The neutrino oscillation parameters are taken from the analysis of various neutrino ex- periments [17, 18], except for θ$_{13}$ [19], as sin $^{2}$2 θ$_{12}$ = 0 . 84 , sin $^{2}$2 θ$_{23}$ = 1 . 00 , (3) Δ m 2 12 = 8 . 1 × 10 − $^{5}$eV$^{2}$, | Δ m 2 13 | = 2 . 2 × 10 − $^{3}$eV$^{2}$. (4)    φ SN ν$_{e}$ ( E$_{ν}$ ) φ SN ¯ ν$_{e}$ ( E$_{ν}$ ) φ SN ν$_{x}$ ( E$_{ν}$ )    =    P ( E$_{ν}$ ) 0 1 − P ( E$_{ν}$ ) 0 ¯ P ( E$_{ν}$ ) 1 − ¯ P ( E$_{ν}$ ) 1 − P ( E$_{ν}$ ) 1 − ¯ P ( E$_{ν}$ ) 2 + P ( E$_{ν}$ ) + ¯ P ( E$_{ν}$ )       φ org ν$_{e}$ ( E$_{ν}$ ) φ org ¯ ν$_{e}$ ( E$_{ν}$ ) φ org ν$_{x}$ ( E$_{ν}$ )   $^{,}$ (5) n$_{e,res}$ ≡ 1 $_{2}$√$_{2}$$_{G}$$_{F}$ Δ m 2 E$_{ν}$ cos 2 θ, (6) γ ≡ Δ m 2 2 E$_{ν}$ sin $^{2}$2 θ cos 2 θ n$_{e,res}$ | dn$_{e}$ dr | . (7) and We calculate the neutrino survival probabilities for both normal (Δ m 2 13 > 0) and inverted (Δ m 2 13 < 0) mass hierarchies for four cases of sin $^{2}$2 θ$_{13}$ value: sin $^{2}$2 θ$_{13}$ = 10 − $^{2}$, 10 − $^{3}$, 10 − 4 and 10 − $^{5}$. The energy spectra of the neutrinos passed through the exploding supernova, φ SN ν ( E$_{ν}$ ), are obtained from the spectra of the neutrino emitted from the neutrino sphere, φ org ν ( E$_{ν}$ ), multiplied by the survival probability in accordance with the following equation, where φ$_{ν}$$_{x}$ ≡ 1 $_{4}$( φ$_{ν}$$_{µ}$ + φ$_{ν}$$_{τ}$ + φ$_{¯}$ ν$_{µ}$ + φ$_{¯}$ $_{ν$_{τ}$}$), and P and ¯ P are survival probabilities of ν$_{e}$ and ¯ ν$_{e}$ , respectively. Neutrinos change largely their flavors at resonances of neutrino oscillations. There are two resonances for supernova neutrinos (e.g., [24]). The resonance points of higher and lower electron number densities correspond to H-resonance and L-resonance, respectively. The electron number density at the resonance point is written as where Δ m 2 and θ correspond to | Δ m 2 13 | and θ$_{13}$ at H-resonance and to Δ m 2 12 and θ$_{12}$ at L-resonance, respectively. The flavor change at a resonance strongly depends on adiabaticity of the resonance. When the resonance is adiabatic, large flavor change occurs. The neutrino adiabaticity is estimated by γ , 8