The 2012 geminids balloon-borne mission over Spain
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Abstract
Observing meteors from the stratosphere
improves detection efficiency thanks to much
lower extinction. Previous airborne missions have already
monitored meteor outbursts. However due to
their cost these missions are not suitable for annual meteor
shower maxima. Thus meteor video detection with
low-light cameras on-board weather balloons is a good
approach to observe meteors in such ideal conditions
[2].
The SPanish Meteor Network (SPMN) has 25
video and CCD observing stations currently operational
[3-5]. The recording of multi-stations meteors
and fireballs each night is only jeopardised by bad
weather conditions. However the addition of balloon
observations can improve observational results with
bad weather during meteor maxima.
During the Geminids 2012 activity peak the Fireball
and Meteor group of the Universidad Complutense
de Madrid[6] launched a balloon in collaboration with
Proyecto Daedalus [1]. During that night the sky was
unfortunately covered in several SPMN stations of central
Spain. However the camera on-board our balloon
detected several Geminids from the troposphere and
the stratosphere, allowing double-station detection with
stations with clear skies located over more distant
SPMN stations in the Iberian Peninsula.
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Bibliographic citation
Sánchez de Miguel, A., Ocaña Gónzalez, F., Madiedo Gil, J.M., Ortuño, F., Conde, A., León, P., Gómez Sánchez-Tirado, M.A., Mayo, D., Raya, R., Zamorano, J., Izquierdo Gómez, J., Trigo Rodríguez, J.M.: "The 2012 geminids balloon-borne mission over Spain". En: 44th Lunar and Planetary Science Conference (The Woolands, Texas, march 18-22, 2013)








