Refer to Appendix B for NFS mounting
requirements.
NOTE: It is highly recommended that all user files are located on a local disk and
not on a NFS mounted disk. This will reduce and possibly eliminate NFS
read/write errors which could cause abnormal termination of runs and/or
corrupt data files. This is manditory for SGI, Solaris, and Linux Shared
Memory workstations.
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.rhosts File
You must be able to remotely log in to the nodes that will be used to run
PARALLEL-VIP without entering a password. This requires that you have a
.rhosts file in your home directory containing the names of all the nodes you want
to be able to access or that your administrator has modified the /etc/hosts file. A
sample .rhosts file is shown below.
Sample .rhosts file:
#
#ptype ibmsp IBM SP
#interface us User Space Comm. (us)
xyzsw1.lgc.com
xyzsw2.lgc.com
xyzsw3.lgc.com
xyzsw4.lgc.com
#interface ip Local IP Comm. (ip)
xyzen1.lgc.com
xyzen2.lgc.com xyzen3.lgc.com
xyzen4.lgc.com
xyz2en1.lgc.com
xyz2en2.lgc.com
xyz2en3.lgc.com
xyz2en4.lgc.com
#ptype sgishm SGI Shared Memory
sgi1.lgc.com
#ptype generic Generic Hosts
ibm1.lgc.com
ibm2.lgc.com
#ptype linux Linux Shared Memory
lin1.lgc.com
lin2.lgc.com #endptype
NOTE: The # is used to indicate comments which are not interpreted by the UNIX or
Linux operating systems.
The #ptype, #interface and #endptype keywords are recognized by the
PARALLEL-VIP job submission system and used to delimit the different
types of nodes available on the system.
The list of nodes and cpu's in the .rhosts file must contain the complete
domain name. In this example xyz2en1.lgc.com is a valid name, while
xyz2en1 is invalid.
Remote Shell Capabilities
A PARALLEL-VIP job submission uses the remote shell (rsh) capabilities of
UNIX and Linux. In developing the applications it has been assumed that a rsh
command will return only the command information. This means that all of the
nodes that can be accessed by PARALLEL-VIP cannot return extraneous echo
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commands in the .cshrc file. Consider the following two of .cshrc files. The first
one is valid, while the second one is invalid for running PARALLEL-VIP.
■ Sample of Valid .cshrc file:
#!/bin/csh
set path =($path .)
#
if ($?prompt) then
if (-e $LM_LICENSE_FILE) then
echo License File is present
else
echo License File is missing
endif
endif
■ Sample of Invalid .cshrc file:
#!/bin/csh
set path =($path .)
#if (-e $LM_LICENSE_FILE) then
echo License File is present
else
echo License File is missing
endif
The invalid file contains an echo command that is invoked anytime, while the
valid file performs a test to ensure that the echo command is performed only for
interactive sessions. Although this distinction is unnecessary for the serial version
of VIP it is very important here.
NOTE: The terms valid and invalid are used here only for the perspective ofwhether PARALLEL-VIP can be run; both these files are valid from aUNIX/Linux perspective.
Testing for Valid rsh Performance
The easiest way to test for valid rsh performance is to perform a simple rsh
command on all of the accessible nodes. For example, a remote shell to get the
date should return just the results of the date command. If anything else is
returned, then the .cshrc file is invalid and the PARALLEL-VIP job submission
scripts will not function correctly.
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For example, consider that you want to run PARALLEL-VIP on the node known
as vip2en1. Using a rsh command to determine the date with the Invalid .cshrc
file listed above will return the following:
% rsh vip2en1 date
License File is present
Thu Jun 12 13:09:22 CDT 1997
The presence of additional information beyond what is normally returned by
the date command indicates a problem!!
Using a rsh command to determine the date with the Valid .cshrc file listed above
will return the following:
% rsh xyz2en1 date
Thu Jun 12 13:09:22 CDT 1997
The lack of additional information beyond what is normally returned by the
date command indicates that the PARALLEL-VIP job submission should
work.
