| Entry | Date | Title | Site | Author | #Graphics |
|---|---|---|---|---|---|
| 1 | Thu 29-Apr-2004 | Logbook created | none | aster | |
| 2 | Thu 29-Apr-2004 | System up | marshall | maclean | |
| 3 | Thu 29-Apr-2004 | Sonic status in rain | marshall | maclean | |
| 4 | Thu 29-Apr-2004 | Marshall flow distortion test | marshall | horst | |
| 5 | Thu 29-Apr-2004 | sonic ?? output | marshall | maclean | |
| 6 | Thu 29-Apr-2004 | CSAT wind tunnel test | marshall | horst | |
| 7 | Thu 29-Apr-2004 | sonic dids | marshall | horst | |
| 8 | Mon 03-May-2004 | Data system sampling | marshall | maclean | 2 |
| 9 | Mon 03-May-2004 | Fixed duplicate channel number 203 in prep.config | marshall | horst | |
| 10 | Tue 04-May-2004 | sonic tilts | marshall | horst | |
| 11 | Fri 07-May-2004 | Raised data-system box | marshall | maclean | |
| 12 | Mon 10-May-2004 | chemistry trailers | marshall | horst | |
| 13 | Mon 10-May-2004 | Sonic azimuths | marshall | horst | |
| 14 | Mon 10-May-2004 | current results | marshall | horst | |
| 15 | Wed 12-May-2004 | height error analysis | marshall | horst | |
| 16 | Fri 14-May-2004 | shut down Marshall | marshall | horst | |
| 17 | Mon 17-May-2004 | Final results | marshall | horst |
initial log file /home/isff/aster/projects/OHATS/logbook/tklog.log created by USER aster
Sonics on goal-post, data system up, network operational
3 sonics, channel 201,205,206 (all of which have firmware rev 3.0.a) are having problems in the rain, reporting >Consec hopped exceeded Here are the firmware rev levels for each channel: 4.0s: 200,204,207 4.0r: 203 3.0a: 201,202,205,206 4.0s is apparently the rain firmware upgrade. These sonics also have nylon "water wicks" on each transducer. However sonic on channel 207 is missing one of the upper wicks. Channel 205 is having the most difficulties, and has needed to be restarted several times. To restart it use the "D" command from rserial -A ragwort 205 rserial -A ragwort 205 Acq sigs 60. Type x to abort....................................< 612a!!!!!!! 2 02554 e 02681 b a 00449 a 00467 c e 02203 f 01556 34?5? >?? ET= 60 ts=i XD=d GN=858a TK=1 UP=5 FK=0 RN=1 IT=1 DR=102 rx=2 fx=038 BX=0 AH=1 AT=0 RS=1 BR=0 RI=1 GO=00000 HA=0 6X=3 3X=2 PD=2 SD=0 ?d sa=1 WM=o ar=0 ZZ=0 DC=1 ELo=010 010 011 ELb=010 010 010 TNo=0o=-2-2-2 C0b=-2-2-2 RC=0 tlo=8 8 9 tlb=8 8 8 DTR=01740 CA=1 TD= duty=087 AQ= 60 AC=1 CD=0 SR=1 UX=0 MX=0 DTU=02320 DTC=01160 RD=o ss=1 XP=2 RF=018 DS=007 SN0367 01nov99 HF=005 JC=3 CB=3 MD=5 DF=05000 RNA=1 rev 3.0a cs=37637 &=1 os= >Consec hopped exceeded. Acq sigs 60. Type x to abort....................................< 012a e 01448 e 03158 b a 00443 a 00470 c f 02500 f 01159 3456 >Consec hopped exceeded. Acq sigs 60. Type x to abort....................................< 012a 6 03069 0 03946 b a 00304 a 00492 c e 02129 a 01656 3456 >Consec hopped exceeded. Acq sigs 60. Type x to abort....................................< 012a 1 01978 a 01907 b b 00450 a 00422 c f 02304 b 01553 3456 >Consec hopped exceeded. Acq sigs 60. Type x to abort....................................< 012a f 02723 9 02779 b b 00410 a 00371 c e 02178 f 01639 3456 >Consec hopped exceeded. Acq sigs 60. Type x to abort....................................< 012a!!!!! e 02673 a 02742 b b 00460 a 00415 c! f456
