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The detection of galactic supernova (SN) neutrinos represents one of thefuture frontiers of low-energy neutrino physics and astrophysics. The neutroncoherence of neutral currents (NC) allows quite large cross sections in thecase of neutron rich targets, which can be exploited in detecting earth and skyneutrinos by measuring nuclear recoils. They are relatively cheap and easy tomaintain. The relevant NC cross sections are not dependent on flavorconversions and, thus, their measurement will provide useful information aboutthe neutrino source. In particular they will yield information about theprimary neutrino fluxes and perhaps about the spectrum after flavor conversionsin neutrino sphere.They might also provide some clues about the neutrino masshierarchy. The advantages of large gaseous low threshold and high resolutiondetectors with time projection counters (TPC) are discussed.

Neutral Current Coherent Cross Sections -- Implications on Gaseous Spherical TPC's for detecting SN and Earth neutrinos