Flux density over the celestial sphere and meteoroid orbital element distributions are discussed. Corrected for selections of observations methods distributions has been compared. Sporadic meteoroid velocity distributions do not depend on minimum registered mass of meteoroids in mass interval 1-10-4 g and depend only on radiant elongation from the Earth's apex. Now there are not reliable sporadic distributions of flux densities over the celestial sphere or distributions of orbital elements confirmed by comparison of results obtained even two different method of observations
The orbital element distributions of meteoroids detected during the Harvard Radio Meteor Project, 19...
International audienceSporadic meteoroids are the most abundant yet least understood component of th...
Hypothesis that the sources of interstellar particles are planet systems of late class stars is disc...
Flux density over the celestial sphere and meteoroid orbital element distributions are discussed. Co...
Flux density over the celestial sphere and meteoroid orbital element distributions are discussed. Co...
The distribution of orbital elements and flux density over the celestial sphere are the most common ...
An analysis of sporadic meteor flux distributions over the celestial sphere is given. Symmetry of th...
Hypothesis that the sources of interstellar particles are planet systems of late class stars is disc...
The meteoroid population in near-Earth space is typically broken down into two components: shower me...
No model of distribution of meteor substance is known to explain the observed diurnal and annual var...
An analysis of the Perseid meteoroid mass distribution is given. It is shown that particle mass dist...
Long-term visual observations of the Lyrid meteoroid shower have been analyzed to determine the mass...
International audienceSporadic meteoroids are the most abundant yet least understood component of th...
We developed a parametric model of the spatial distribution of sporadic meteoroids by taking their p...
The orbital element distributions of meteoroids detected during the Harvard Radio Meteor Project, 19...
The orbital element distributions of meteoroids detected during the Harvard Radio Meteor Project, 19...
International audienceSporadic meteoroids are the most abundant yet least understood component of th...
Hypothesis that the sources of interstellar particles are planet systems of late class stars is disc...
Flux density over the celestial sphere and meteoroid orbital element distributions are discussed. Co...
Flux density over the celestial sphere and meteoroid orbital element distributions are discussed. Co...
The distribution of orbital elements and flux density over the celestial sphere are the most common ...
An analysis of sporadic meteor flux distributions over the celestial sphere is given. Symmetry of th...
Hypothesis that the sources of interstellar particles are planet systems of late class stars is disc...
The meteoroid population in near-Earth space is typically broken down into two components: shower me...
No model of distribution of meteor substance is known to explain the observed diurnal and annual var...
An analysis of the Perseid meteoroid mass distribution is given. It is shown that particle mass dist...
Long-term visual observations of the Lyrid meteoroid shower have been analyzed to determine the mass...
International audienceSporadic meteoroids are the most abundant yet least understood component of th...
We developed a parametric model of the spatial distribution of sporadic meteoroids by taking their p...
The orbital element distributions of meteoroids detected during the Harvard Radio Meteor Project, 19...
The orbital element distributions of meteoroids detected during the Harvard Radio Meteor Project, 19...
International audienceSporadic meteoroids are the most abundant yet least understood component of th...
Hypothesis that the sources of interstellar particles are planet systems of late class stars is disc...