  Here we present a continuation of the work that was based on video
observations of the Tau Her 2022 outburst from the McDonald Observatory, Texas,
US. On the night of the maximum in 2022 we detected 626 individual Tau Her
meteors, for which we estimated photovisual magnitudes and analysed their
distribution on the sky to determine the radiant position in an innovative way.
The derived population index is $5.56 \pm 1.83$, while the radiant position for
the mid-time of the observations is: $\mathrm{RA} = 209.71 ^\circ \pm 1.01
^\circ$, $\mathrm{Dec} = 27.73 ^\circ \pm 0.07 ^\circ$. Both measurements are
in good agreement with other results in the literature, although our population
index seems to be higher than most of the published values. We speculate this
might be due to the higher sensitivity of our equipment to fainter meteors.
