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====== Methods of data processing used in Bolidozor networkr ======

This site contains several designs of algorithms used for data processing.

* Estimate of an vector of meteor in the atmosphere
  * Record of available meteorological data for future reconstructions (satellite images, ČHMÚ measurements at a particular time, radar images)
  * Data collections from individual stations
  * Calculations of vector and vertical wind profile (?? Výšový profil větru)

There are some already existing projects that can used in the process of data processing.

* [[http://boinc.berkeley.edu/|BOINC]]
  * [[http://gnuradio.org/redmine/projects/gnuradio/wiki|GNU Radio]]
  * [[http://sourceforge.net/projects/cutesdr/|CuteSDR]]

===== Calculation of meteor trail parameters  =====

There already exists a network dealing with similar problem called [[http://meteor.uwo.ca/research/radar/cmor_intro.html|CMOR]], which observes meteors using transmitter and several receiver stations. Such approach is, however, not really suitable for Bolidozor network.

The most realistic solution seems to be a calculations using spatial coordinates of meteor’s head-echo. This approach has already been tested
[[http://ea4eoz.blogspot.cz/2016/04/determining-radiant-of-meteor-using_10.html|Miguel A. Vallejo, EA4EOZ]]

==== Data from GRAVES radar ====

|TR| ≈ 700 km
  60 km < b < 100 km
  |TM| + |MR| = Rb
  Rb(tM)´ = 0

=== Meteor detection ===

Currently, meteors are detected by comparing the signal intensity in area, where we expect the radio reflection with the signal intensity in area with frequency shift against the transmitted signal.

==== VOR transmitters ====

Aircraft navigation [[en:vor|VOR]] transmitters are one of the options, how to see the radio reflections.

=== Signal model ===

To calculate the energy balance, Jakub Kákona has created a [[http://nbviewer.ipython.org/github/kaklik/iPython-models/blob/master/VOR_beacons.ipynb|model of signal]].

=== Collecting the data ===

When processing data from VOR beacons, it is necessary to solve a problem of lower radiated power of transmitter. Lower transmitter power causes that the intensity of received signals is often below the noise level.

* Signal detection above the noise level by at least one station
  * Sending a control network packet with a request for data containing the suspicious part from the nearest stations. [[http://www.ros.org/about-ros/|Possiblity of using ROS]].
  * Correlation of detected signal with noise on other stations. 
  * As a result of the calculation the corresponding signal should be found in noise on other stations.
  * A detection will be confirmed if the meteor will be detected on several stations at the same time.
  * Otherwise, the event will be evaluated as false detection.

In case of positive detection, model parameters to calculate the replica have to be extracted from the signal.

Calculation of path will be carried out using several methods. First is the [[https://en.wikipedia.org/wiki/Multilateration|multilateration]] based on different records’ time shifts on individual stations. Time shifts has to be obtained by time correlations of recorded data. This correlation can be carried out either in signal time-space or using Fourier transformations (?? Fourierov obraz).

Next step is a measurement of doppler parameters of meteor’s head-echo, which determines the inclination and speed of the path.

Overall, the path calculation implementation will be carried out in two steps:

- Calculation of meteor position with respect to individual stations (can be done using the reflection from meteor trail).
  - Calculation of path vector in absolute coordinates.

==== Data from DVB-T ====

DVB-T signal has an advantage compared to VOR beacons in that it is broadband. This feature can help to improve the accuracy of measurement. However, the system transmits in multiplexes, meaning that there is a transmission of an identical signal from several places at once - causing a complication.

=== Decesion process and search for fragments ===

Should a scripting language be used to describe the [[http://www.ros.org/wiki/|ROS]] process?

* Command assignment to individual stations.
  * Start re-planing due to unsuccessful launch (??vypuštení) or rejection from station. 
  * Control of a potential violation of airspace and prohibited zones.

==== Multichannel detector from GnuRadio ====

A Marcus Leech group, Science Radio Laboratories has prepared a signal schema for GnuRadio that enables a [[http://www.sbrac.org/files/meteor_forward_scatter.pdf|processing of more channels at once]].

===== Optimising algorithms =====

* [[https://en.wikipedia.org/wiki/Particle_swarm_optimization|Particle swarm]]
  * https://pypi.python.org/pypi/cma

====== Tools for algorithms testing ======

===== Interactive scientific tool Jupyter =====
 
A good solution for testing is an interactive iPython environment where you can directly try individual parts of code and process data.

Its basic installation in Ubuntu can be carried out by installing the following packages:
  sudo apt-get install ipython-notebook python-scipy python-numpy

Afterwards, you can run iPython from the command line:
  ipython notebook --pylab inline

In order to get acquainted with [[http://www.tutorialspoint.com/python/|Python]] language you can use [[https://www.codecademy.com/learn/python|Codeacademy]].

==== Existing iPython scripts ====

There are several already existing iPython notebooks for data processing from Bolidozor network - you can find them at:
http://meteor1.astrozor.cz:8080/ 
More specifically for example [[http://meteor1.astrozor.cz:8080/ntbk/pub/radio-processing/iPython/iDHProcessor.html|Histogram of frequency shift of meteors]] and [[http://meteor1.astrozor.cz:8080/ntbk/pub/trails-processing/interactive_meteors.html|Visualisation of meteor trails]] from [[cs:meteor-observer|Meteor Observer Mobile aplication]].

(?? dáta) Data on server are reloaded every 5 minutes with [[https://github.com/paulgb/runipy|runipy]] programme.

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