VISUAL-VESTIBULAR INTERACTION IN HUMANS DURING ACTIVE … · data on the effect of active as...
Transcript of VISUAL-VESTIBULAR INTERACTION IN HUMANS DURING ACTIVE … · data on the effect of active as...
Journal of Vestibular Research, Vol. 3, pp. 101-114, 1993 Printed In the USA. All rights reserved.
0957-4271/93 $6.00 + .00 Copyright © 1993 Pergamon Press Ltd.
VISUAL-VESTIBULAR INTERACTION IN HUMANS DURING ACTIVE AND PASSIVE, VERTICAL HEAD MOVEMENT
Joseph L. Derner, MD, PhD , * t John G. Oas, MD, t and Robert W. Balah, Mot
*Jules Stein Eye Institute and tDepartment of Neurology, University of California at Los Angeles Reprint address: Joseph L. Derner, M.D., Ph.D., Jules Stein Eye Institute, Comprehensive Division ,
100 Stein Plaza, UCLA, Los Angeles, CA 90024-7002
o Abstract - We studied visual-vestibular interaction (VVn in 9 normal human subjects using active and passive vertical head rotations. Gain and phase of the vertical vestibulo-ocular reflex (VOR) and visually enhanced vestibulo-ocular reflex (VVOR) were measured for single frequency sinusoidal motion, as well as for sinusoidal motion of continuously increasing frequency, over the range of 0.4 to 4.0 Hz. In addition to measurement of VVOR during normal vision, telescopic spectacles having a magnification of 1.9x were used to challenge VVI to facilitate measurement of visual enhancement of VOR gain. In the mid.frequency range (1.6 to 2.4 Hz), the active VOR exhibited gain closer to compensatory than did the passive VOR; at other frequencies, active and passive VOR gains were similar. VVOR gain during normal vision was compensatory for both active and passive motion throughout the frequency range tested. VVOR gain with 1.9x telescopic spectacles was greater than VOR gain at all frequencies tested, including up to 3.2 Hz for passive head movements, and up to 4.0 Hz for active head movement. However, gain enhancement with telescopic spectacles was consistently greater during active than during passive head movement. Phase errors for the VOR and VVOR were smaJ[ under all testing conditions. AIthougt. active VOR and: VVOR were directionall~'
symmetrical, gain of upward slow phases differed from that of downward slow phases for passive VOR and VVOR in a manner depending on rotational frequency. For both active and passive testing, gain and phase values obtained during swept frequency rotations were similar to those obtained
Presented at the Society for Neuroscience Annual Meeting, New Orleans, Louisiana, November 12, 1991.
during single frequency sinusoidal testing. These data indicate that VVI can enhance gain of the passive vertical VOR even at frequencies above what is usually considered to be the upper limit of visual pursuit tracking. The additional enhancement observed during active head movements at these bigh frequences is attributable to use of efference copy of the skeletal motor command to neck musculature.
o Keywords - active head movement; passive head movement; vertical, visual-vestibular interaction.
Introduction
A large body of data indicates that the horizontal (1-4) and vertical (4-6) eye movements produced by the vestibulo-ocular reflex (VOR) imperfectly compensate for passively imposed head movements. Perfect compensation would imply that VOR gain (eye velocity divided by head velocity) be equal to 1.0, indicating that I the reflexive eye velocity is equal and opposite to head velocity. The presence of normal vision is extremely effective in improving the precision 0: compensatory eye movements during pass!v::, wioie-body ::'o;.ation, wj:~ gair. at low frequencies usually within a fe~.' percent of the ideal value, both for horizontal (7,8) and vertical eye movements (6). However, even during normal vision, gain departs from unity for either high rotational frequencies (4,8) or, somewhat paradoxically, small rotational amplitudes (9). Since high frequency rotations of the head are present over a large range of amplitudes during normal standing
RECEIVED 15 June 1992; REVISED MANUSCRIPT RECEIVED 24 August 1992; ACCEPTED 26 August 1992.
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and ambulation (10), and since inappropriate gain leads to retinal image motion and consequent impairment in visual acuity (11,12), it is functionally advantageous for the ocular motor system to use other inputs to optimize gain.
