The spectra of 25 meteors, recorded with an image orthicon technique in December 1969, are studied in relation to similar records made in August of the same year. Of 19 Geminid meteors in the absolute visual magnitude range 0 to +2, only one showed any evidence of the forbidden line of oxygen at 5577 A, while all Perseid meteors recorded in August exhibited the oxygen line, a result of the large difference in geocentric velocity between the two showers. Atoms identified in faint Geminid meteors include neutral iron, magnesium, calcium and sodium. The molecular bands of nitrogen are also observed
The ECOMA (Existence of Charge state Of meteoric smoke particles in the Middle Atmosphere) sounding ...
The capabilities of the radiometeor method of wind measurement increase with the increase of the tra...
Abstract: Every night we experience the celestial phenomenon of meteors falling to Earth. Meteors ar...
Spectral observations of meteors have been carried out for several years using an optical electronic...
This paper shows the first result of a Geminid meteor spectrum in the visible–ultraviolet region. W...
The fluxes and ZHRs from the 2012 Geminid meteor shower as seen in NASA's Meteoroid Environment Offi...
Studies on meteor spectroscopy are reported. The following topics are discussed: photometric spectra...
Asteroid (3200) Phaeton is the par- ent body of the Geminid meteoroid stream. These par- ticles gi...
A Geminid fireball with an absolute magnitude of -13 was observed over the south of Spain on 2009 De...
In the early morning hours of December 13, 2002, a bright Geminid fireball with an absolute magnitud...
The Geminid meteor shower was observed in 2015 using the Western Meteor Physics Groups Canadian Mete...
The three-station Canadian Meteor Orbit Radar (CMOR) is used here to examine the Geminid meteor show...
Low light level television systems offer the ability to observe meteors as faint as 10th magnitude w...
Aims. We present a library of low-resolution meteor spectra that includes sporadic meteors...
Preliminary data required to extrapolate available meteor physics information (obtained in the photo...
The ECOMA (Existence of Charge state Of meteoric smoke particles in the Middle Atmosphere) sounding ...
The capabilities of the radiometeor method of wind measurement increase with the increase of the tra...
Abstract: Every night we experience the celestial phenomenon of meteors falling to Earth. Meteors ar...
Spectral observations of meteors have been carried out for several years using an optical electronic...
This paper shows the first result of a Geminid meteor spectrum in the visible–ultraviolet region. W...
The fluxes and ZHRs from the 2012 Geminid meteor shower as seen in NASA's Meteoroid Environment Offi...
Studies on meteor spectroscopy are reported. The following topics are discussed: photometric spectra...
Asteroid (3200) Phaeton is the par- ent body of the Geminid meteoroid stream. These par- ticles gi...
A Geminid fireball with an absolute magnitude of -13 was observed over the south of Spain on 2009 De...
In the early morning hours of December 13, 2002, a bright Geminid fireball with an absolute magnitud...
The Geminid meteor shower was observed in 2015 using the Western Meteor Physics Groups Canadian Mete...
The three-station Canadian Meteor Orbit Radar (CMOR) is used here to examine the Geminid meteor show...
Low light level television systems offer the ability to observe meteors as faint as 10th magnitude w...
Aims. We present a library of low-resolution meteor spectra that includes sporadic meteors...
Preliminary data required to extrapolate available meteor physics information (obtained in the photo...
The ECOMA (Existence of Charge state Of meteoric smoke particles in the Middle Atmosphere) sounding ...
The capabilities of the radiometeor method of wind measurement increase with the increase of the tra...
Abstract: Every night we experience the celestial phenomenon of meteors falling to Earth. Meteors ar...