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    Vibrophonocardiograph Patent

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    Vibrophonocardiograph comprising low weight and small volume piezoelectric microphone with amplifier having high imput impedance for high sensitivity and low frequency respons

    Angular Power Spectrum of the Microwave Background Anisotropy seen by the COBE Differential Microwave Radiometer

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    The angular power spectrum estimator developed by Peebles (1973) and Hauser & Peebles (1973) has been modified and applied to the 2 year maps produced by the COBE DMR. The power spectrum of the real sky has been compared to the power spectra of a large number of simulated random skies produced with noise equal to the observed noise and primordial density fluctuation power spectra of power law form, with P(k)knP(k) \propto k^n. Within the limited range of spatial scales covered by the COBE DMR, corresponding to spherical harmonic indices 3 \leq \ell \lsim 30, the best fitting value of the spectral index is n=1.250.45+0.4n = 1.25^{+0.4}_{-0.45} with the Harrison-Zeldovich value n=1n = 1 approximately 0.5σ\sigma below the best fit. For 3 \leq \ell \lsim 19, the best fit is n=1.460.44+0.39n = 1.46^{+0.39}_{-0.44}. Comparing the COBE DMR ΔT/T\Delta T/T at small \ell to the ΔT/T\Delta T/T at 50\ell \approx 50 from degree scale anisotropy experiments gives a smaller range of acceptable spectral indices which includes n=1n = 1.Comment: 22 pages of LaTex using aaspp.sty and epsf.sty with appended Postscript figures, COBE Preprint 94-0
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