Analysis of HATS data showed that the spatial resolution of finite-difference estimates of horizontal and vertical gradients can be matched by making the vertical spacing of the two horizontal arrays approximately equal to the sonic spacing within those arrays. For OHATS, WHOI engineers working on the array support structure (Mike Purcell and Megan Carroll) have chosen the sonic spacing to be 58 cm. The closest vertical spacing used for HATS was 1 m. Comparison of wind speed, TKE, and u* between the horizontal arrays and a nearby reference tower do not show any evidence of flow distortion. However it is possible that the closer vertical spacing for the OHATS arrary may start to show some evidence of flow distortion. Peter Sullivan, John Wyngaard, and I have discussed this issue and will address it from two approaches. Peter found a potential flow solution for two parallel cylinders, surrogates for the two horizontal masts, in Morse and Feshbach, Volume 2. I have made preliminary steps to applying the technique of Wyngaards's 1981 investigation of flow distortion of a single cylinder to the two cylinder problem, using Mathematica. In the meantime, however, we have also erected a subset of the planned OHATS array at Marshall to directly measure flow distortion. The Marshall array, or OHATS ops0, consists of two horizontal ASTER masts at nominal heights of 4.75 m and 5.27 m. (Because of interference between the cross-bracing of the vertical ASTER masts and the attachment hardware, we could not separate the horizontal masts by the desired 58 cm and had to settle for 52 cm.) The horizontal masts are oriented E-W so that winds from the south are perpendicular to them. About 6 m to the W we erected a reference tower. Nine sonic yokes were placed on each of the two horizontal masts, with a spacing of 58 cm, and CSAT electronics were mounted on the back of the masts in the intervening spaces. Sonics were mounted at the center three locations on both horizontal masts and at the same two heights on the reference tower. The sonics are designated as, e.g. u3, l2, etc, with u and l referring to the upper and lower arrays and the ordinal number increasing from west to east. Thus u1 and l1 are the reference sonics and u3 and l3 are the center sonics in the horizontal arrays. The specific sonics are: Loc S/N Channel l1 855 200 l2 246 201 l3 247 202 l4 800 203 u1 856 204 u2 367 205 u3 369 206 u4 853 207 Sonics 853, 855, and 856 (u4, l1, u1) have the new CSI modification to enhance their ability to operate in rain. However, one of the nylon rain socks is missing on an upper transducer of SN 853.
Output from "??" command on each sonic during ops0 flow distortion
test at Marshall. Configuration as of April 29, 2004.
channel 200:
>??
SN0855 04mar04 rev 4.0s &=1 AC=1 AF=050 AH=1 AO=00300 ar=0 AQ= 60 BR=0 BX=0
CF=1 C0o= 0 0 0 C0b= 0 0 0 CA=1 CD=0 cs=26307 DC=4 dl=015 DM=c DR=03465
duty=087 DT=16240 ET= 60 FA=00050 FL=007 FX=038 GN=744a GO=00000 HA=0
HG=01560 HH=02700 KT=0 LG=00832 LH=00100 MA=-020 MS=-010 MX=0 ND=1 NI=2
ns=00203 OR=1 os=0 PD=2 RA=00020 RC=0 RF=00900 RH=015 RI=1 RS=1 RX=002 SD=0
SL=035 SR=1 ss=1 T0123=1000 TD=a TF=02600 02600 02600 TK=1 TO= 0 0 0 TP=t
ts=i UX=0 WM=o WR=006 XD=d xp=2 XX=00875 ZZ=0
channel 201
>??
