During the 1999 Leonids, an intensified HDTV camera was used for slitless m
eteor spectroscopy at visible and near-UV wavelengths in three night flight
s of the Leonid Multi-instrument Aircraft Campaign. The IIDTV system provid
ed a high dynamic range (digital 10-bit) and a wide field of view of 37 x 2
1 degrees. The maximum spectral sensitivity is at 405 nm, while the resolvi
ng power of the spectrograph was lambda/Delta lambda similar to 250. Here,
we report on the results for one particularly nice spectrum from a Leonid m
eteor at 03:24:40 UT. Numerous atomic emission lines of magnesium and iron
were detected, with an excitation temperature of T = 5,000 +/- 1,000. It is
confirmed that sodium is released from the meteoroid earlier than iron and
magnesium, just as in meteors of the 1998 Leonid shower. Rovibrational ban
ds of N-2 dominate the spectrum in the visible and near-IR. We searched for
CN band emission at 389 nm, but could not detect it due to the overlap of
numerous iron lines.