Add to ORKGThe fluxes and ZHRs from the 2012 Geminid meteor shower as seen in NASA's Meteoroid Environment Office's wide-field meteor cameras are presented, as well as meteoroid densities as found using the meteor's light curve and deceleration
We developed a parametric model of the spatial distribution of sporadic meteoroids by taking their p...
This paper outlines new methods to measure optical meteor fluxes for showers and sporadic sources. M...
Meteor showers and their outbursts are the dominant source of meteoroid impact risk to spacecraft on...
Asteroid (3200) Phaeton is the par- ent body of the Geminid meteoroid stream. These par- ticles gi...
We have optically recorded faint meteors using a large aperture LLLTV (low light level television) s...
The Geminid meteor shower was observed in 2015 using the Western Meteor Physics Groups Canadian Mete...
110-121 The meteoroid disintegration mechanism is a subject of interest as they are the sources fo...
A Geminid fireball with an absolute magnitude of -13 was observed over the south of Spain on 2009 De...
Most meteor showers will display typical activity levels in 2017. Perseid activity is expected to be...
NASA's Meteoroid Environment Office (MEO) is charged with monitoring the meteoroid environment in ne...
NASA's Meteoroid Environment Office (MEO) recently established two wide-field cameras to detect mete...
The orbit and radiant of the Geminid meteoroid stream based on an analysis of the current version of...
By using an array of high-sensitivity CCD video devices and spectrographs, the activity of meteor e...
Meteoroids are known to pose a threat to spacecraft; they can puncture components, disturb spacecraf...
The three-station Canadian Meteor Orbit Radar (CMOR) is used here to examine the Geminid meteor show...
We developed a parametric model of the spatial distribution of sporadic meteoroids by taking their p...
This paper outlines new methods to measure optical meteor fluxes for showers and sporadic sources. M...
Meteor showers and their outbursts are the dominant source of meteoroid impact risk to spacecraft on...
Asteroid (3200) Phaeton is the par- ent body of the Geminid meteoroid stream. These par- ticles gi...
We have optically recorded faint meteors using a large aperture LLLTV (low light level television) s...
The Geminid meteor shower was observed in 2015 using the Western Meteor Physics Groups Canadian Mete...
110-121 The meteoroid disintegration mechanism is a subject of interest as they are the sources fo...
A Geminid fireball with an absolute magnitude of -13 was observed over the south of Spain on 2009 De...
Most meteor showers will display typical activity levels in 2017. Perseid activity is expected to be...
NASA's Meteoroid Environment Office (MEO) is charged with monitoring the meteoroid environment in ne...
NASA's Meteoroid Environment Office (MEO) recently established two wide-field cameras to detect mete...
The orbit and radiant of the Geminid meteoroid stream based on an analysis of the current version of...
By using an array of high-sensitivity CCD video devices and spectrographs, the activity of meteor e...
Meteoroids are known to pose a threat to spacecraft; they can puncture components, disturb spacecraf...
The three-station Canadian Meteor Orbit Radar (CMOR) is used here to examine the Geminid meteor show...
We developed a parametric model of the spatial distribution of sporadic meteoroids by taking their p...
This paper outlines new methods to measure optical meteor fluxes for showers and sporadic sources. M...
Meteor showers and their outbursts are the dominant source of meteoroid impact risk to spacecraft on...