Many everyday head rotations are selfgenerated, which allows the possibility that knowledge of the intended head movement could be used to optimize VOR gain. Indeed, nemons in the reticul:1r ~()r:naticn {!3, ld' 'l!ld
in the superior ,;oilicuius (15) that exhibit 4aze movement activity project to both oculomotor and head motor control centers. For actively generated movements up to 5.0 Hz, the horizontal VOR has a gain of unity, unlike during passive movement (16). However, Skavenski and collaborators studied both small horizontal and vertical, active and passive head movements over a broad frequency spectrum and found that normal vision increased gain from 0.65 in darkness to a maximum of only 0.90, and then only at frequencies below 3.0 Hz (9). These differences are difficult to interpret, partly because the VOR is normally close to compensatory and because of the small amount of gain enhancement required by normal vision. There is a paucity of data on the effect of active as compared with passive head movement on visual-vestibular interaction (VVI) , particularly for vertical movement.
The literature would suggest that the visual contribution to gain enhancement should be limited to relatively low frequencies in the physiologic range. Effective horizontal (17) and vertical (6) pursuit tracking are commonly said to be limited to frequencies below about 2 Hz, while the spectrum of physiologic head movements during standing and walking extends to appreciably greater frequencies (4,10). This limitation on vertical tracking would suggest that other mechanisms besides pursuit might make important contributions to VVI at high frequencies.
Telescopic spectacles afford an improved opportunity to study enhancement of VOR gain by vision. These devices are telescopes having magnification from around 2x to 8x
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mounted in spectacle frames for use as visual aids for patients suffering from ocular diseases (18). Telescopic spectacles magnify the visual effects of head motion in proportion to their optical power, and thus require compensatory eye movements with gain substantially greater than the ordinary ideal value of unity during normal vision (7). Magnification permits the gain-enhancing effect of vision to be more easily demonstrated, even at its upward limit of frequency. The present investigation ~hl:s ~!TIployed telescopic spectacles as a challenge : 0 VVI and compared VVI during active vertical head movements with those during passive vertical head movements.
Materials and Methods
Subjects
Nine young adult, paid volunteers gave written informed consent to a protocol approved by the Human Subject Protection Committee. All underwent ophthalmological examination by the author, verifying visual acuities in each eye correctable to 20120 or better . Average age of subjects was 30.2 ± 6.8 years (mean ± standard deviation, SO, range 19 to 39); there were 6 women and 3 men. During experiments, the comfort of subjects was monitored using an intercom and closed circuit television.
Apparatus
The host computer for these experiments was a Macintosh II (Apple Computer, Cupertino, CA) equipped with analog-to-digital converter (ADC), digital-to-analog converter (DAC), and direct memory access devices (National Instruments, Austin, TX). Custom software was written for these experiments using the Lab View software package (National Instruments). Sampling was at 200 Hz for stimulus frequencies below 1.0 Hz, and 400 Hz for greater stimulus frequencies. Digitizer sensitivity was increased up to 8-fold accord-
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ing to stimulus amplitude, increasing the effective performance of the ADC to 15 bits as necessary.
Subjects were seated in a custom fabricated swing rotator having a horizontal interaural axis. Their heads were firmly strapped to a headrest on the rotator, and their torsos and extremities were comfortably secured to the rotator using harnesses and belts. The rotator was driven by a servomotor (l08 ft-lb, 4.5 kW, Inland Motors, Radford, VA) controlled by a computer via a DAC. This permitted sinusoidal rotation of the subject's head and body at peak velocities of up to 40° to 75°/s, depending on subject weight and body habitus. Swing rotator position was registered by a precision potentiometer. Pairs of magnetic field generator coils 1 m in diameter were mounted on the swing rotator to permit measurement of horizontal and vertical eye and head position using the magnetic search coil technique (19). Subjects wore a headband to which was attached a search coil for the measurement of head position relative to the swing rotator, since decoupling of head, body, and swing motion often occurred at high frequencies despite restraints. The signal from the head coil was used to compensate for decoupling, so that corrected eye-in-head and head-in-space measurements were analyzed. The mechanical properties of the swing rotator depended upon loading by individual subjects, particularly with respect to weight and weight distribution. Many subjects' bodies exhibited mechanical resonances within the frequency range tested. Due to motor torque limitations in control of the swing rotator, as well as decoupling of the head from the rotator. it was impossible to precisely comroi head velocity. Data are reported here at nominal velocities of the swing rotator, but gains were always computed using measured head velocities. Generally, head velocities were close to nominal at 0.8 Hz, exceeded nominal from 1.2 to 2.0 Hz, and declined to less than nominal at higher frequencies. Observed gain values were not strongly dependent upon variations in head velocity within the range of head velocities employed.
