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Mesospheric temperature estimation from meteor decay times during Geminids meteor shower. / Kozlovsky, Alexander; Lukianova, Renata; Shalimov, Sergey; Lester, Mark.

в: Journal of Geophysical Research: Space Physics, Том 121, № 2, 30.01.2016, стр. 1669-1679.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Kozlovsky, A, Lukianova, R, Shalimov, S & Lester, M 2016, 'Mesospheric temperature estimation from meteor decay times during Geminids meteor shower', Journal of Geophysical Research: Space Physics, Том. 121, № 2, стр. 1669-1679. https://doi.org/10.1002/2015JA022222

APA

Kozlovsky, A., Lukianova, R., Shalimov, S., & Lester, M. (2016). Mesospheric temperature estimation from meteor decay times during Geminids meteor shower. Journal of Geophysical Research: Space Physics, 121(2), 1669-1679. https://doi.org/10.1002/2015JA022222

Vancouver

Kozlovsky A, Lukianova R, Shalimov S, Lester M. Mesospheric temperature estimation from meteor decay times during Geminids meteor shower. Journal of Geophysical Research: Space Physics. 2016 Янв. 30;121(2):1669-1679. https://doi.org/10.1002/2015JA022222

Author

Kozlovsky, Alexander ; Lukianova, Renata ; Shalimov, Sergey ; Lester, Mark. / Mesospheric temperature estimation from meteor decay times during Geminids meteor shower. в: Journal of Geophysical Research: Space Physics. 2016 ; Том 121, № 2. стр. 1669-1679.

BibTeX

@article{d4e946781c1e4109896f59970875ed10,
title = "Mesospheric temperature estimation from meteor decay times during Geminids meteor shower",
abstract = "Meteor radar observations at the Sodankyl{\"a} Geophysical Observatory (67° 22′N, 26° 38′E, Finland) indicate that the mesospheric temperature derived from meteor decay times is systematically underestimated by 20-50 K during the Geminids meteor shower which has peak on 13 December. A very good coincidence of the minimum of routinely calculated temperature and maximum of meteor flux (the number of meteors detected per day) was observed regularly on that day in December 2008-2014. These observations are for a specific height-lifetime distribution of the Geminids meteor trails and indicate a larger percentage of overdense trails compared to that for sporadic meteors. A consequence of this is that the routine estimates of mesospheric temperature during the Geminids are in fact underestimates. The observations do, however, indicate unusual properties (e.g., mass, speed, or chemical composition) of the Geminids meteoroids. Similar properties were found also for Quadrantids in January 2009-2015, which like the Geminids has as a parent body an asteroid, but not for other meteor showers.",
keywords = "Geminids, mesosphere temperature, meteors, Quadrantids, radar",
author = "Alexander Kozlovsky and Renata Lukianova and Sergey Shalimov and Mark Lester",
year = "2016",
month = jan,
day = "30",
doi = "10.1002/2015JA022222",
language = "English",
volume = "121",
pages = "1669--1679",
journal = "Journal of Geophysical Research: Biogeosciences",
issn = "0148-0227",
publisher = "American Geophysical Union",
number = "2",

}

RIS

TY - JOUR

T1 - Mesospheric temperature estimation from meteor decay times during Geminids meteor shower

AU - Kozlovsky, Alexander

AU - Lukianova, Renata

AU - Shalimov, Sergey

AU - Lester, Mark

PY - 2016/1/30

Y1 - 2016/1/30

N2 - Meteor radar observations at the Sodankylä Geophysical Observatory (67° 22′N, 26° 38′E, Finland) indicate that the mesospheric temperature derived from meteor decay times is systematically underestimated by 20-50 K during the Geminids meteor shower which has peak on 13 December. A very good coincidence of the minimum of routinely calculated temperature and maximum of meteor flux (the number of meteors detected per day) was observed regularly on that day in December 2008-2014. These observations are for a specific height-lifetime distribution of the Geminids meteor trails and indicate a larger percentage of overdense trails compared to that for sporadic meteors. A consequence of this is that the routine estimates of mesospheric temperature during the Geminids are in fact underestimates. The observations do, however, indicate unusual properties (e.g., mass, speed, or chemical composition) of the Geminids meteoroids. Similar properties were found also for Quadrantids in January 2009-2015, which like the Geminids has as a parent body an asteroid, but not for other meteor showers.

AB - Meteor radar observations at the Sodankylä Geophysical Observatory (67° 22′N, 26° 38′E, Finland) indicate that the mesospheric temperature derived from meteor decay times is systematically underestimated by 20-50 K during the Geminids meteor shower which has peak on 13 December. A very good coincidence of the minimum of routinely calculated temperature and maximum of meteor flux (the number of meteors detected per day) was observed regularly on that day in December 2008-2014. These observations are for a specific height-lifetime distribution of the Geminids meteor trails and indicate a larger percentage of overdense trails compared to that for sporadic meteors. A consequence of this is that the routine estimates of mesospheric temperature during the Geminids are in fact underestimates. The observations do, however, indicate unusual properties (e.g., mass, speed, or chemical composition) of the Geminids meteoroids. Similar properties were found also for Quadrantids in January 2009-2015, which like the Geminids has as a parent body an asteroid, but not for other meteor showers.

KW - Geminids

KW - mesosphere temperature

KW - meteors

KW - Quadrantids

KW - radar

UR - http://www.scopus.com/inward/record.url?scp=84975748722&partnerID=8YFLogxK

U2 - 10.1002/2015JA022222

DO - 10.1002/2015JA022222

M3 - Article

AN - SCOPUS:84975748722

VL - 121

SP - 1669

EP - 1679

JO - Journal of Geophysical Research: Biogeosciences

JF - Journal of Geophysical Research: Biogeosciences

SN - 0148-0227

IS - 2

ER -

ID: 36800473