ET= 60 ts=i XD=d GN=848a TK=1 UP=5 FK=0 RN=1 IT=1 DR=102 rx=2 fx=038 BX=0 AH=1
AT=0 RS=1 BR=0 RI=1 GO=00000 HA=0 6X=3 3X=2 PD=2 SD=0 ?d sa=1
WM=o ar=2 ZZ=0 DC=1 ELo=010 010 010 ELb=010 010 010 TNo=471 d TNb=576 JD= 005
C0o=-2-2-2 C0b=-2-2-2 RC=0 tlo=8 8 8 tlb=8 8 8 DTR=01740 CA=1 TD= duty=086
AQ= 60 AC=1 CD=0 SR=1 UX=0 MX=0 DTU=02320 DTC=01160 RD=o ss=1 XP=2 RF=018 DS=007 SN0246 26mar98 HF=005 JC=3 CB=3 MD=5 DF=05000 RNA=1 rev 3.0a cs=36550 &=1 os=
>Consec hopped exceeded.
channel 202
ET= 60 ts=i XD=d GN=858a TK=1 UP=5 FK=0 RN=1 IT=1 DR=102 rx=2 fx=038 BX=0 AH=1
AT=0 RS=1 BR=0 RI=1 GO=00000 HA=0 6X=3 3X=2 PD=2 SD=0 ?d sa=1
WM=o ar=1 ZZ=0 DC=1 ELo=010 010 011 ELb=010 010 010 TNo=181 d TNb=670 JD= 005
C0o=-2-2-2 C0b=-2-2-2 RC=0 tlo=8 8 9 tlb=8 8 8 DTR=01740 CA=1 TD= duty=087
AQ= 60 AC=1 CD=0 SR=1 UX=0 MX=0 DTU=02320 DTC=01160 RD=o ss=1 XP=2 RF=018 DS=007 SN0247 26mar98 HF=005 JC=3 CB=3 MD=5 DF=05000 RNA=1 rev 3.0a cs=04332 &=1 os=
>Consec hopped exceeded.
channel 203
>??
SN0800 19sep03 rev 4.0r &=1 AC=1 AF=050 AH=1 AO=00300 ar=0 AQ= 60 BR=0 BX=0
CF=1 C0o= 0 0 0 C0b= 0 0 0 CA=1 CD=0 cs=59636 DC=4 dl=015 DM=c duty=087
DT=16240 ET= 60 FA=00050 FL=007 FX=038 GN=866a GO=00000 HA=0 HG=01560
HH=02700 KT=0 LG=00832 LH=00100 MA=-020 MS=-010 MX=0 ND=1 NI=2 ns=00203 OR=1
os=0 PD=2 RA=00020 RC=0 RF=00900 RH=015 RI=1 RS=1 RX=002 SD=0 SL=035 SR=1
ss=1 T0123=1000 TD=a TF=02600 02600 02600 TK=1 TO= 0 0 0 TP=t ts=i UX=0 WM=o
XD=d xp=2 XX=00875 ZZ=0
channel 204:
>??
SN0856 04mar04 rev 4.0s &=1 AC=1 AF=050 AH=1 AO=00300 ar=0 AQ= 60 BR=0 BX=0
CF=1 C0o= 0 0 0 C0b= 0 0 0 CA=1 CD=0 cs=47929 DC=4 dl=015 DM=c DR=03465
duty=087 DT=16240 ET= 60 FA=00050 FL=007 FX=038 GN=555a GO=00000 HA=0
HG=01560 HH=02700 KT=0 LG=00832 LH=00100 MA=-020 MS=-010 MX=0 ND=1 NI=2
ns=00203 OR=1 os=0 PD=2 RA=00020 RC=0 RF=00900 RH=015 RI=1 RS=1 RX=002 SD=0
SL=035 SR=1 ss=1 T0123=1000 TD=a TF=02600 02600 02600 TK=1 TO= 0 0 0 TP=t
ts=i UX=0 WM=o WR=006 XD=d xp=2 XX=00875 ZZ=0
channel 205:
>??
ET= 60 ts=i XD=d GN=868a TK=1 UP=5 FK=0 RN=1 IT=1 DR=102 rx=2 fx=038 BX=0 AH=1
AT=0 RS=1 BR=0 RI=1 GO=00000 HA=0 6X=3 3X=2 PD=2 SD=0 ?d sa=1
WM=o ar=0 ZZ=0 DC=1 ELo=010 010 011 ELb=010 010 010 TNo=bf7 d TNb=75f JD= 007
C0o=-2-2-2 C0b=-2-2-2 RC=0 tlo=8 8 9 tlb=8 8 8 DTR=01740 CA=1 TD= duty=089
AQ= 60 AC=1 CD=0 SR=1 UX=0 MX=0 DTU=02320 DTC=01160 RD=o ss=1 XP=2 RF=018 DS=007 SN0367 01nov99 HF=005 JC=3 CB=3 MD=5 DF=05000 RNA=1 rev 3.0a cs=37637 &=1 os=
>Consec hopped exceeded.
channel 206:
>??