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For active head rotations, subjects were trained to make sinusoidal vertical head movements in synchrony with the pitch of an audible tone presented via a loudspeaker. The tone was provided by a loudspeaker driven by a voltage controlled oscillator under the control of a computer via a DAC. Head movements were recorded using a search coil attached to a headband, and subjects remained seated in the locked swing rotator with head restraints removed. During training, head position and velocity were monitored in real time on a polygraph, and verbal feedback was given to subjects regarding the amplitude, frequency, and distortion of their head movements. With such feedback, most subjects learned to make sinusoidal head movements of the correct frequency and appropriate velocity amplitude after less than 10 min of training. The lowest frequencies were most difficult to produce without distortion, and maximum frequencies varied from subject to subject. Single frequency testing was generally performed at a constant velocity amplitude in the range of 40° to 1000/s, at the following approximate single frequencies: 0.5, 1.0, 1.6, 2.0,2.4,3.0, and 4.0 Hz. In each case, the actual frequency achieved in the trial was verified by Fourier analysis. Not every subject achieved every frequency, and some were unable to achieve 4.0 Hz. Some subjects also made active head movements of constant frequency, but progressively increasing velocity amplitude, from 30° to 150°/5. Active frequency sweeps were also made using constant velocity amplitude, from 0.4 to 4.0 Hz over 20 to 25 seconds.
The apparatus was located in a roOlT. tha~ couie. be made to:aI!y dark; i; faced c; gra~ '
waH locatee! 3 m from Ine subject's eyes. ro, VVOR testing, the wall was illuminated with standard fluorescent lighting to a centralluminance of 50 Cd/m2 • On the wall directly in front of the subjects was a small cross flanked by 4 red bars extending its arms, serving as the central fixation target. Four other crosses flanked the central target at 10° horizontal and vertical eccentricity from it, serving as horizontal and vertical calibration targets. The
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remainder of the central 10° of the wall facing the subjects was filled by concentric diamonds comprised of diagonal stripes spaced about 2 ° apart.
Measurement Conditions
Rotational stimuli consisted of trains of approximately 8 cycles of single frequency sinusoids, as well as trains of sinusoids I)f ~ontinuously inc:-easing ~requenc:, over a ;ogarithmic progression. For passive rotations, the command to the servomotor was set for a constant velocity amplitude of 300/s, and the following single frequencies were tested: 0.8, 1.2, 1.6, 2.0, 2.4, and 3.2 Hz. The passive frequency sweeps also had a constant nominal velocity amplitude of 300/s and a frequency increasing in continuous, logarithmic fashion over 20 seconds, from 0.4 to 3.2 Hz. Actual velocity amplitudes varied somewhat with the size and weight of the subject, and generally were less than nominal above 2.4 Hz.
Unaided visual-vestibulo-ocular reflex (1 x VVOR condition) testing was performed in normal room illumination with instructions to the subject to ftxate the central target directly ahead. Magnified VVOR testing was performed during wearing of 1.9x binocular telescopic spectacles having a field diameter of -16.8°, with instruction to attend to visual details on the wall ahead. The visual field peripheral to the telescopes was occluded. The VOR was tested in total darkness with instructions to ftxate the remembered central ftxation target on the wall ahead.
Eye and Head Movement Measurement
Vertical eye position was measured using the magnetic search coil technique, with the scleral search coil contact lens (Skalar Medical, Delft, The Netherlands) (20). Topical proparacaine 0.51170 was applied to the eye before insertion of the search coil contact lens, and the lens was removed within 30 minutes. Calibration was obtained for vertical saccades to targets located at 10° eccentricity from the pri-
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mary position. True head position in space was taken as the sum of swing rotator position plus head position relative to the swing rotator, thus compensating for any possible decoupling of the head from the rotator. To calibrate the sensitivity of the search coil on the head, the subject was instructed to fixate a target at the end of a 25-cm rigid rod held tightly in the teeth, as head position was changed in roughly 10° increments about pri:nar~1 ~osition. Since the sensitivity of the searc!1 -:oil on the eye had 'Jeen previously calibrated, the change head position was thus calibrated against the search coil on the eye. Eye, head, target, and chair rotator position data were displayed on a polygraph, with electronic differentiation for real time monitoring of velocities. Data were recorded in pulse code modulated analog format on magnetic tape for possible later editing, and were digitally sampled and stored to hard disc memory.
