We briefly review the current status of standard oscillations of atmospheri
c neutrinos in schemes with two, three, and four flavor mixing. It is shown
that, although the pure nu (mu) --> nu (tau) channel provides an excellent
2 nu fit to the data, one cannot exclude, at present, the occurrence of ad
ditional sub-leading nu (mu) --> nu (e) oscillations (3 nu schemes) or of s
izable nu (mu) --> nu (s) oscillations (4 nu schemes). It is also shown tha
t the wide dynamical range of energy and pathlength probed by the Super-Kam
iokande experiment puts severe constraints on nonstandard explanations of t
he atmospheric neutrino data, with a few notable exceptions.