this an — 
gular effect i 
t in the meteoric plane is simply + AM on,at 
perp br 
an extreme fo 
other dista r the same conditi 
nees inversely as os legge + 6°6/; and for 
ce. (D) 
Referring now ffects rving the 
ow to i bse 
angles of the e in the plane u v and obse ing 
of mm, and 72° in the eas 268 
eof rr, and with the velocity 168 
miles per seco 
ond j 
ccond, while that of the earth is 18:89, we obtain ior 
; that 
