Greetings everyone! Given the interest in TVN's direct observation of a 138.8 MPH peak wind speed in the
Aurora, NE tornado on June 17th, I would like to contribute some background information to the ongoing discussion of this intercept.
The instrument used to measure wind speed and direction on Reed's vehicle (the "
SRV") is an R. M. Young
marine model wind monitor. This unit is, for all intents and purposes, equivalent to the mechanical R. M. Young wind monitors pressed into operation by the
Oklahoma Mesonet,
West Texas Mesonet, and
mobile mesonet vehicle probes of Vortex/V2, among many other scientific projects, meteorological networks, and chasers alike. As
specified by R. M. Young, this wind monitor is accurate to within +/- 0.3 m/s (~0.7 MPH) for wind speeds lower than 30 m/s (~67 MPH) and +/- 1% for wind speeds exceeding 30 m/s up to 100 m/s (~224 MPH). The SRV features an instrumentation mast, extending approximately 2.5 feet above rooftop level, to which the wind monitor is mounted. Presently, the magnitude of any error introduced as a consequence of the wind monitor's location in relation to the body of the vehicle is not well known. Proper siting of the wind monitor, including its position relative to the vehicle's slip-stream, is an issue of consequence to be sure. We have speculated about a handful of potential complications which could conceivably lead to both low and high biases in wind speed measurements under various circumstances. Given the inherent scientific import of in situ measurements taken near ground level in tornadic circulations, sources of potentially significant error in this dataset will certainly need to be formally identified and, if at all possible, adequately quantified before inclusion in literature.
Specifically concerning the 138.8 MPH gust, that measurement was the maximum 1 second average wind speed recorded while the SRV was deployed in a stationary position during the Aurora intercept. The direction of this wind gust was perpendicular to the vehicle from left (driver's side) to right. As is evident in the
video (near the 2:08 mark) recorded by the SRV's rooftop "bubble cam" and
footage (near the 3:05 mark) from Darin Brunin and Dick McGowan, the vehicle was impacted by a rather vigorous suction vortex at a time coincident with our observation of the 138.8 MPH wind velocity. The front driver's side tempered glass inner window shattered at that moment. Outside an 18 second window of time during which the suction vortex/vortices traversed the SRV, 1 second average wind speeds were entirely lower than 100 MPH.
Insomuch that the SRV wind observations have been referenced in discussions heretofore of the EF scale, note that the wind relationships in the EF scale are based upon 3 second average wind speeds (see
TTU,
SPC). The peak 3 second average wind speed measured by TVN during the Aurora intercept was 122.4 MPH. That 122.4 MPH 3 second average wind velocity integrates the 138.8 MPH peak 1 second average velocity with two temporally adjacent 1 second average velocities of 131.1 MPH and 97.3 MPH. Adding to the sentiment expressed in earlier posts by other members, generally speaking, I would caution that it is inadvisable to draw significant parallels between the SRV's peak wind measurement, a measurement over a limited temporal and spatial extent, and either the tornado's overall EF scale rating (which is assessed at the location of most significant damage -- a point disparate in both time and space from the SRV's peak wind observation) or visual impressions of tornado intensity.
In all likelihood neither the 138.8 MPH 1 second nor 122.4 MPH 3 second average peak wind speed observations are wholly representative of the horizontal velocities in the Aurora tornado's entire core flow region at the time those measurements were taken. Nevertheless, it seems genuinely reasonable that those measurements are substantially representative of the smaller scale suction vortex we sampled within the larger circulation of the maturing Aurora tornado.
The Aurora tornado and its parent supercell certainly exhibited a fascinating evolutionary progression! In addition to wind monitor measurements of horizontal flow, the
CLOVER project was in operation during the intercept and enabled us to sample vertical velocities within the tornadic circulation. The CLOVER data is still being analyzed at this time, and we believe that a good deal of additional knowledge stands to be gleaned from this event.