Data Analysis
Data were automatically analyzed using custom software under the Lab View package. All sampled channels were digitally low pass filtered (6 pole Butterworth, 0 to 42 Hz) and differentiated. Large quick phases and saccades were removed using velocity and duration criteria. Cross spectral analysis of eye compared with head velocity was then performed to determine the phase shift of the eye velocity response. After correction for phase, a linear regression of eye velocity against head velocity was obtained, and data points found to be statistical outliers from this ftt were also excluded as quick phases. Separate regressions were performed for the upward and downward directions, and the slopes so determined were taken to be the gains in each direction. The direction of gain is considered to be that of the slow phase response. After removal of quick phases, the remaining slow phase data points were fit cycle-by-cycle by least squares to a sinusoidal equation. Head velocity, eye velocity, phase, and gain (eye velocity/ head velocity) were computed for each cycle, and outlying cycles were automatically ex-
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eluded using a statistical criterion previously described to be effective for the removal of low gain artifacts (3). Points removed as quick phases and artifacts were then replaced by velocity values computed from the linear regressions, phase shifts, and instantaneously measured head velocities. Fourier spectral analysis was repeated to compute gain and phase at each of a range of frequencies. Phase lags were taken to be negative, while leads were taken to be positive. An ideal phase of 180° was taken as implicit for the VOR and VVOR, and reported phase values are relative to this. Values obtained by Fourier analysis were considered reliable only if the coherence at the single frequency in question exceeded 0.80; a coherence of 0.96 or greater was required for frequency sweeps. Typical values of coherence for single frequency VOR and VVOR testing exceeded 0.98. Since relatively few data are obtained at anyone frequency for sweep testing, higher coherence values were required to assure reliability; typically this affected only scattered and extreme frequencies in the spectrum for VOR and VVOR.
In order to correct for calibration errors inherent in the derivation of passive gains from eye, head, and chair position, 1 x VVOR gain at 0.8 Hz as computed by Fourier analysis was assumed to be the ideal value of 1.0. "For each individual subject, all other measurements of passive VOR and VVOR gain were normalized against 1 x VVOR gain at 0.8 Hz. No normalization was performed for active head head rotations.
Results
Single Frequency RotationsGain and Phase
For both active and passive vertical head movements, normal and telescopically magnified vision were effective in enhancing VOR performance. Under all viewing conditions, eye movements during passive rotations were opposite the direction of head movement, having slight phase variations as described below. Trials conducted with active head veloc-
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ities varying over the range of 30° to 1500/s demonstrated that VOR and VVOR gain were independent of peak head velocity.
Gain for the VOR was typically less than 1.0 for both passive and active head rotations, while gain during normal viewing (1 x) was almost perfectly compensatory. During 1.9 x viewing, gain exceeded 1.0 at lower frequencies and declined at higher frequencies, but gain enhancement was greater during active head rotations than during passive head rotations for all frequencies tested. Typical data illustrating this effect for single frequency rotation at 1.2 Hz are shown in Figure 1, which compares active and passive VOR responses with active and passive VVOR responses during l.9x viewing. Pooled gain data of all subjects obtained using Fourier analysis are plotted against frequency in Figures 2 through 4. Figure 2 illustrates that VOR gain during passive rotations was less than during active rotations between 1.2 and 2.4 Hz; within this frequency range, the active VOR was almost perfectly compensatory. Figure 3 illustrates that 1 x VVOR gain was essentially independent of frequency for both passive and active head rotations. The slight differences between gains obtained under the two rotational conditions could easily be attributable to variations in calibration of measurements, but all values closely approximate the ideal value of 1.0. Figure 4 illustrates the marked increase in VVOR gain produced by the wearing of 1.9x telescopic spectacles for both passive and active rotations. There was a trend toward greater gains during active head rotations, which was statistically significant (P < 0.01 two-tailed t:es~1 a: :.0 and :.4 !iz. Gain enhancemen~ during magnified vision occurred even at the highest frequencies tested for both types of rotations.
Phase values during passive and active head rotations are also illustrated in Figure 5. Under all viewing conditions, there was a trend toward phase lead (positive phase) below about 1.5 Hz, often with a slight phase lag for greater frequencies. However, phase errors were uniformly less than 5° and were independent of whether rotations were passively or actively induced. Phase compensation of the
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Active VOR
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Figure 4. VVOR gain during viewing with 1.9x telescopic spectacles in 9 subjects tested at multiple single frequencies during passive and active head rotations. Gain enhancement was greatest at low frequencies and was greater during active than during passive head rotations.
