Superconducting Gravity Gradiometers (SGGs)

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Superconducting Gravity Gradiometers (SGGs) Three models of SGGs with increasing complexity and sensitivity have been developed at Maryland [Chan et al., 1987; Moody et al., 2002]. The Model II SGG has reached an operating sensitivity of 0.02 E Hz -1/2 (1 E 1 Eötvös 10-9 s -2 ), three orders of magnitude improvement over the sensitivity achieved by room-temperature gradiometers. With such vastly improved sensitivity, the SGG finds useful application in geophysical measurements, oil and mineral prospecting, and inertial navigation. The great potential for practical application has inspired several groups around the world to develop similar instruments. At Maryland, a new SGG with improved linear acceleration rejection capability is under development. Basic Superconducting Accelerometer Figure 1 shows a superconducting accelerometer in its simplest form. The accelerometer consists of a superconducting proof mass, a superconducting sensing coil and a SQUID with input coil. A persistent current is stored in the loop formed by the sensing coil and the SQUID input coil. When the platform undergoes an acceleration, or equivalently, when a gravity signal is applied, the proof mass is displaced relative to the sensing coil, modulating its inductance through the Meissner effect. This induces a time-varying current in the loop to preserve flux quantization. The SQUID converts the induced current into an output voltage signal. Figure 1. Principle of a superconducting accelerometer.

In-line-Component SGG Figure 2 shows a component accelerometer of Model II SGG. The proof mass weighing 1.2 kg is suspended by a pair of diaphragm flexures with folded cantilevers. The entire structure is machined from niobium (Nb). Six identical accelerometers are mounted on six faces of a precision titanium (Ti) alloy cube, with the sensitive axes normal to the cube surfaces, to form a three-axis SGG (see Figure 3). Figure 4 is a schematic circuit diagram for each axis of the Model II SGG. The two proof Figure 2. Component accelerometer for Model II SGG. masses on opposite faces of the mounting cube are connected by a superconducting circuit to form a gradiometer. The proof masses are levitated against gravity by storing a persistent current I L in the loop formed by L L1 and L L2. Figure 3. Three-axis Model II SGG. The coils L S1 and L S2 are connected in parallel to a SQUID to form a sensing circuit. Each axis of the gradiometer has two circuits. In one circuit, we store the currents I S1 and I S2 with the same sense (as shown in Figure 4) and the SQUID detects the differential acceleration, or the gravity gradient. In the other circuit (not shown), we reverse the

I L R BS L t2 L S3 L B1 L L1 L S1 L S2 L L2 L B2 TEST MASS 1 L t1 R SP SQUID TEST MASS 2 direction of one of the currents, and the SQUID detects the commonmode motion. Signal differencing by means of persistent currents before detection assures excellent null stability of the device, which in turn improves the overall commonmode rejection. Further, the SQUID sees only a small differential signal, thereby reducing the dynamic-range requirement on the amplifier and signal-processing electronics. We adjust I S2 /I S1 to maximize the common-mode rejection. Although the component of the linear acceleration parallel to the sensitive axis can be rejected precisely by this current adjustment, components normal to the sensitive axis couple to the gradient output through misalignments of the sensitive axes. In the Model II SGG, all the misalignment angles are measured from the response of the gradiometer to accelerations applied in various directions. The results are then multiplied by the measured linear acceleration components and subtracted from the gradiometer outputs to achieve the residual commonmode balance [Moody et al., 1986]. The misalignments were about 10-4 rad. The residual balance improved the common-mode rejection to 10 7. The power spectral density of the intrinsic gradient noise of the SGG can be shown to be [Chan and Paik, 1987] S I S2 - I S1 I S1 I S2 R BP R SS Figure 4. Circuit diagram for each axis of Model II SGG R L I B1 I B2 2 8 0 0 ( f ) ( ), 2 kbt EA f m Q 2 where m, Q and T are the mass, quality factor and temperature of the proof mass, is the baseline of the gradiometer, is the electromechanical (1)

energy coupling constant of the transducer, is the energy coupling efficiency from the superconducting circuit to the SQUID, E A (f) is the input energy resolution of the SQUID, and f = /2 is the signal frequency. The numerical values of the gradiometer parameters are: m = 1.2 kg, = 0.19 m, 0 /2 = 10 Hz, Q = 10 6, T = 4.2 K, = = 0.25, E A (f) = [1 + (0.1 Hz)/f] 5 10-31 J Hz -1 below f 0.1 Hz (commercial dc SQUID). Equation (1) predicts a white-noise level of 2 10-3 E Hz -1/2. Below 0.1 Hz, a 1/f power noise should appear. Figure 5 shows the actual noise spectrum of the Model II SGG obtained in the laboratory. The whitenoise level corresponds to 0.02 E Hz -1/2, dominated by uncompensated angular acceleration noise. Below 0.1 Hz, a 1/f power noise appears, but with an amplitude an order of magnitude higher than expected from the SQUID noise. This excess lowfrequency noise is believed to come from a combination of temperature drift of the Figure 5. Noise spectrum of Model II SGG. instrument, which couples to the gradiometer through modulation of the penetration depth of the superconductor, and down-converted centrifugal acceleration noise. The demonstrated sensitivity of the SGG represents three orders of magnitude improvement over that of the conventional gravity gradiometers operated at room temperature. The sensitivity requirement of NASA s gravity mapping mission have prompted further innovations in technology, a superconducting negative spring [Parke et al., 1984]. This has led to the design of the Model III SGG with an intrinsic sensitivity of 10-4 E Hz -1/2.

Chan, H. A. and Paik, H. J. (1987), Physical Review D 35, 3551-3571. Chan, H. A., Moody, M. V., and Paik, H. J. (1987), Physical Review D 35, 3572-3597. Moody, M. V., Canavan, E. R., and Paik, H. J. (2002), Rev. Sci. Instrum. 73, 3957. Moody, M. V., Chan, H. A., and Paik, H. J. (1986), J. Appl. Phys. 60, 4308-4315. Parke, J. W. et al. (1984) in Proc. 10th International Cryogenic Engineering Conference, Butterworth, Surrey, D. H. Collan et al. (eds.), pp. 361-364.