Live observations
RMOB Data

RMOB Archives

Search Engine

RMOB Tools

Excel

Formula

Set Up

Software

NewsLetter
To receive news about this website, consider subscribing to our Newsletter.
Subscribe
Unsubscribe
133 Subscribers
Visites

   visitors

   visitors online

Webmaster - Infos
downloadDownload
If you find a broken link in this list, please report it to the webmaster.

Close Free Software GNU GPL

Bolidozor

Bolide observation network using radio and visual measuring station systems.

on GitHub
 


bolidozor(??? Kb)Downloaded 408 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

Then run software.



colorlabv3.zip(705.40 Kb)Downloaded 264 timesDownload

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

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 398 timesDownload

HROFFT audio spectrum software dedicated to meteor detection



HROFFT100f.zip(??? Kb)Downloaded 1971 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 1155 timesDownload

Close RMOB Tools

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

Please see explanations here !

rmobxls.zip(??? Kb)Downloaded 3206 timesDownload


rmob_survey_year_2005.zip(??? Kb)Downloaded 2617 timesDownload


rmob_survey_year_2006.zip(??? Kb)Downloaded 2530 timesDownload


rmob_survey_year_2000.zip(??? Kb)Downloaded 2544 timesDownload


rmob_survey_year_2001.zip(??? Kb)Downloaded 2494 timesDownload


rmob_survey_year_2002.zip(??? Kb)Downloaded 2532 timesDownload


rmob_survey_year_2003.zip(??? Kb)Downloaded 2573 timesDownload


rmob_survey_year_2004.zip(??? Kb)Downloaded 2465 timesDownload


rmob_survey_year_2007.zip(??? Kb)Downloaded 2211 timesDownload


rmob_survey_year_2008.zip(??? Kb)Downloaded 2293 timesDownload


rmob_survey_year_2009.zip(??? Kb)Downloaded 2520 timesDownload


rmob_survey_year_2010.zip(517.94 Kb)Downloaded 1857 timesDownload


rmob_survey_year_2011.zip(551.07 Kb)Downloaded 1891 timesDownload


rmob_survey_year_2012.zip(677.38 Kb)Downloaded 1515 timesDownload


rmob_survey_year_2013.zip(817.90 Kb)Downloaded 947 timesDownload


rmob_survey_year_2014.zip(807.61 Kb)Downloaded 515 timesDownload


rmob_survey_year_2015.zip(768.83 Kb)Downloaded 138 timesDownload

RMOB survey free Windows® software (860 Ko)

rmob_survey_v11.zip(??? Kb)Downloaded 3221 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 967 timesDownload