Meteors and Meteor Showers as Observed by Optical Techniques
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00520232" target="_blank" >RIV/67985815:_____/19:00520232 - isvavai.cz</a>
Výsledek na webu
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DOI - Digital Object Identifier
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Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Meteors and Meteor Showers as Observed by Optical Techniques
Popis výsledku v původním jazyce
Optical observations are one of the most important sources of data for meteor science. Visual observation was the only method used for centuries and remains an important branch of meteor astronomy for monitoring daily shower activity. Photography became an important tool in the second half of the 20th century, later followed by television and video. Direct and spectral observational techniques have experienced significant progress in the last two decades. Today, all these techniques provide valuable data on meteors and meteor showers. The separate experiments of past decades have evolved into multi-instrumental campaigns which can significantly increase scientific output from observations. Combining data can provide more information about such events than photographic or video records alone. The importance of optical observations has been realized in many branches of meteor astronomy. Visual and video observations of meteor shower activity are often used for validation of meteor stream models. Models of meteoroid structure and fragmentation are based on photographic and video data. Meteorite falls are often optically recorded from multiple sites to determine strewn field locations.
Název v anglickém jazyce
Meteors and Meteor Showers as Observed by Optical Techniques
Popis výsledku anglicky
Optical observations are one of the most important sources of data for meteor science. Visual observation was the only method used for centuries and remains an important branch of meteor astronomy for monitoring daily shower activity. Photography became an important tool in the second half of the 20th century, later followed by television and video. Direct and spectral observational techniques have experienced significant progress in the last two decades. Today, all these techniques provide valuable data on meteors and meteor showers. The separate experiments of past decades have evolved into multi-instrumental campaigns which can significantly increase scientific output from observations. Combining data can provide more information about such events than photographic or video records alone. The importance of optical observations has been realized in many branches of meteor astronomy. Visual and video observations of meteor shower activity are often used for validation of meteor stream models. Models of meteoroid structure and fragmentation are based on photographic and video data. Meteorite falls are often optically recorded from multiple sites to determine strewn field locations.
Klasifikace
Druh
C - Kapitola v odborné knize
CEP obor
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OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
<a href="/cs/project/GA16-00761S" target="_blank" >GA16-00761S: Rozpady meteoroidů a malých asteroidů v zemské atmosféře</a><br>
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2019
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název knihy nebo sborníku
Meteoroids: Sources of Meteors on Earth and Beyond
ISBN
9781108426718
Počet stran výsledku
26
Strana od-do
90-115
Počet stran knihy
306
Název nakladatele
University Press
Místo vydání
Cambridge
Kód UT WoS kapitoly
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