ET= 60 ts=i XD=d GN=888a TK=1 UP=5 FK=0 RN=1 IT=1 DR=102 rx=2 fx=038 BX=0 AH=1
AT=0 RS=1 BR=0 RI=1 GO=00000 HA=0 6X=3 3X=2 PD=2 SD=0 ?d sa=1
WM=o ar=0 ZZ=0 DC=1 ELo=010 010 010 ELb=010 011 010 TNo=670 d TNb=a64 JD= 007
C0o=-2-2-2 C0b=-2-2-2 RC=0 tlo=8 8 8 tlb=8 9 8 DTR=01740 CA=1 TD= duty=087
AQ= 60 AC=1 CD=0 SR=1 UX=0 MX=0 DTU=02320 DTC=01160 RD=o ss=1 XP=2 RF=018 DS=007 SN0369 04nov99 HF=005 JC=3 CB=3 MD=5 DF=05000 RNA=1 rev 3.0a cs=26112 &=1 os=
>Consec hopped exceeded.
channel 207:
>??
SN0853 04mar04 rev 4.0s &=1 AC=1 AF=050 AH=1 AO=00300 ar=0 AQ= 60 BR=0 BX=0
CF=1 C0o= 0 0 0 C0b= 0 0 0 CA=1 CD=0 cs=43838 DC=4 dl=015 DM=c DR=03465
duty=087 DT=16240 ET= 60 FA=00050 FL=007 FX=038 GN=567a GO=00000 HA=0
HG=01560 HH=02700 KT=0 LG=00832 LH=00100 MA=-020 MS=-010 MX=0 ND=1 NI=2
ns=00203 OR=1 os=0 PD=2 RA=00020 RC=0 RF=00900 RH=015 RI=1 RS=1 RX=002 SD=0
SL=035 SR=1 ss=1 T0123=1000 TD=a TF=02600 02600 02600 TK=1 TO= 0 0 0 TP=t
ts=i UX=0 WM=o WR=006 XD=d xp=2 XX=00875 ZZ=0
Summary of CSAT wind tunnel tests for OHATS, 4/26-27/04 Reran CSAT853. Original run had smallest slope (0.955) and found the rain sock on one of the lower transducers to be extended beyond the transducer face by about half its length. l1fit to all data, 1.9 m/s < speed < 19.6 m/s (11 pts): 246: sonic speed = 4.3 cm/s + 0.976 pitot speed (rms = 4.1 cm/s) 247: sonic speed = 1.5 cm/s + 0.979 pitot speed (rms = 2.9 cm/s) 364: sonic speed = 5.8 cm/s + 0.970 pitot speed (rms = 1.7 cm/s) 367: sonic speed = 1.4 cm/s + 0.979 pitot speed (rms = 3.7 cm/s) 368: sonic speed = 7.2 cm/s + 0.982 pitot speed (rms = 1.9 cm/s) 369: sonic speed = 0.6 cm/s + 0.974 pitot speed (rms = 2.5 cm/s) 370: sonic speed = 4.2 cm/s + 0.980 pitot speed (rms = 5.1 cm/s) 373: sonic speed = 8.1 cm/s + 0.976 pitot speed (rms = 2.8 cm/s) 800: sonic speed = 4.6 cm/s + 0.968 pitot speed (rms = 2.9 cm/s) 853: sonic speed = 6.4 cm/s + 0.961 pitot speed (rms = 2.9 cm/s) 855: sonic speed = 2.7 cm/s + 0.973 pitot speed (rms = 3.2 cm/s) 856: sonic speed = -0.2 cm/s + 0.972 pitot speed (rms = 3.3 cm/s) l1fit to 1.9 m/s < speed < 10 m/s (5 pts): 246: sonic speed = -4.8 cm/s + 0.991 pitot speed (rms = 1.3 cm/s) 247: sonic speed = -3.8 cm/s + 0.989 pitot speed (rms = 1.1 cm/s) 364: sonic speed = 2.8 cm/s + 0.976 pitot speed (rms = 1.1 cm/s) 367: sonic speed = -2.5 cm/s + 0.986 pitot speed (rms = 1.5 cm/s) 368: sonic speed = 4.0 cm/s + 0.988 pitot speed (rms = 0.6 cm/s) 369: sonic speed = -3.5 cm/s + 0.980 pitot speed (rms = 0.8 cm/s) 370: sonic speed = -1.5 cm/s + 0.988 pitot speed (rms = 1.6 cm/s) 373: sonic speed = -0.2 cm/s + 0.988 pitot speed (rms = 1.2 cm/s) 800: sonic speed = -1.4 cm/s + 0.978 pitot speed (rms = 1.0 cm/s) 853: sonic speed = 2.0 cm/s + 0.968 pitot speed (rms = 1.0 cm/s) 855: sonic speed = 1.2 cm/s + 0.975 pitot speed (rms = 0.9 cm/s) 856: sonic speed = -2.6 cm/s + 0.976 pitot speed (rms = 0.5 cm/s)