Other Notes
PARALLEL-VIP carries memory overhead which scales with the total number of
gridblocks in the simulation (NB). The program uses 2 extra arrays, each of
dimension NB, per processor. This overhead is quite minimal when running on a
distributed memory machine, but can become quite large when running on a
shared memory system.
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Appendix B: NFS Mounting Requirements for Parallel or Remote Submission
In order for Parallel or Remote Job submission to be fully functional, it is required
that:
1. For any given directory path, there should be at least one common directory
path name for ALL the nodes;
2. There is a consistent way to generate this common directory path name on
ANY of the nodes.
We can satisfy these two requirements in two different ways: 1) Manual mounts
and 2) Automounter:
The following sections describe the restrictions for each methods.
Manual Mounts
It is necessary that the result of /bin/pwd on ALL of the nodes/machines is a
common directory path name.
Assumptions
Machine Alpha - Contains physical disks mounted as filesystems:
/u1 and /u2.
- These filesystems are exported to other
machines as:/u1 and /u2
Machine Beta - Mounts the filesystems as /u1 and /u2 using the
commands:
mount Alpha:/u1 /u1
mount Alpha:/u2 /u2
Tests
1. A user logs onto Alpha. At the prompts, Alpha%, he types in:
Alpha% cd /u1/some/sub/directoryAlpha% /bin/pwd
He would see the following on his screen:
/u1/some/sub/directory
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2. A user logs onto Beta. At the prompts, Beta%, he types in :
Beta% cd /u1/some/sub/directory
Beta% /bin/pwd
He would see the following on his screen:
/u1/some/sub/directory
WARNING: There is a common practice that NFS mounted filesystems will look the
same; i.e., /bin/pwd would generate a common path name for all NFSclients. The exception to this practice is on NFS servers, where symbolic
links (i.e. "ln -s") are used to access common path names. There is no
consistent way to generate a common path name from the result of /bin/pwd on NFS servers; e.g., /bin/pwd would report /arbitrary/path/name, to which a symlink /common/path/name is pointed. There is noconsistent way to derive a /common/path/name from a /arbitrary/path/name except for ugly hacks. Hence Requirement 2 above would not be satisfied. On such systems DTOP submissions will still work as long as
NFS servers are not among the simulation nodes/machines.
Automount Mounts
Automount (assuming all the involved filesystems are exported), such that;
1. For NFS servers, /bin/pwd would report a /arbitrary/path/name, from
which a common path name /net/node/arbitrary/path/name can be derived.
NFS servers are the machines where the filesystems are mounted locally.
2. For NFS clients, /bin/pwd would report either a /common/path/name (for
recent autofs configurations) or /tmp_mnt/common/path/name (for vanilla
automounter), from which a common path name/common/path/name can be derived. For the vanilla automounter, NFS
clients would report either:
a. /tmp_mnt/net/machine/common/path/name
b. /tmp_mnt/home/machine/userID/common/path/name
Assumptions
Machine Alpha - Contains physical disks mounted as filesytems
/u1 and /u2These filesystems are exported to the world.
Machine Beta - Automounter has mounted the filesystems
/u1 and /u2
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Limitation:
1. DESKTOP-VIP does not support command line options for automount
daemon that override auto.master.
In order for DESKTOP-VIP to work, the customer’s site must have an /dir to -
hosts map entry in auto.master. Typical entry maps hosts to -hosts. Customizeddirectory names are permitted; typical directory names include /net, /nfs, /remote,
etc.
Rules
1. If VIPNFSAUTO is set to "no", "NO", or "0", then the path normalization for
automounter is disabled.
2. If VIPNFSAUTO is set to any other values from "no", "NO", or "0", then the
path normalization for automounter is enabled.
3. If VIPNFSAUTO is not set, DESKTOP-VIP will attempt to determinewhether automount is running by lo