Zobrazeno 1 - 10
of 3 454
pro vyhledávání: '"Meteor (satellite)"'
Publikováno v:
Advances in Space Research. 69:1344-1350
Our observations show that on some occasions an influx of meteor ablation possibly contributes to appearance of a sudden enhancement in mesospheric sodium density. On July 05, 2013, all-sky images with a narrow sodium filter in the 589 nm emission, o
Publikováno v:
Cosmic Research. 59:433-445
Autor:
Anna Solomatnikova, Yana Virolainen, Alexander V. Polyakov, Georgy Nerobelov, Y. M. Timofeyev
Publikováno v:
International Journal of Remote Sensing. 42:8709-8733
Ozone is one of the key atmospheric trace gases that protects life on Earth from harmful solar ultraviolet radiation. The importance of ozone and its influence on various atmospheric processes led ...
Autor:
Josep M. Trigo-Rodríguez, Jürgen Blum
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 512:2277-2289
Meteor physics can provide new clues about the size, structure, and density of cometary disintegration products, establishing a bridge between different research fields. From meteor magnitude data we have estimated the mass distribution of meteoroids
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 508:3897-3909
To guarantee the successful observation of a meteor shower, the ‘Meteor Automated Light Balloon Experimental Camera’ will put two meteor cameras aboard stratospheric nacelles, at altitudes where clouds can no longer hinder the observation. After
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 508:326-339
Meteor showers occur when streams of meteoroids originating from a common source intersect the Earth. There will be small dissimilarities between the direction of motion of different meteoroids within a stream, and these small differences will act to
Publikováno v:
Annales Geophysicae, Vol 39, Pp 709-719 (2021)
Non-specular meteor trail echoes are radar reflections from plasma instabilities that are caused by field-aligned irregularities. Meteor simulations are examined to show that these plasma instabilities, and thus the associated meteor trail echo, stro
Autor:
M. Kaliuzhnyi, S. G. Savchuk, A.V. Shulga, B. O. Hrudynin, N.A. Kulichenko, L. M. Yankiv-Vitkovska, F.I. Bushuev, Ye.V. Malynovskyi
Publikováno v:
Kosmìčna nauka ì tehnologìâ. 27:85-92
During the decade of research, the Research Institute “Mykolaiv Astronomical Observatory” (RI “MAO”) developed hardware and software for monitoring, extracting, and calculating the parameters of meteor phenomena using the forward scattering b
Publikováno v:
Atmospheric Measurement Techniques, Vol 14, Pp 3583-3596 (2021)
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
Publikováno v:
Astronomy Reports. 65:427-434
The problems of the study of small celestial bodies are an important component of modern space research. This applies both to the study of physicochemical and evolutionary parameters and the search for the genetic relationships between meteor showers