time.Sleep(time.Second)
	}
	rx := float64(globalNetPerfRX.RXSample)
	delta := globalNetPerfRX.firstToDisconnect.Sub(globalNetPerfRX.lastToConnect)
	if delta < 0 {
		rx = 0
		errStr = "network disconnection issues detected"
	}

	globalNetPerfRX.Reset()
	return madmin.NetperfNodeResult{Endpoint: "", TX: r.n / uint64(duration.Seconds()), RX: uint64(rx / delta.Seconds()), Error: errStr}
}

	if err != nil {
		return errMalformedAuth
	}

	localTime := UTCNow()
	remoteTime := time.Unix(0, nanoTime)

	delta := remoteTime.Sub(localTime)
	if delta < 0 {
		delta *= -1
	}

	if delta > DefaultSkewTime {
		return errSkewedAuthTime
	}

	return nil
}

// IsAuthValid - To authenticate and verify the time difference.

	}

	msdosModified := msDosTimeToTime(f.ModifiedDate, f.ModifiedTime)
	f.Modified = msdosModified
	if !modified.IsZero() {
		f.Modified = modified.UTC()

		// If legacy MS-DOS timestamps are set, we can use the delta between
		// the legacy and extended versions to estimate timezone offset.
		//
		// A non-UTC timezone is always used (even if offset is zero).
		// Thus, FileHeader.Modified.Location() == time.UTC is useful for

## Breaking Changes to the API

*   `AdjustContrast` kernel deprecated, new kernel `AdjustContrastv2` takes and
    outputs float only. `adjust_contrast` now takes all data types.
*   `adjust_brightness`'s `delta` argument is now always assumed to be in
    `[0,1]` (as is the norm for images in floating point formats), independent
    of the data type of the input image.

#define SEL1 V7 #define CAR1 V8 #define CAR2 V9 #define TT0 V11 #define TT1 V12 #define T2 V13 // p256MulAsm Parameters #define X0 V0 #define X1 V1 #define Y0 V2 #define Y1 V3 #define T0 V4 #define T1 V5 #define PL V30 #define PH V31 /* * https://delta.cs.cinvestav.mx/~francisco/arith/julio.pdf "Software Implementation of the NIST Elliptic Curves Over Prime Fields" * * A = X₁×Z₂² * B = Y₁×Z₂³ * C = X₂×Z₁²-A * D = Y₂×Z₁³-B * X₃ = D² - 2A×C² - C³ * Y₃ = D×(A×C² - X₃) - B×C³ * Z₃ = Z₁×Z₂×C * * Three-operand...

#define SEL1 V7 #define CAR1 V8 #define CAR2 V9 #define TT0 V11 #define TT1 V12 #define T2 V13 // p256MulAsm Parameters #define X0 V0 #define X1 V1 #define Y0 V2 #define Y1 V3 #define T0 V4 #define T1 V5 #define PL V30 #define PH V31 /* * https://delta.cs.cinvestav.mx/~francisco/arith/julio.pdf "Software Implementation of the NIST Elliptic Curves Over Prime Fields" * * A = X₁×Z₂² * B = Y₁×Z₂³ * C = X₂×Z₁²-A * D = Y₂×Z₁³-B * X₃ = D² - 2A×C² - C³ * Y₃ = D×(A×C² - X₃) - B×C³ * Z₃ = Z₁×Z₂×C * * Three-operand...