CODEMARK: nice-ibr
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CODEMARK: end
Internet background radiation (IBR) are packets gathered from dark (unpopulated) networks, which are known in the IBR community as telescopes.
This software contains tools to help gather and analyze IPv4 IBR packets.
This file documents how to build and prepare to use the IBR tools, how to build and install them in your local directory, and guidance about how to configure the tools to use on your system with your own data.
Many of these tools are designed to take their parameters from parameter
files that define things like the path to the input pcap or CSV files,
and where to store the output. You will need to create parameter files
for your local setup before you use most of the analysis tools. For
more information about the parameter files, look in the ./params
directory and read the documentation in the example parameter files.
For information about the tools for preprocessing pcap files and doing
some analyses on them, and the general workflow of analyzing pcap files,
look at the README in the ./tools
directory. This directory contains
tools to capture pcaps, pre-process them into formats used by the rest
of the tools, and perform some analyses.
For examples of quick-look analyses, look at the README and COOKBOOK
files in the ./firecracker
directory.
These tools were developed and tested on Ubuntu 20.04 and Ubuntu 22.04. Some are known to work correctly on other platforms (or in some cases, they may be easily ported), but these are the only platforms for which we have tested all of the tools.
Some of the tools use libraries or tools that are Linux-specific, and will not work on non-Linux platforms without additional engineering.
Run the setup-sysadmin.sh
script in this directory. Note that this
script requires sudo
permissions (including permission to install
software) to run some of its commands. This script will install
software used to build and run the IBR tools.
Run the setup.sh
script in this directory. The setup script will
build the executables that are part of this package, and install them
in the bin
subdirectory of this directory. Note that this
will fail if the required packages have not already been installed
(usually accomplished using setup-sysadmin.sh
).
Many of the scripts read their parameters from parameter files, and these parameter files must be created and edited before the scripts will work correctly.
The top-level parameter files defines the paths to the input and output directories, and some related paths. If you have more than one IBR telescope (or other data source), then you will need to have different parameter files for each telescope, in order to avoid overwriting the output files from one telescope with those for another.
A template for the top-level parameter file is given in
params/example.params
.
A key parameter in the top-level parameter file is DATANAME. This variable is used to define other values, and MUST be unique for each different telescope or data source. (if it is not unique, you risk having the analysis files from different telescopes overwrite each other)
The names of two of the other parameter files are defined by DATANAME.
These parameter files list the allowed destinations (the addresses
within the telescope) and omitted sources (any sources that are ignored
by the analysis steps). These are located in the params
directory,
and examples are given in params/example-allowed-dsts.dat
and
params/example-omitted-srcs.dat
.
To begin to capture and analyze data, consult the README file in
./tools
, and the README and COOKBOOK files in ./firecracker
.