The full list for 2000 is available in an ASCII Test file.
The following is an extract to assist in the interpretation of the notes below.
#Final numerical order list for 2000 Race : Prepared 24-Mar-08 17:14:37
.........Start ........Barnes ...........ARA ........Finish
#NUM - COD - CLB
@PFR @TFR @PFR @TFR @PFR @TFR TDR
STA %PFS %TFS %PFS %TFS %PFS %TFS OTI
PRZ DFG DFR DFG DFR DFG DFR GRP
NPD $SEQ GMT $SEQ GMT $SEQ GMT .
TBW
#019 - ULO - University of London
@019 03:21.04 @019 11:09.89 @019 18:17.29 2
S.2 %019 03:21.04 %020 07:48.85 %018 07:07.40 1
V -1.07 0.51 -0.15 -6.16 1.24 5.66 3
$017 15:35:25.15 $015 15:38:46.19 $017 15:46:35.04 $016 15:53:42.44
+01:01.22
#020 - MBC2 - Molesey II
@015 03:19.70 @015 11:05.03 @016 18:11.10 5
%015 03:19.70 %013 07:45.33 %015 07:06.07 1
P 1.77 0.30 -1.01 -7.00 -0.74 6.71 2
$018 15:35:35.66 $016 15:38:55.36 $018 15:46:40.69 $017 15:53:46.76
+00:55.03
#021 - TYR1 - University of London Tyrian I
@035 03:25.39 @047 11:29.62 @038 18:39.95 30
%035 03:25.39 %054 08:04.23 %027 07:10.33 .
V -0.89 0.72 5.54 -0.59 -4.63 -0.12 3
$019 15:35:52.49 $017 15:39:17.88 $019 15:47:22.11 $019 15:54:32.44
+01:23.88
#022 - STA1 - Star I
@062 03:27.77 @053 11:31.94 @059 18:55.60 32
S.1 %062 03:27.77 %053 08:04.17 %082 07:23.66 3
JA -0.25 0.24 -3.73 -7.42 3.99 7.20 4
$020 15:36:01.48 $018 15:39:29.25 $021 15:47:33.42 $023 15:54:57.08
+01:39.53
#023 - LDR3 - Leander III
@034 03:25.23 @026 11:16.94 @024 18:24.40 16
%034 03:25.23 %023 07:51.71 %019 07:07.46 1
P 1.81 3.40 -0.33 -6.38 -1.46 2.99 3
$021 15:36:11.32 $019 15:39:36.55 $020 15:47:28.26 $020 15:54:35.72
+01:08.33
#024 - LEA1 - Lea I
@020 03:21.40 @025 11:14.98 @025 18:26.06 15
%020 03:21.40 %028 07:53.58 %032 07:11.08 2
P -2.33 -0.73 0.83 -5.22 1.51 5.97 3
$022 15:36:25.86 $020 15:39:47.26 $023 15:47:40.84 $022 15:54:51.92
+01:09.99
#025 - CRB1 - Crabtree I
@011 03:17.85 @010 10:58.46 @010 17:59.55 8
%011 03:17.85 %007 07:40.61 %006 07:01.09 2
.... etc
The following information is shown
The figure in (TDR) column indicates the total
deviation in rank position for the crew for the three parts of the race
when compared with its final position. If the crew maintained a steady
position for all three sections of the race, this 'TDR' would be zero.
A high 'TDR' indicates large change in position, which may be caused by
a crew blowing up, or by bad steering or a problem in some part of the
race.
The group (GRP) to which each crew is allocated
is fixed in half minute intervals from the time of the fastest crew over
the course. (Crews within 30 seconds of the winner are allocated to group
1, those between 30 seconds and one minute to group 2, and so on.)
The spread of the group numbers in the final order gives an overall
view of the variability of strength of crews from year to year, and also
indicate the fortunes of new entrants.
The two times given in ss.hh for each each location indicate the deviation
of the performance of the crew relative to all crews in the same half-minute
final-time grouping (DFG) and relative to all crews
in the race (DFR), for each section of the race.
This figure is obtained by multipying the crew's overall time by the average
proportion of the course time taken for each section of the race by all
crews in the same group GRP (for DFG)
and for all crews in the race (for DFR).
A positive variation indicates that the crew went slower than average
over the section, a negative score that it went faster.
NB - the total
deviation for each crew is zero, so these scores indicate relatively slow
and fast parts of the course for the crew, NOT overall speed.
It is interesting to note that weaker crews sometimes go quickly off
the start and near the finish, while the better crews perform relatively
better in the middle of the race.
The variability of performance of a particular crew over the three stages of the race can be seen by tracing its positions (PFS) at Barnes, ARA and the finish with a pair of lines drawn in the manner of a traditional bumps chart. A flat line indicates steady performance, while a steeply sloping line would indicate variation.
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