> It is said that the maximum = output current of drive pin should > be more than the sum of all input pi= n driven. You should consider the above to be the absolute minimum drive capability, below which your circuit has no chance of ever working. If the drive strength is less than this, then your signals won't reach valid logic levels at your inputs even if you wait forever for all transient effects to die down. As you already noted, for CMOS inputs, the desired output current to support reasonable switching (transient response) needs to be more than given by the above statement. There was a time, and there were logic families, where you had to pay close attention to the static (stable phase) input currents and simply make sure the output had enough current capability to drive them. This was sometimes the situation with old TTL (almost never used in new designs anymore), where one output could drive as many as (say) eight standard input loads, and you could almost ignore the transient effects because traces were short and gate delays were in the tens of nanoseconds, so it wasn't a big deal to wait several more nanoseconds for a non-optimum transient response. Today, when every nanosecond matters, you can't ignore the transient response, so you need to choose your output drive strengths to give you clean switching, which has nothing to do with CMOS input currents. Regards, Andy ------------------------------------------------------------------ To unsubscribe from si-list: si-list-request@xxxxxxxxxxxxx with 'unsubscribe' in the Subject field or to administer your membership from a web page, go to: //www.freelists.org/webpage/si-list For help: si-list-request@xxxxxxxxxxxxx with 'help' in the Subject field List FAQ wiki page is located at: http://si-list.org/wiki/wiki.pl?Si-List_FAQ List technical documents are available at: http://www.si-list.org List archives are viewable at: //www.freelists.org/archives/si-list or at our remote archives: http://groups.yahoo.com/group/si-list/messages Old (prior to June 6, 2001) list archives are viewable at: http://www.qsl.net/wb6tpu