I changed the dids from l{1:4}.4.5m and u{1:4}.5m to the actual heights,
l{1:4}.4.75m and u{1:4}.5.27m. Changes made in ops0/prep.config and
ops0/covar.config. Gordon said he would restart covars.
The attached plots show the sampling jitter and drift in a 1 hour 15 minute series from the u.l1.4.75m sonic. One can see the 9600 baud inter-character spacing in the vertical spacing between the groups of points: 10bits/byte / 9600 bits/sec = .001 secs/byte. The jitter is about +-0.005 sec. This is about 1/3rd the sampling period, which isn't great. The first plot is from u.l1.4.75m (CSAT SN 855), and the second is u.u1.5.27m (CSAT SN 856). The system clock was kept with NTP. Here are the ntp log messages around that time. May 3 12:43:29 localhost ntpd[55]: offset -0.001755 sec freq 7.762 ppm error 0.001982 poll 10 May 3 13:43:29 localhost ntpd[55]: offset -0.001508 sec freq 7.755 ppm error 0.002179 poll 10 May 3 14:43:29 localhost ntpd[55]: offset -0.007275 sec freq 7.754 ppm error 0.025945 poll 10
In prep.config, two successive channels were designated 203, when they should have been 202, 203. I fixed this at 11:30 MDT and Gordon restarted the processes.
Marshall sonic tilts determined on data from 5/1 - 5/4 09:10 MDT Assumed w.off=0 rm.azm=45 deg for reference sonics l1 and u1 rm.azm=120 deg for sonics in horizontal array sonic w.off lean leanaz l1 0 2.4 -8.1 l2 0 0.1 123.8 l3 0 1.0 -37.3 l4 0 1.9 21.9 u1 0 1.7 -0.3 u2 0 0.5 131.3 u3 0 0.1 91.5 u4 0 0.2 -61.8 Gordon applied these tilts and I verified them by rerunning plot.tilt as requested: Tom, I've re-run the covars with the new tilts. Could you check them with plot.tilt? The tilt files are in $ASTER/projects/OHATS/cal_files if you want to check/change them. Gordon 5/13 Marshall sonic tilts determined on data from 5/1 - 5/12 15:00 MDT Assumed w.off=0 rm.azm=90 deg for reference sonics l1 and u1 rm.azm=120 deg for sonics in horizontal array sonic w.off lean leanaz l1 0 2.6 0.9 l2 0 0.2 -97.8 l3 0 1.1 -47.9 l4 0 1.7 18.2 u1 0 1.5 -7.8 u2 0 0.3 123.3 u3 0 0.1 160.8 u4 0 0.3 -84.7 :sagebrush2:cal_files: grep apr csat3* csat3.l1:2004 apr 29 00:00 0.00 0.00 0.00 2.6 0.9 269.1 0 csat3.l2:2004 apr 29 00:00 0.00 0.00 0.00 0.2 -97.8 268.9 0 csat3.l3:2004 apr 29 00:00 0.00 0.00 0.00 1.1 -47.9 268.9 0 csat3.l4:2004 apr 29 00:00 0.00 0.00 0.00 1.7 18.2 269.4 0 csat3.u1:2004 apr 29 00:00 0.00 0.00 0.00 1.5 -7.8 268.6 0 csat3.u2:2004 apr 29 00:00 0.00 0.00 0.00 0.3 123.3 269.7 0 csat3.u3:2004 apr 29 00:00 0.00 0.00 0.00 0.1 160.8 269.2 0 csat3.u4:2004 apr 29 00:00 0.00 0.00 0.00 0.3 -84.7 268.6 0 5/17 Checked the tilt correction by running plot.tilt on the corrected data (without the azimuth correction!). Two sonics (l2.4.75m and u2.5.27m) had b coefficients of 0 0 -0.001; the rest had coefficients of 0 0 0.
