Streamer breakdown of long (> 10 cm) air gaps under normal conditions
is studied numerically. It is shown that streamer breakdown requires a
n average electric field of 25 kV/cm. The time during which streamer b
reakdown develops is primarily determined by the stage of quasi-unifor
m heating of a streamer channel, which begins after the gap is bridged
by the streamer and the return wave of the enhanced electric field is
damped. This time is less than a hundred nanoseconds; and, for stream
er breakdown to develop in a gap with a strongly nonuniform electric f
ield, the voltage pulse should have a sufficiently sharp front. It is
shown that such breakdowns can occur only in the submicrosecond range.
The main microscopic processes responsible for the composition and te
mporal evolution of a streamer plasma at different stages of the disch
arge are revealed. The results of calculations agree qualitatively wit
h experimental data on nanosecond breakdown.