  We discuss a scenario in which TeV neutrinos are produced during explosions
of Novae. It is argued that hadrons are accelerated to very high energies in
the inner part of a Nova wind, as a result of reconnection of the strong
magnetic field of a White Dwarf. Hadrons are expected to interact efficiently
with a dense matter of the wind, either already during the acceleration process
or during their advection with the equatorial wind. We calculate the neutrino
spectra, and estimate the muon neutrino event rates in the IceCube telescope,
in the case of a few Novae. In general, those event rates are unlikely to be
detected with the present neutrino detectors. However, for favourable location
of the observer, some neutrino events might be detected not only from the class
of Novae recently detected in the GeV $\gamma$-rays by the {\it Fermi}-LAT
telescope but also from novae not detected in $\gamma$-rays. The GeV
$\gamma$-ray emission observed from Novae cannot originate in terms of the
model discussed here, since protons are accelerated within a few stellar radii
of the White dwarf, i.e. in the region in which GeV $\gamma$-rays are expected
to be severely absorbed in the interactions with the radiation field and the
matter of the wind.