Kurt had noticed water in the bottom of the data-system weather box after the rains at the end of April. So today at around 3:00pm Tom raised the data-system box onto the tower. This required disconnecting all the data cables. We've checked with rserial to channel 200,204 that the cables are connected as before. He also add some extra cable between the charge monitor and the data-system - previously it was stretched tight.
There are 2 chemistry trailers to the north of the sonic array (which is oriented for winds from the south). The height of the trailers is 125" and the distance to the horizontal sonic array is 80 paces/strides or about 240'. I also used the range finder function on the data scope to estimate the distance in units of trailer height. The distance was roughly 24 (+/- 1) trailer heights, consistant with the paced distance. Thus the flow distortion due to the trailers is about (1/24)^2 = 0.002.
I used the data scope to measure the orientation of the sonics. 5/7: Calibrated the data scope at Marshall. This took three tries, the last two using the monopod to help hold it steady as I rotated in 45 degree increments. The final try was graded "good 9". 5/8 Entered declinatation 10.2 E 5/10: Measured azimuths for all 8 sonics and repeated the process 4 times: Sonic mean median std dev u1 358.8 358.0 358.3 359.8 358.7 358.6 0.8 u2 000.1 359.2 358.7 000.7 359.7 359.7 0.9 u3 359.0 359.3 358.8 000.3 359.4 359.2 0.7 u4 359.1 358.8 358.4 358.3 358.7 358.6 0.4 l1 359.1 358.4 359.0 359.5 359.0 359.1 0.5 l2 359.0 358.2 358.8 359.2 358.8 358.9 0.4 l3 359.0 358.5 358.8 000.5 359.2 358.9 0.9 l4 359.5 359.3 358.7 000.9 359.6 359.4 0.9 Also measured a single azimuth 10 times. In numerical order, the samples were: 000.3 000.6 000.7 000.9 001.0 001.2 001.3 001.3 001.3 001.3 The median is 1.1. Deleting the 0.3, the mean is 1.07, the standard deviation is 0.3, and the range is +0.23, -0.47.
