< T A B L E B O R D E R = 0 C E L L S P A C I N G = 0 C E L L P A D D I N G = 0 W I D T H = 7 0 0 > < T R B G C O L O R = " # 0 0 0 0 0 0 " V A L I G N = T O P A L I G N = R I G H T > < T D B G C O L O R = " # 0 0 0 0 0 0 " > < T A B L E B O R D E R = 0 C E L L S P A C I N G = 0 C E L L P A D D I N G =0 WIDTH=110 > < T R V A L I G N = T O P A L I G N = L E F T W I D T H = 1 1 0 > < T D B G C O L O R = " # 0 0 0 0 0 0 " > < c e n t e r > < P > < i m g s r c = " l o g o _ 3 d . g i f " a l t = " l o g o " a l i g n = " b o t t o m " > < H 3 > L e o n i d M A C < / H 3 > < / f o n t > < / t d > < / t r >
Philip D. Hammer, NASA Ames Research Center, CA 
Last updated: October 1999
Brief Biographical Information: Staff scientist, NASA Ames Research Center, Earth Science Division (Code SG), Moffett Field CA. Previously - Research associate, NOAA Aeronomy Laboratory U. of Colorado (CIRES), Atmospheric Chemical Kinetics Group, Boulder CO. Ph.D. (physics), 1981, Univ. of Calif., Berkeley CA. Research:
Near-IR spectral imagery of meteors. I am instrument co-PI with Bill Smith of the University of Washington for the ERAST/DASI instrument. Related spectral imaging sensor work (ERAST/DASI)
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