OA fE TI'.~E vqOUP 2. SOURCE 10. CONCLUSION .t. NUMBER OF 03JE CTS 11. B~I:!P SU\W!.RY AND ANALYSIS s. LE:NGTH OF O:lSEAVA TION 6. TYPE OF OBSERVATION G1otm !-'/i:;uJ o. PHOiOS 9. PHYSIC!.L EVIOENC! FTD se P 6 3 0329 (TOE) p,..,tcna IUU- o1 o.tt lora_, be " \ ..J COL O Pt\R:\Pli \SE r~OT R!:Qt'lf)EO. s:F. C:~YPTO cr~lfF.~ f'll' I II I. P~9Er1ptio~ or Incidt~t At 0910 :l a blui~h e.r:Zlerical light with n tapering tail wa 3 obser ved movi: g aour~o~aly at a tremendo~3 spoed and e t n croat distance , parall6l to tho hori- son, tor 3 Becor~ The roport. ind1cate3 tha t tho objoctlns probably n mot oor. Tho dcncrlpti'>n cfven close~ approximates a meteor's performance~ III. Conclu!lion Probably a:Jtro nomicul phono::1enon UNCL/'.SS r