HR: 10:25h
AN: AE41B-01 INVITED [PDF]
TI: New Space Shuttle Observations of Transient Luminous Events During the MEIDEX
AU: * Yair, Y
EM: yoavya@openu.ac.il
AF: The Open University of Israel, 16 Klausner St., Tel-Aviv, 61392
Israel
AU: Price, C
EM: cprice@flash.tau.ac.il
AF: Tel-Aviv University, Haim Levanon Rd., Tel-Aviv, 69978
Israel
AU: Israelevitch, P
EM: peter@luna.tau.ac.il
AF: Tel-Aviv University, Haim Levanon Rd., Tel-Aviv, 69978
Israel
AU: Devir, A
EM: iardad@iard.org.il
AF: Tel-Aviv University, Haim Levanon Rd., Tel-Aviv, 69978
Israel
AU: Moalem, M
EM: meir_moalem@yahoo.com
AF: IAF, Space Branch, Tel-Aviv, 61909
Israel
AU: Ziv, B
EM: baruchz@openu.ac.il
AF: The Open University of Israel, 16 Klausner St., Tel-Aviv, 61392
Israel
AU: Levin, Z
EM: zev@hail.tau.ac.il
AF: Tel-Aviv University, Haim Levanon Rd., Tel-Aviv, 69978
Israel
AU: Joseph, J
EM: yoya@luna.tau.ac.il
AF: Tel-Aviv University, Haim Levanon Rd., Tel-Aviv, 69978
Israel
AB:
The Mediterranean Israeli Dust Experiment (MEIDEX) was conducted on-board the space shuttle Columbia during its last mission
in January 2003. Nocturnal observations with a multispectral CCD video camera were targeted above thunderstorms near the
Earth's limb, with the aim or recording Transient Luminous Events (TLEs) in the mesosphere. Most of our nighttime
observations were conducted in the SE-Pacific (Australia and Papua-New Guinea), equatorial Africa, the southern Indian Ocean
and South America. Relevant inputs and information on the active storms during a specific orbit were uplinked to the crew
daily. The necessary shuttle attitude maneuvers were deduced based on the use of (almost) real-time IR satellite images and
VLF lightning location data that were available on the Internet. In order to enhance the probability of success of each
observation, the astronauts were instructed to visually observe lightning activity (easily discernable from the shuttle) and
to direct the gimbaled camera toward these regions.
A total of more than 8 hours of video obtained during the MEIDEX was saved, and it includes a considerable amount of new
sprite data. Most events were captured at ranges 1600-1900 km from the shuttle, using the red filter (665nm). The results
suggest the occurrence rate of sprites and elves over oceanic and continental storms may be higher than earlier estimates.
Strong enhancements of the brightness of the airglow layer above lightning flashes were observed, with lateral dimensions on
the order of 400-500 km. It is assumed that these may be Elves observed edge-on, though it may also be a new type of airglow
enhancement. The calculated brightness of these events is in the range 2.2-8.8 MR. This phenomena seems to be widespread and
is probably a manifestation of the interaction between lightning EMP and QE fields and the lower nocturnal ionosphere. A
unique observation from space of the Congo basin in Africa caught a chain of events where in the span of less than 2 minutes
two meteors penetrated above a thunderstorm, that immediately afterwards generated several Sprites and Elves in the same
atmospheric volume. This seems to confirm earlier observations and theoretical work on the role of meteors in mesospheric TLE
generation. International, multiple-station ground-based ELF-VLF data obtained during the mission is used for geo-location
of the parent flashes of the optically visible TELs.
DE: 0310 Airglow and aurora
DE: 2427 Ionosphere/atmosphere interactions (0335)
DE: 2435 Ionospheric disturbances
DE: 3304 Atmospheric electricity
DE: 3324 Lightning
SC: Atmospheric and Space Electricity [AE]
MN: 2003 Fall Meeting