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VOR and VVOR was thus always essentially ideal.
Single Frequency RotationsDirectional Symmetry
Directional symmetry of the VOR and VVOR responses were evaluated under all testing conditions using phase-corrected Un~3.r ;-eg:.-essicrrs of ~~re '/e!oc:!~, :lgainst head. 're:oC:ty . These jara are ;Jiotted in Figure 5. :n general, pooled responses of multiple subjects during active rotations were directionally symmetrical, and this was also typical of the responses of each individual subject. In contrast, VOR and VVOR responses during passive rotations occasionally exhibited directional asymmetries, but these were not always consistent over all frequencies. Significant directional asymmetries were observed in pooled gain data only for the VOR and 1 x VVOR, and
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only at some frequencies. Figure 6A illustrates that VOR gain for upward slow phases was significantly greater than for downward slow phases for passive rotations at 2.0 Hz (P < 0.01, two-tailed t-test), with a trend toward significance at both higher and lower frequencies. Figure 6B illustrates that 1 x VVOR gain was significantly greater for downward than for upward slow phases during passive rotations at 0.8 Hz, but was significantly greater for upward ,low phases from 1.6 to 2.4 Hz. Figure 5C :llustrates :hat 1.9x YVOR gain exhibited no significant directional asymmetries for either active or passive head rotation.
Frequency Sweeps - Gain and Phase
Frequency sweep waveforms permit the frequency spectrum of head rotation to be studied more rapidly than sinusoidal testing
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Figure 6. Gain of 9 subjects analyzed for directional symmetry during passive and head rotations. Asterisk indicates statistical Significance of comparison of upward with downward gain for each type of rotation. (a) VOR was significantly asymmetrical only for passive rotation. (b) VVOR during normal viewing (1 x) was symmetrical during active head rotation, but exhibited a complex asymmetry during passive rotation. (c) VVOR with telescopic spectacles (1.9 x ) was directionally symmetrical for active and passive rotation. (Figure continues on facing page.)
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at discrete frequencies. Active and passive swept frequency testing was performed in all subjects for the VOR, 1 x VVOR, and 1.9x VVOR conditions. Gain and phase were ob-
tained using Fourier analysis, tabulated at the same frequencies used for single frequency testing. In general, gain and phase values obtained using frequency sweeps were quite sim-
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Har to those obtained using single frequency testing, and the small differences were not statistically significant. The exception to this generality was for the active VOR at 0.4 and 1.0 Hz, where gains for sweep testing were about 25070 greater than during single frequency testing (P < 0.01).
Discussion
VOR Gain Enhancemem in Darkness
The present data indicate that the vertical VOR is more precise during active than during passive head rotation. This was most evident at frequencies between 1.2 and 2.4 Hz, where VOR gain during active rotation was higher than during passive rotation, although gains were similar at lower and higher frequencies (Figure 2). Since the cervico-ocular reflex is insignificant in normal humans (21) and monkeys (22), the more precise VOR gain observed during active head movements could be explained through use of efference copy of the command to neck musculature to supplement the VOR. The anatomical substrate for such a sharing of efference copy is provided by neurons in reticular formation (13,14) and in the superior colliculus (15) encoding gaze movement signals that project to both oculomotor and cerivcal motor centers.
Directional Symmetry
The present study is the first to examine the issue of symmetry of the passive vertical VOR and VVOR at frequencies exceeding 1.6 Hz. In this study, the vertical VOR and VVOR were found to occasionally exhibit complicated directional asymmetries, depending upon frequency. Asymmetries in human vertical VOR gain have not been consistently observed by other investigators (5,6), although asymmetries have been found in individual subjects. The asymmetries were small and favored gain for downward slow phases below 1.0 Hz, but for upward slow phases from 1.6 to 2.4 Hz, so testing over a limited frequency
J . L. Derner et al
range might not disclose them or might yield inconsistent results. Asymmetries in VOR and VVOR gain observed during passive head rotation were corrected during active head rotation (Figure 6). In agreement with Ranalli and Sharpe, the present study found no directional asymmetry of the active vertical VOR or VVOR (23). The correction of asymmetry during active head movement is probably also due to the availability of efference copy of the t:eac! :ncvement ,:ommaP..d. Consequently. since :nest natural pitch head :novements of 3ubstantial velecity are likely IO oe self-generated. asymmetries in the vertical VOR and VVOR are unlikely to be of behavioral significance in normal humans.
