Specimen Fireball 1
: December 11, 2008 1149 UT
( 4:49 am MST )
Observer's comment: This was the brightest fireball of the night and
happened directly over Albuquerque, New Mexico.
Sonic
Movie 1: Ashcraft's dual frequency forward
scatter system; video and stereo sound:
This fireball occurred during a previous radio fireball reflection so it
is difficult to distinguish the head echo. Full duration of reflection
in next movie.
FB20081211_1149uthe_Ashcraft.mp4
22 seconds 1.1 MB
Sonic
Movie 2: Ashcraft's dual frequency forward
scatter system; video and stereo sound:
Strong fireball.
Fb20081211_1149utlo_Ashcraft.mp4
1 minute 41 seconds 5 MB
Here is the movie from the Sandia Sentinel camera system, without sound:
v20081211_044931.29.mov
Radio spectrogram of the
time of the above meteor. 61.250 MHz reception
above white line, 83.250
MHz below white line.
Meteor reflection occurs during the 1149-1151 UT minutes
in following two spectrograms.
Specimen
Fireball 2: December 11, 2008 0635 UT
Sonic
Movie 1: Ashcraft's dual frequency forward
scatter system; video and stereo sound:
Good dopplering head echo.
FB20081211_0635uthe_Ashcraft.mp4 12
seconds 700 KB
Sonic
Movie 2: Ashcraft's dual frequency forward
scatter system; video and stereo sound:
Strong fireball.
FB20081211_0635utlo_Ashcraft.mp4
1 minute 9 seconds 3.5 MB
Radio spectrogram of the
time of the above meteor. 61.250 MHz reception
above white line, 83.250
MHz below white line.
Meteor reflection occurs during the 0635-0636 UT minutes.
Specimen Fireball 3
: December 11, 2008 0819 UT
Sonic
Movie : Ashcraft's dual forward scatter
system; video and stereo sound:
Hard to see this meteor in movie.
FB20081211_0819ut_Ashcraft.mp4
44 seconds 2.2 MB
Radio spectrogram of the
time of the above meteor. 61.250 MHz reception
above white line, 83.250
MHz below white line.
Meteor reflection occurs during the 0819-0920 UT minutes.
Specimen Fireball 4
: December 11, 2008 0833 UT
Sonic
Movie : Ashcraft's dual forward scatter
system; video and stereo sound:
Nice stereo doppler with moderate trailing ionization.
FB20081211_0833ut_Ashcraft.mp4
1 minute 8 seconds 3.5 MB
Radio spectrogram of the
time of the above meteor. 61.250 MHz reception
above white line, 83.250
MHz below white line.
Meteor reflection occurs during the 0833-0834 UT minutes.
Specimen Fireball 5
: December 11, 2008 0935 UT
Sonic Movie : Ashcraft's
dual forward scatter system; video
and stereo sound:
Small head echo with trailing ionization.
FB20081211_0935ut_Ashcraft.mp4
1 minute 19 seconds 1.5 MB
Radio spectrogram of the
time of the above meteor. 61.250 MHz reception
above white line, 83.250
MHz below white line.
Meteor reflection occurs during the 0935 UT minute.
Specimen Fireball 6
: December 11, 2008 1026 UT
Sonic Movie : Ashcraft's
dual forward scatter system; video
and stereo sound:
Good specimen.
FB20081211_1026ut_Ashcraft.mp4
57 seconds 2.8 MB
Radio spectrogram of the
time of the above meteor. 61.250 MHz reception
above white line, 83.250
MHz below white line.
Meteor reflection occurs during the 1026-1027 UT minutes.
Specimen Fireball 7
: December 11, 2008 1237 UT
No sonic movie for this fireball.
Radio spectrogram of the
time of the above meteor. 61.250 MHz reception
above white line, 83.250
MHz below white line.
Meteor reflection occurs during the 1237 UT minute.
Specimen Fireball 8
: December 11, 2008 1301 UT
Sonic Movie : Ashcraft's
dual forward scatter system; video
and stereo sound:
Subtle reflection.
FB20081211_1301ut_Ashcraft.mp4
26 seconds 1.2 MB
Radio spectrogram of the
time of the above meteor. 61.250 MHz reception
above white line, 83.250
MHz below white line.
Meteor reflection occurs during the 1301 UT minutes.
Specimen Fireball 9
: December 11, 2008 1325 UT
Sonic Movie : Ashcraft's
dual forward scatter system; video
and stereo sound:
Strong reflection. Almost a daylight fireball.
FB20081211_1325utlo_Ashcraft.mp4
1 minute 32 seconds 3.6 MB
Radio spectrogram of the
time of the above meteor. 61.250 MHz reception
above white line, 83.250
MHz below white line.
Meteor reflection occurs during the 1325-1326 UT minutes.
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