Disk
brightness profiles
from eclipses
€From
the eclipse shadows the brightness of each part of the disk can be determined
€Behaviour
can be followed
through an outburst
€Changes can be seen in the structure of the disk
€In
bright states the disk temperature is T µ
r –3/4
€In
faint states the disk temperature has a flatter relation and the
effect of the hot spot from the stream impact is evident
EX
Dra
Baptista & Catalàn (2000)