reflow comments in modules/{webaudio,vr}

third_party/WebKit/Source/modules/webaudio/IIRDSPKernel.cpp

 // Copyright 2016 The Chromium Authors. All rights reserved.
 // Use of this source code is governed by a BSD-style license that can be
 // found in the LICENSE file.
 
 #include "modules/webaudio/IIRDSPKernel.h"
 
 #include "wtf/MathExtras.h"
 
 namespace blink {
 
@@ skipping 22 matching lines @@
   // Convert from frequency in Hz to normalized frequency (0 -> 1),
   // with 1 equal to the Nyquist frequency.
   for (int k = 0; k < nFrequencies; ++k)
     frequency[k] = clampTo<float>(frequencyHz[k] / nyquist);
 
   m_iir.getFrequencyResponse(nFrequencies, frequency.data(), magResponse,
                              phaseResponse);
 }
 
 double IIRDSPKernel::tailTime() const {
-  // TODO(rtoy): This is true mathematically (infinite impulse response), but perhaps it should be
-  // limited to a smaller value, possibly based on the actual filter coefficients.  To do that, we
-  // would probably need to find the pole, r, with largest magnitude and select some threshold,
-  // eps, such that |r|^n < eps for all n >= N.  N is then the tailTime for the filter.  If the
-  // the magnitude of r is greater than or equal to 1, the infinity is the right answer. (There is
-  // no constraint on the IIR filter that it be stable.)
+  // TODO(rtoy): This is true mathematically (infinite impulse response), but
+  // perhaps it should be limited to a smaller value, possibly based on the
+  // actual filter coefficients.  To do that, we would probably need to find the
+  // pole, r, with largest magnitude and select some threshold, eps, such that
+  // |r|^n < eps for all n >= N.  N is then the tailTime for the filter.  If the
+  // the magnitude of r is greater than or equal to 1, the infinity is the right
+  // answer. (There is no constraint on the IIR filter that it be stable.)
   return std::numeric_limits<double>::infinity();
 }
 
 double IIRDSPKernel::latencyTime() const {
   return 0;
 }
 
 }  // namespace blink