Temperature distribution in cylindrically symmetric coronal magnetic l
oops has been reinvestigated under various conditions: (a) loop with t
he pressure varying along the radial distance, and (b) loop with const
ant pressure, for cooler apex loops and hotter apex loops. This work i
s reinvestigation of our previous work published in Astrophysics and S
pace Science (Chandra and Prasad, 1993b).