The 2011 Draconids: The First European Airborne Meteor Observation Campaign

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00444961" target="_blank" >RIV/67985815:_____/15:00444961 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.1007/s11038-014-9455-5" target="_blank" >http://dx.doi.org/10.1007/s11038-014-9455-5</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1007/s11038-014-9455-5" target="_blank" >10.1007/s11038-014-9455-5</a>

Jazyk výsledku

angličtina

Název v původním jazyce

The 2011 Draconids: The First European Airborne Meteor Observation Campaign

Popis výsledku v původním jazyce

On 8 October 2011, the Draconid meteor shower (IAU#8, DRA) was predicted to cause two brief outbursts of meteors, visible from locations in Europe. For the first time, a European airborne meteor observation campaign was organized, supported by ground-based observations. Two aircraft were deployed from Kiruna, Sweden, carrying six scientists, 19 cameras and eight crew members. The flight geometry was chosen such that it was possible to obtain double-station observations of many meteors. The instrument setup on the aircraft as well as on the ground is described in full detail. The main peak from 1900-dust ejecta happened at the predicted time and at the predicted rate. The second peak was observed from the earlier flight and from the ground, and was caused most likely by trails ejected in the nineteenth century. A total of 250 meteors were observed, for which light curve data were derived. The trajectory, velocity, deceleration and orbit of 35 double station meteors were measured. The ma

Název v anglickém jazyce

The 2011 Draconids: The First European Airborne Meteor Observation Campaign

Popis výsledku anglicky

On 8 October 2011, the Draconid meteor shower (IAU#8, DRA) was predicted to cause two brief outbursts of meteors, visible from locations in Europe. For the first time, a European airborne meteor observation campaign was organized, supported by ground-based observations. Two aircraft were deployed from Kiruna, Sweden, carrying six scientists, 19 cameras and eight crew members. The flight geometry was chosen such that it was possible to obtain double-station observations of many meteors. The instrument setup on the aircraft as well as on the ground is described in full detail. The main peak from 1900-dust ejecta happened at the predicted time and at the predicted rate. The second peak was observed from the earlier flight and from the ground, and was caused most likely by trails ejected in the nineteenth century. A total of 250 meteors were observed, for which light curve data were derived. The trajectory, velocity, deceleration and orbit of 35 double station meteors were measured. The ma

Druh

J_x - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)

CEP obor

BN - Astronomie a nebeská mechanika, astrofyzika

OECD FORD obor

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Projekt

<a href="/cs/project/GA14-25251S" target="_blank" >GA14-25251S: Nelineární obrazové systémy s prostorově variantní bodovou rozptylovou funkcí</a><br>

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2015

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Earth, Moon, and Planets

ISSN

0167-9295

e-ISSN

—

Svazek periodika

114

Číslo periodika v rámci svazku

3-4

Stát vydavatele periodika

NL - Nizozemsko

Počet stran výsledku

21

Strana od-do

137-157

Kód UT WoS článku

000350232200003

EID výsledku v databázi Scopus

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