Physics – Optics
Scientific paper
Jan 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005georl..3202103h&link_type=abstract
Geophysical Research Letters, Volume 32, Issue 2, CiteID L02103
Physics
Optics
6
Atmospheric Composition And Structure: Airglow And Aurora, Atmospheric Composition And Structure: Thermosphere: Energy Deposition (3369), Electromagnetics: Optics (4264), Electromagnetics: Instruments And Techniques
Scientific paper
An all-sky scanning Fabry-Pérot spectrometer was used to observe temperatures of auroral OI (557.7-nm) emissions over Poker Flat, Alaska (65.12N, 147.43W). The sudden temporal and spatial changes in Doppler temperatures observed are likely owing to the emission height changing as a response to variations in the characteristic energy of the precipitating electron population. Three cases were analyzed: (1) A Doppler temperature drop (~200 K) over the entire sky occurred immediately after an auroral brightening; the temperature remained lower after the auroral intensity had resumed its quiescent levels. (2) A local increase of Doppler temperature, colocated with a weak auroral arc, occurred 25 minutes before a westward propagating substorm onset. When the auroral luminosity suddenly increased the Doppler temperature had a sharp decrease. (3) The region inside a loop-like auroral arc showed elevated Doppler temperature relative to that of the arc itself. Auroral fading prior to onset was accompanied by increased temperatures.
Conde Maria M.
Deehr Charles
Holmes Jeremy M.
Lummerzheim Dirk
No associations
LandOfFree
Morphology of evening sector aurorae in λ557.7-nm Doppler temperatures does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Morphology of evening sector aurorae in λ557.7-nm Doppler temperatures, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Morphology of evening sector aurorae in λ557.7-nm Doppler temperatures will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-902264