Visual Enhancement of Vertical VOR Gain
The present data confirm previous findings that the vertical VVOR in the presence of normal vision is compensatory when tested both for active (2,5) and passive (6) head movements, despite considerable variations in VOR gain in darkness. This VVI is appropriate, but the amount of gain change required is small and not as challenging as that required during the wearing of telescopic spectacles. The present data also indicate that during passive, predictable vertical head movements considerable VVI occurs with telescopic spectacles up to frequencies of at least 2.0 Hz, and that phase is compensatory. For active head movements, VVI with telescopic spectacles had an even broader spectrum, being significant at all frequencies tested, even up to the highest frequencies subjects could voluntarily achieve. There was a consistent trend for VVOR gain with telescopic spectacles to be greater during active than passive rotations, reaching statistical significance at 2.0 and 2.4 Hz. Although predictive mechanisms have been demonstrated to contribute to gain enhancement during head motion with telescopic spectacles (24), the active and passive head movements studied here were equally predictable. It is likely that the superior VVI observed during active head movements is due to use of effer-
Active and Passive Visual-Vestibular Interaction
ence copy of the skeletal muscle command to the neck musculature. Efference copy during active head movements permits precise estimation of speed and timing, and probably accounts for the superior gain enhancement with telesopic spectacles observed during active as opposed to passive head movements (16). This performance may be further influenced by anticipatory intent (25).
High-Frequency VVI
Baloh and colleagues have found that vertical pursuit exhibits substantially declining gain as frequency increases toward 1.6 Hz (6). Such observations have led others to the conclusion that normal vision (26) and other extra vestibular influences have negligible effects on the VOR at frequencies above 2.0 Hz (16). However, other data indicate that if target acceleration is not excessive, pursuit at reduced gain does occur at high frequencies (17). This sort of visual tracking contribution may explain the significant VVOR gain enhancement observed here at frequencies above 2.0 Hz. Even though compensation is imperfect, and insufficient to match the magnification of powerful telescopic spectacles, VVI contributes in a functionally valuable manner beyond 2.0 Hz, and presumably throughout the physiologic range. This finding deserves consideration in the development of clinical tests of the active VOR.
Implications for Visual Function
Observing tha~ 1 x VVOR gair. du::-ing V~:-~" small amplitude head rotations is insufficient to prevent retinal image motion, Skavenski and colleagues have argued that VVOR gain is down-regulated to assure that a small amount of retinal image motion always occurs (9). This may be advantageous to prevent perceptual fading of stationary images, but retinal image slip velocities exceeding 2°/s markedly degrade visual acuity (11). Although significant VVI was observed here with telescopic spectacles during even at high frequencies, it
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should be stressed in the present case that the highest observed VVOR gains with telescopic spectacles were always less than the ideal values equal to telescope magnification, and were comparable to those measured during a visual acuity task with telescopic spectacles where acuity was degraded by motion (11). This implies that retinal images are unstable during these head movements with telescopic spectacles, and that this instability is functionally disadvantageous, probably reflecting limitations in the ocular motor system.
Swept Frequency Testing
As opposed to multiple cycles at each of several discrete frequencies, continuously increasing stimulus frequency over a short time interval represents one way of reducing the time required to test rotational VOR and VVOR performance over a spectrum of frequencies (16). While the swept frequency approach suffers from the disadvantage. of having relatively little stimulus energy at any given frequency, the present data indicate that resulting gain and phase values are nonetheless quite close to those obtained using discrete frequency testing in normal subjects. The only exception is for testing at "frequencies below 1.0 Hz, where even trained subjects experience difficulty making undistorted sinusoidal head movements. Use of swept frequency stimuli at frequencies above 1.0 Hz would thus permit essentially the same data to be obtained in about one-tenth the time required for discrete frequency testing, an advantage that might be of considerable value in clinical settings. now~" e: " the vaiue of swept fiequency testing in subjects with vestibular disease remains to be demonstrated.
Acknowledgments- The authors thank Laura A. Hovis for assisting with recruitment and testing of subjects, and Douglas Wong and James Li for hardware and software support. This work was supported by U.S. Public Health Service grants EY-08656 and NS-10940. JLD is a Research to Prevent Blindness William and Mary Greve International Research Scholar.
114 J. L. Derner et al
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