Marshall results to date, 5/1/2004 8:45 - 5/10/2004 12:45
linear fits of data from horizontal array sonics to reference sonics
wind speed (5 min averages):
spd.u2.5.27m = 0.980 spd.u1.5.27m + 0.02 m/s nmr = 0.056
spd.u3.5.27m = 0.974 spd.u1.5.27m + 0.03 m/s nmr = 0.059
spd.u4.5.27m = 0.984 spd.u1.5.27m + 0.03 m/s nmr = 0.057
spd.l2.4.75m = 0.996 spd.l1.4.75m - 0.00 m/s nmr = 0.063
spd.l3.4.75m = 0.986 spd.l1.4.75m + 0.01 m/s nmr = 0.059
spd.l4.4.75m = 0.988 spd.l1.4.75m + 0.00 m/s nmr = 0.059
turbulent kinetic energy (5 min averages):
tke.u2.5.27m = 1.00 tke.u1.5.27m - 0.001 m2/s2 nmr = 0.073
tke.u3.5.27m = 0.983 tke.u1.5.27m + 0.001 m2/s2 nmr = 0.075
tke.u4.5.27m = 0.999 tke.u1.5.27m - 0.001 m2/s2 nmr = 0.076
tke.l2.4.75m = 1.01 tke.l1.4.75m - 0.002 m2/s2 nmr = 0.075
tke.l3.4.75m = 1.01 tke.l1.4.75m - 0.002 m2/s2 nmr = 0.077
tke.l4.4.75m = 1.01 tke.l1.4.75m - 0.002 m2/s2 nmr = 0.078
friction velocity (30 min averages):
u*.u2.5.27m = 1.03 u*.u1.5.27m + 0.01 m/s nmr = 0.231
u*.u3.5.27m = 1.02 u*.u1.5.27m + 0.01 m/s nmr = 0.224
u*.u4.5.27m = 1.02 u*.u1.5.27m + 0.01 m/s nmr = 0.225
u*.l2.4.75m = 1.02 u*.l1.4.75m + 0.001 m/s nmr = 0.221
u*.l3.4.75m = 0.965 u*.l1.4.75m + 0.005 m/s nmr = 0.300
u*.l4.4.75m = 0.962 u*.l1.4.75m + 0.00k m/s nmr = 0.229
nmr = mean absolute deviation from linear fit/
standard deviation of data
For comparison, here are the same data for the fourth HATS configuration;
sonic spacing = 50 cm for d array, 62.5 cm for the s array, vertical
spacing = 1 m.
Speed (30 min averages) nmr
d1.4m spd = 0.994 spd.0.4m + 0.02 m/s 0.045
d2.4m spd = 0.980 spd.0.4m + 0.05 m/s 0.057
d3.4m spd = 0.995 spd.0.4m - 0.00 m/s 0.038
d4.4m spd = 0.991 spd.0.4m - 0.00 m/s 0.044
d5.4m spd = 0.993 spd.0.4m + 0.08 m/s 0.050
d6.4m spd = 0.998 spd.0.4m + 0.03 m/s 0.051
d7.4m spd = 0.992 spd.0.4m + 0.03 m/s 0.037
d8.4m spd = 0.984 spd.0.4m + 0.01 m/s 0.055
d9.4m spd = 0.985 spd.0.4m + 0.04 m/s 0.053
s1.5m spd = 0.982 spd.0.5m + 0.05 m/s 0.053
s2.5m spd = 0.989 spd.0.5m + 0.08 m/s 0.040
s3.5m spd = 0.995 spd.0.5m + 0.06 m/s 0.048
s4.5m spd = 0.996 spd.0.5m + 0.05 m/s 0.039
s5.5m spd = 0.982 spd.0.5m + 0.08 m/s 0.047
Turbulent kinetic emergy (30 min averages):
d1.4m tke = 0.972 tke.0.4m + 0.020 m2/s2 0.072
d2.4m tke = 0.967 tke.0.4m + 0.047 m2/s2 0.071
d3.4m tke = 0.973 tke.0.4m - 0.044 m2/s2 0.071
d4.4m tke = 0.972 tke.0.4m - 0.003 m2/s2 0.069
d5.4m tke = 0.984 tke.0.4m + 0.079 m2/s2 0.067
d6.4m tke = 0.979 tke.0.4m + 0.028 m2/s2 0.065
d7.4m tke = 0.971 tke.0.4m + 0.033 m2/s2 0.063
d8.4m tke = 0.972 tke.0.4m + 0.013 m2/s2 0.061
d9.4m tke = 0.973 tke.0.4m + 0.039 m2/s2 0.059
s1.5m tke = 0.974 tke.0.5m + 2.5e-4 m2/s2 0.067
