This Source.zip has three application code folders containing .java and .class files and two .jar files as follows:
1. desktop-side_JXTA4JMS
2. mobile-side_JXTA4JMS
3. JMS Test Client
4. Listener.jar
5. JMSTestClient.jar
We now explain execution steps, we followed, to run this JXTA4JMS application.
Before we try we require Application softwares and need to configure JXTA relay and J2EE server.
This package consists of the executable (UCW), a default script file,
this file, and the library files. It is important that the header files
end up in a include subdirectory of the directory where UCW is found.
If you unzip this file using its path information ( use folder names ) this will
automatically happen. You can optionally specify the UnderC directory
with the environment variable UC_HOME note that this points to the directory
containing ucw.exe. If you do this, then you can copy the executable anywhere
and it will still be able to find the header files.
In this paper, a new family of Cassinian wave-guides
is proposed, simulating and calculation are finished with CST
Microwave Studio that based on Finite Integral Technique (FIT),
and some results are given. Electromagnetic field mode type of it
is TE, electromagnetic field is stronger near neck region, and
some resonance frequencies appear. The new Cassinian curve
wave-guides will possess higher power than ones of the
rectangular and elliptic wave-guides because the height at the
position where maximal electric field occurs is smaller.
jobo, famous crawler open source which is implemented by java.
used in many big websites.
You will need a Java Runtime Environment 1.3 or later (on many
System Java 1.2 is installed, it will NOT work !).