359 precisely reduced meteor orbits are presented that are the result of the Dutch Meteor Society's Photographic Meteor Survey in the period 1981 until 1993. Orbits include those of major and minor showers, doubling the number of known precise orbits of some meteor streams. From the spread in solutions of all possible sets of two photographic stations, we derive the measurement uncertainties from which we are able to calculate the intrinsic scatter in the Perseid meteor stream. The new Geminid orbits are compared to those obtained in similar surveys in the 1950's. This first measurement of the rate of change of Geminid orbits over time agrees well with model predictions
Sufficient observations exist of the returns of comet 55P!fempel-Tuttle in 1865 and 1965 for accurat...
All-sky Meteor Orbit System (AMOS) is a semi-autonomous video observatory for detection of transient...
Visual meteor observations are carried out on a regular basis by many experienced observers worldwid...
Double station data on 496 meteors belonging to several meteor showers were obtained within the pro...
By using of new discrete solution of a quasi thomography problem of determination of a meteor spatia...
A quasi-thomography procedure application to the goniometric data of a meteor radar has allowed conf...
The structure of a radar-derived meteoroid orbit data set is examined in the current study. Biases i...
Perseid and sporadic meteor hourly rates and magnitudes observed in 1953-1983 by a team of visual ob...
peer reviewedWhat long-period comets with orbital periods >250 years cause detectable meteor showers...
74-75Results of an extensive study of the visual meteor survey of the geminid shower observed during...
Context. The double-station video experiment was established in Tajikistan to confirm the ...
By analyzing high-accuracy Leonid orbits obtained from multiple-station meteor observations during t...
The results of an analysis of the orbital structure of the meteor complex accessible for radar obser...
The radar detection of meteor trails is discussed with reference to the equipment used, the methods ...
Meteor radar observations at the Sodankylä Geophysical Observatory (67° 22′N, 26° 38′E, Finland) ind...
Sufficient observations exist of the returns of comet 55P!fempel-Tuttle in 1865 and 1965 for accurat...
All-sky Meteor Orbit System (AMOS) is a semi-autonomous video observatory for detection of transient...
Visual meteor observations are carried out on a regular basis by many experienced observers worldwid...
Double station data on 496 meteors belonging to several meteor showers were obtained within the pro...
By using of new discrete solution of a quasi thomography problem of determination of a meteor spatia...
A quasi-thomography procedure application to the goniometric data of a meteor radar has allowed conf...
The structure of a radar-derived meteoroid orbit data set is examined in the current study. Biases i...
Perseid and sporadic meteor hourly rates and magnitudes observed in 1953-1983 by a team of visual ob...
peer reviewedWhat long-period comets with orbital periods >250 years cause detectable meteor showers...
74-75Results of an extensive study of the visual meteor survey of the geminid shower observed during...
Context. The double-station video experiment was established in Tajikistan to confirm the ...
By analyzing high-accuracy Leonid orbits obtained from multiple-station meteor observations during t...
The results of an analysis of the orbital structure of the meteor complex accessible for radar obser...
The radar detection of meteor trails is discussed with reference to the equipment used, the methods ...
Meteor radar observations at the Sodankylä Geophysical Observatory (67° 22′N, 26° 38′E, Finland) ind...
Sufficient observations exist of the returns of comet 55P!fempel-Tuttle in 1865 and 1965 for accurat...
All-sky Meteor Orbit System (AMOS) is a semi-autonomous video observatory for detection of transient...
Visual meteor observations are carried out on a regular basis by many experienced observers worldwid...