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Close Free Software GNU GPL

Bolidozor

Bolide observation network using radio and visual measuring station systems.

on GitHub
 


bolidozor(??? Kb)Downloaded 2502 timesDownload

Close Free Windows® Software

Colorgramme Lab v 3.0 (EXE only)  for previous version user.
Unzip colorlab.exe file and curl.exe file then copy these 2 files in the Colorgramme Lab directory   ( c:/program files/colorgramme lab/ )  by default

WARNING ! under Windows 64 bit like Windows 10 run Colorgramme in 32 bit emulator, if not data transfert dosn't work !

Then run software.


colorlabv3.zip(705.40 Kb)Downloaded 2257 timesDownload

Colorgramme Lab v 3.0   Full version with INSTALL setup
Unzip file and run setup

WARNING ! under Windows 64 bit like Windows 10 run Colorgramme in 32 bit emulator, if not data transfert dosn't work !

Follow instruction then run software from program panel.

This version include HROFFT executable file un hrofft subdirectory of Colorgramme lab

setup_colorgramme_lab_v3.zip(996.03 Kb)Downloaded 3100 timesDownload

HROFFT audio spectrum software dedicated to meteor detection



HROFFT100f.zip(??? Kb)Downloaded 4246 timesDownload

RaMAP v 1.7  is a free cross plateform software writen under java by Esteban Holgado N.

Radio Meteor Activity Projection
--------------------------------

The Radio Meteor Observation Bulletin (RMOB) web site (www.rmob.org) collects information on Radio Meteor Reflection
counts that have been registered by several observers around the world.

This information is recorded in RMOB Survey files, which is a time based format. The sample data content is composed
by a matrix of hours versus days. A meteor reflection count for every UTC hour of every day in a month is provided.

The RMOB File contains observer's related information, as latitude and longitude. With the UTC time, the date and the
Longitude information of the observer, it is possible to calculate the Julian Day (Julian Day calculation from Jean
Meeus, (1991), Astronomical Algorithms and the Local Sideral Time (LST) (Local Sideral Time calculation from Simon
Newcomb Sideral Time formula) of the observer at the UTC hour of the count, and consequently, the Right Ascension (RA)
of the local meridian of the observer at that time. The declination is directly obtained from the Observer's Latitude.

The observer's count for every UTC hour is normalized using the own observer's average figure calculated over a complete
month of data. With the RA and Dec calculated as indicated before, we have the observer's zenit at the UTC time of every
count (in fact, the zenit is calculated based on UTC + 30 minutes, to have a centered representation for every UTC hour).
Once the zenit is in this way located, a square of 15º by 15º of Sky Region, centered at that zenit, is coloured based on
the normalized count.

The contribution of all observers is then averaged providing a final picture with a spatial granularity of 5º by 5º of
Sky Region. In summary, the Radio Meteor Activity Projection program produces a couloured representation of the Meteor
Activity Projection over a Star Chart" or "SkyMAP", assigning a colour, which is directly proportional to the average
of the normalized contribution of all observers counts.

 Copyleft (c) - 2014 - Esteban Holgado N.         Gran Canaria  -  Spain

RaMAP_Ver17.zip(195.17 Kb)Downloaded 2910 timesDownload

Close RMOB Tools

To build an RMOB standard file with Excel (16 Ko)

Please see explanations here !

rmobxls.zip(??? Kb)Downloaded 4971 timesDownload


rmob_survey_year_2005.zip(??? Kb)Downloaded 4434 timesDownload


rmob_survey_year_2006.zip(??? Kb)Downloaded 4296 timesDownload


rmob_survey_year_2000.zip(??? Kb)Downloaded 3955 timesDownload


rmob_survey_year_2001.zip(??? Kb)Downloaded 4089 timesDownload


rmob_survey_year_2002.zip(??? Kb)Downloaded 4207 timesDownload


rmob_survey_year_2003.zip(??? Kb)Downloaded 4211 timesDownload


rmob_survey_year_2004.zip(??? Kb)Downloaded 4031 timesDownload


rmob_survey_year_2007.zip(??? Kb)Downloaded 3872 timesDownload


rmob_survey_year_2008.zip(??? Kb)Downloaded 3929 timesDownload


rmob_survey_year_2009.zip(??? Kb)Downloaded 4199 timesDownload


rmob_survey_year_2010.zip(517.94 Kb)Downloaded 3453 timesDownload


rmob_survey_year_2011.zip(551.07 Kb)Downloaded 3192 timesDownload


rmob_survey_year_2012.zip(677.38 Kb)Downloaded 2970 timesDownload


rmob_survey_year_2013.zip(817.90 Kb)Downloaded 2444 timesDownload


rmob_survey_year_2014.zip(807.61 Kb)Downloaded 2089 timesDownload


rmob_survey_year_2015.zip(768.83 Kb)Downloaded 2107 timesDownload


rmob_survey_year_2016.zip(835.60 Kb)Downloaded 181 timesDownload


rmob_survey_year_2017.zip(900.60 Kb)Downloaded 218 timesDownload


rmob_survey_year_2018.zip(826.61 Kb)Downloaded 193 timesDownload

RMOB survey free Windows® software (860 Ko)

rmob_survey_v11.zip(??? Kb)Downloaded 5092 timesDownload

RaMAP v 1.7  is a free cross plateform software writen under java by Esteban Holgado N.

Radio Meteor Activity Projection
--------------------------------

The Radio Meteor Observation Bulletin (RMOB) web site (www.rmob.org) collects information on Radio Meteor Reflection
counts that have been registered by several observers around the world.

This information is recorded in RMOB Survey files, which is a time based format. The sample data content is composed
by a matrix of hours versus days. A meteor reflection count for every UTC hour of every day in a month is provided.

The RMOB File contains observer's related information, as latitude and longitude. With the UTC time, the date and the
Longitude information of the observer, it is possible to calculate the Julian Day (Julian Day calculation from Jean
Meeus, (1991), Astronomical Algorithms and the Local Sideral Time (LST) (Local Sideral Time calculation from Simon
Newcomb Sideral Time formula) of the observer at the UTC hour of the count, and consequently, the Right Ascension (RA)
of the local meridian of the observer at that time. The declination is directly obtained from the Observer's Latitude.

The observer's count for every UTC hour is normalized using the own observer's average figure calculated over a complete
month of data. With the RA and Dec calculated as indicated before, we have the observer's zenit at the UTC time of every
count (in fact, the zenit is calculated based on UTC + 30 minutes, to have a centered representation for every UTC hour).
Once the zenit is in this way located, a square of 15º by 15º of Sky Region, centered at that zenit, is coloured based on
the normalized count.

The contribution of all observers is then averaged providing a final picture with a spatial granularity of 5º by 5º of
Sky Region. In summary, the Radio Meteor Activity Projection program produces a couloured representation of the Meteor
Activity Projection over a Star Chart" or "SkyMAP", assigning a colour, which is directly proportional to the average
of the normalized contribution of all observers counts.

 Copyleft (c) - 2014 - Esteban Holgado N.         Gran Canaria  -  Spain

RaMAP_Ver17.zip(195.17 Kb)Downloaded 2519 timesDownload