Left: spectrum of the IGW luminosity generated by the convective Reynolds stresses of the envelope for various frequencies σ and degrees ℓ. Middle: spectrum of the IGW luminosity at 0.05 R⊙ below the convective envelope for retrograde (left) and prograde (right) waves with various frequencies and degrees ℓ. Only the cases with m = ℓ (top) and m = 1 (bottom) are shown. Right: spectrum of the net luminosity at 0.05 R⊙ below the convective envelope for various frequencies and degrees ℓ (and m).
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