Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly different regimes: a dense and transient plasma region co-moving with the ablating meteoroid and a trail of diffusing plasma left in the atmosphere and moving with the neutral wind. Interferometric radar systems are used to observe the meteor trails and determine their positions and drift velocities. Depending on the spatial configuration of the receiving antennas and their individual gain patterns, the voltage response can be the same for several different plane wave directions of arrival (DOAs), thereby making it impossible to determine the correct direction. A low signal-to-noise ratio (SNR) can create the same effect probabilistically even if the syst...
During the flight of a meteoroid through the neutral atmosphere, the high kinetic energy is suffici...
We have developed an automated analysis scheme for meteor head echo observations by the 46.5 MHz Mid...
Understanding the global meteor flux at Earth requires the measurement of meteor velocities. While s...
Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly different reg...
Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly different reg...
Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly different reg...
Abstract Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly dif...
Meteors and hard targets produce coherent radar echoes. If measured with an interferometric radar sy...
Meteors and hard targets produce coherent radar echoes. If measured with an interferometric radar sy...
Non-specular meteor trail echoes are radar reflections from plasma instabilities that are caused by ...
This dissertation presents details of new techniques in specular meteor radar data acquisition, mode...
This paper is concerned with short lived (<2 s) meteor trails which produced VHF radar echoes, sp...
[1] Radar data of non-specular meteor trails shows two clear and consistent features: (1) non–specul...
We have developed an automated analysis scheme for meteor head echo observations by the 46.5 MHz Mid...
We have developed an automated analysis scheme for meteor head echo observations by the 46.5 MHz Mid...
During the flight of a meteoroid through the neutral atmosphere, the high kinetic energy is suffici...
We have developed an automated analysis scheme for meteor head echo observations by the 46.5 MHz Mid...
Understanding the global meteor flux at Earth requires the measurement of meteor velocities. While s...
Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly different reg...
Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly different reg...
Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly different reg...
Abstract Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly dif...
Meteors and hard targets produce coherent radar echoes. If measured with an interferometric radar sy...
Meteors and hard targets produce coherent radar echoes. If measured with an interferometric radar sy...
Non-specular meteor trail echoes are radar reflections from plasma instabilities that are caused by ...
This dissertation presents details of new techniques in specular meteor radar data acquisition, mode...
This paper is concerned with short lived (<2 s) meteor trails which produced VHF radar echoes, sp...
[1] Radar data of non-specular meteor trails shows two clear and consistent features: (1) non–specul...
We have developed an automated analysis scheme for meteor head echo observations by the 46.5 MHz Mid...
We have developed an automated analysis scheme for meteor head echo observations by the 46.5 MHz Mid...
During the flight of a meteoroid through the neutral atmosphere, the high kinetic energy is suffici...
We have developed an automated analysis scheme for meteor head echo observations by the 46.5 MHz Mid...
Understanding the global meteor flux at Earth requires the measurement of meteor velocities. While s...