A brief description is given of the instrumentation, the facilities, and the patrol technique used by the NASA faint meteor spectra patrol. A classification of 500 meteor spectra obtained in the first 2-1/2 years of the patrol is reported. The general characteristics of typical spectra are discussed and preliminary conclusions drawn. Examples of unusual spectra are briefly described
It is proposed to carry out slitless spectroscopy at ultraviolet wavelengths from orbit of meteoric ...
Meteor spectroscopy provides valuable data about the composition of meteoroids striking the atmosp...
Context. Meteor spectra are commonly interpreted using data from databases and tables. Several studi...
Composition and mass data analysis of meteoroids in 1 milligram to 1 gram range using NASA LRC Faint...
Studies on meteor spectroscopy are reported. The following topics are discussed: photometric spectra...
A spectrogram of a fast optical meteor was reduced and analyzed, and 60 features were identified in ...
Preliminary data required to extrapolate available meteor physics information (obtained in the photo...
Spectral observations of meteors have been carried out for several years using an optical electronic...
Since the advent of low light level television (LLLTV) systems, it has been recognized that such dev...
Low light level television systems offer the ability to observe meteors as faint as 10th magnitude w...
The radar detection of meteor trails is discussed with reference to the equipment used, the methods ...
Aims. We present a library of low-resolution meteor spectra that includes sporadic meteors...
Small, faint meteors (with masses between 10-7 and 10-4 kg) were once part of an asteroid or comet, ...
We have optically recorded faint meteors using a large aperture LLLTV (low light level television) s...
Meteorite samples are measured with the University of Helsinki integrating-sphere UV-vis-NIR spectro...
It is proposed to carry out slitless spectroscopy at ultraviolet wavelengths from orbit of meteoric ...
Meteor spectroscopy provides valuable data about the composition of meteoroids striking the atmosp...
Context. Meteor spectra are commonly interpreted using data from databases and tables. Several studi...
Composition and mass data analysis of meteoroids in 1 milligram to 1 gram range using NASA LRC Faint...
Studies on meteor spectroscopy are reported. The following topics are discussed: photometric spectra...
A spectrogram of a fast optical meteor was reduced and analyzed, and 60 features were identified in ...
Preliminary data required to extrapolate available meteor physics information (obtained in the photo...
Spectral observations of meteors have been carried out for several years using an optical electronic...
Since the advent of low light level television (LLLTV) systems, it has been recognized that such dev...
Low light level television systems offer the ability to observe meteors as faint as 10th magnitude w...
The radar detection of meteor trails is discussed with reference to the equipment used, the methods ...
Aims. We present a library of low-resolution meteor spectra that includes sporadic meteors...
Small, faint meteors (with masses between 10-7 and 10-4 kg) were once part of an asteroid or comet, ...
We have optically recorded faint meteors using a large aperture LLLTV (low light level television) s...
Meteorite samples are measured with the University of Helsinki integrating-sphere UV-vis-NIR spectro...
It is proposed to carry out slitless spectroscopy at ultraviolet wavelengths from orbit of meteoric ...
Meteor spectroscopy provides valuable data about the composition of meteoroids striking the atmosp...
Context. Meteor spectra are commonly interpreted using data from databases and tables. Several studi...