Hi,
Can anyone tell me if they've measured any differences between the new and old SEAS W18-E001 drivers?
The new one is identifiable via the rubber boot over the magnet.
The old ones have the copper plated magnets.
In the older versions, there seems to be a droop between 1-3Khz. The droop is most noticable at 3KHz, right before the cone takes off and hits the stratosphere by 5KHz.
Also, has been a drift in the frequency (and intensity) of this breakup mode?
regards,
Thanh.
Can anyone tell me if they've measured any differences between the new and old SEAS W18-E001 drivers?
The new one is identifiable via the rubber boot over the magnet.
The old ones have the copper plated magnets.
In the older versions, there seems to be a droop between 1-3Khz. The droop is most noticable at 3KHz, right before the cone takes off and hits the stratosphere by 5KHz.
Also, has been a drift in the frequency (and intensity) of this breakup mode?
regards,
Thanh.
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