The Global Meteor Network - Methodology and first results

The Global Meteor Network (GMN) utilizes highly sensitive low-cost CMOS video cameras which run open-source meteor detection software on Raspberry Pi computers. Currently, over 450 GMN cameras in 30 countries are deployed. The main goal of the network is to provide long-term characterization of the radiants, flux, and size distribution of annual meteor showers and outbursts in the optical meteor mass range. The rapid 24-h publication cycle the orbital data will enhance the public situational awareness of the near-Earth meteoroid environment. The GMN also aims to increase the number of instrumentally observed meteorite falls and the transparency of data reduction methods. A novel astrometry calibration method is presented which allows decoupling of the camera pointing from the distortion, and is used for frequent pointing calibrations through the night. Using wide-field cameras (88 degrees x 48 degrees) with a limiting stellar magnitude of +6.0 +/- 0.5 at 25 frames per second, over 220000 precise meteoroid orbits were collected since 2018 December until 2021 June. The median radiant precision of all computed trajectories is 0.47 degrees, 0.32 degrees for of meteors which were observed from 4 + stations, a precision sufficient to measure physical dispersions of meteor showers. All non-daytime annual established meteor showers were observed during that time, including five outbursts. An analysis of a meteorite-dropping fireball is presented which showed visible wake, fragmentation details, and several discernible fragments. It had spatial trajectory fit errors of only similar to 40m, which translated into the estimated radiant and velocity errors of 3 arcmin and tens of meters per second.

Automated summary

The Global Meteor Network (GMN) uses low-cost CMOS video cameras and Raspberry Pi computers for meteor detection, aiming to provide long-term characterization data on meteor showers and outbursts. The network also focuses on increasing observed meteorite falls and data transparency, presenting a novel astrometry calibration method. With wide-field cameras, over 220,000 precise meteoroid orbits have been collected, along with an analysis of a meteorite-dropping fireball.