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Lidar observations of elevated temperatures in bright chemiluminescent meteor trails during the 1998 Leonid Shower
Author(s) -
Chu Xinzhao,
Liu Alan Z.,
Papen George,
Gardner Chester S.,
Kelley Michael,
Drummond Jack,
Fugate Robert
Publication year - 2000
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2000gl000080
Subject(s) - meteoroid , meteor shower , meteor (satellite) , lidar , airglow , environmental science , atmosphere (unit) , atmospheric sciences , astrophysics , meteorology , physics , astrobiology , optics
Seven persistent trails associated with bright fireballs were probed with a steerable Na wind/temperature lidar at Starfire Optical Range, NM during the 17/18 Nov peak of the 1998 Leonid meteor shower. These chemiluminescence trails were especially rich in Na. The average Na abundance within the trails was 52% of the background Na layer abundance, which suggests that the corresponding masses of the meteors were from l g up to 1 kg. CCD images show that the chemiluminescent emissions (including Na and OH) are confined to the walls of a tube, which expands with time by molecular diffusion. Lidar profiles within the trails show that the temperatures are highest at the edges of the tube where the airglow emissions are brightest. Approximately 3 min after ablation, temperatures at the tube walls are 20–50 K warmer than the tube core and background atmosphere. Neither chemical nor frictional heating provides a satisfactory explanation for the observations.