s2.5m tke = 0.986 tke.0.5m + 1.5e-4 m2/s2 0.062
s3.5m tke = 1.000 tke.0.5m + 0.8e-4 m2/s2 0.061
s4.5m tke = 1.000 tke.0.5m + 0.6e-4 m2/s2 0.060
s5.5m tke = 0.989 tke.0.5m - 0.2e-4 m2/s2 0.057
Friction velocity (30 min averages):
d1.4m u* = 1.014 u*.0.4m + 0.001 m/s 0.156
d2.4m u* = 1.003 u*.0.4m - 0.001 m/s 0.183
d3.4m u* = 1.000 u*.0.4m + 0.000 m/s 0.169
d4.4m u* = 0.993 u*.0.4m - 0.000 m/s 0.173
d5.4m u* = 0.996 u*.0.4m + 0.001 m/s 0.179
d6.4m u* = 0.990 u*.0.4m + 0.001 m/s 0.180
d7.4m u* = 0.993 u*.0.4m + 0.001 m/s 0.161
d8.4m u* = 0.989 u*.0.4m + 0.002 m/s 0.170
d9.4m u* = 1.002 u*.0.4m + 0.001 m/s 0.171
s1.5m u* = 0.990 u*.0.5m + 0.001 m/s 0.223
s2.5m u* = 1.004 u*.0.5m + 0.002 m/s 0.216
s3.5m u* = 0.988 u*.0.5m + 0.002 m/s 0.220
s4.5m u* = 1.021 u*.0.5m + 0.002 m/s 0.215
s5.5m u* = 1.015 u*.0.5m + 0.001 m/s 0.210
What is error in wind speed due to a height difference between the
reference sonic and the horizontal array?
U = (u*/k)*ln(z/zo)
dU/dz = u*/kz = U/(z*ln(z/zo))
dU/U = dz/(z*ln(z/zo))
= (1 cm/500 cm)/ln(500/3) = 0.04% per cm height error
= 0.1% per inch height error
Thus a 1% error in U requires a 10 inch height error
We shut down data collection at Marshall around noon today (Friday, May 14). We plan to tear down the sensors and data system this afternoon.
Final Marshall results, 5/1/2004 8:45 - 5/12/2004 13:45
linear fits of data from horizontal array sonics to reference sonics
wind speed (942 5-min averages):
spd.u2.5.27m = 0.987 spd.u1.5.27m + 0.00 m/s nmr = 0.042
spd.u3.5.27m = 0.983 spd.u1.5.27m + 0.01 m/s nmr = 0.044
spd.u4.5.27m = 0.988 spd.u1.5.27m + 0.03 m/s nmr = 0.043
spd.l2.4.75m = 0.994 spd.l1.4.75m + 0.00 m/s nmr = 0.045
spd.l3.4.75m = 0.992 spd.l1.4.75m - 0.01 m/s nmr = 0.044
spd.l4.4.75m = 0.984 spd.l1.4.75m + 0.01 m/s nmr = 0.044
turbulent kinetic energy (942 5-min averages; TKE < 5 m^2/s^2):
tke.u2.5.27m = 0.984 tke.u1.5.27m + 0.001 m2/s2 nmr = 0.069
tke.u3.5.27m = 0.978 tke.u1.5.27m + 0.002 m2/s2 nmr = 0.070
tke.u4.5.27m = 0.993 tke.u1.5.27m + 0.001 m2/s2 nmr = 0.071
tke.l2.4.75m = 0.994 tke.l1.4.75m + 0.000 m2/s2 nmr = 0.072
tke.l3.4.75m = 0.995 tke.l1.4.75m + 0.000 m2/s2 nmr = 0.073
tke.l4.4.75m = 0.984 tke.l1.4.75m + 0.000 m2/s2 nmr = 0.074
friction velocity (359 15 min averages):
u*.u2.5.27m = 0.999 u*.u1.5.27m + 0.01 m/s nmr = 0.202
u*.u3.5.27m = 0.995 u*.u1.5.27m + 0.01 m/s nmr = 0.209
u*.u4.5.27m = 0.965 u*.u1.5.27m + 0.01 m/s nmr = 0.215
u*.l2.4.75m = 1.01 u*.l1.4.75m + 0.01 m/s nmr = 0.204
u*.l3.4.75m = 0.986 u*.l1.4.75m + 0.01 m/s nmr = 0.222
u*.l4.4.75m = 0.960 u*.l1.4.75m + 0.01 m/s nmr = 0.208
nmr = mean absolute deviation from linear fit/
standard deviation of data