WTC _,
WTC _,
WTC _,
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
IPC VII Part 1: Measurements and Results<br />
(p.33). Sunphotometer measurements are used to determine total vertical optica! depth at 368,500 and 778 nm (p.32).<br />
The daily Ozone values are measured at Arosa and amount to: 28.09: 273.0, 2.10: 282.8, 3.10: 278.5, 9.10: 270.0,<br />
10.10: 260.0 and 11.10: 261.6 mcm (Dobsön units).<br />
4. Results<br />
A total of 36 runs taken during 7 days (1 to 11 runs per day) have been selected for the finai evaluation.- The<br />
value of PM02 readings are plotted in Fig.2.28 (p,31) and the individual ratios to PM02 on Fig.2.1-2.57 (pp.12-30)<br />
together with the frequency distribution of the data to ülustrate possible deviaüons from a normal distribution. The<br />
sky eonditions were not always ideal and the criteria for keeping a specific reading is based on the Standard deviation<br />
of the 8 readings of PM02, which had to be lower than 0.8 Wm"^. If this criterion was not reached the readings of<br />
all instruments at that particular time were dismissed. The mean results are summarized in Table 1!2 with the<br />
calibration faetdrs (C„ Q, C3) used in the evaluation and the WRR calibration factor from IPC VI if available.<br />
Instrument<br />
PM02<br />
PM05<br />
CROM 2L<br />
CROM 3L<br />
PAC 3<br />
MKVI-67814<br />
HF-18748<br />
PM06-5<br />
PMO6-10<br />
PM06-79121<br />
PMÖ6-80022<br />
PMO6r811104<br />
PMO6-811107<br />
PMO6-811108<br />
PMO6-850401<br />
PMO6-850407<br />
EPAC-12843<br />
EPAC-13219<br />
EPAC-13617<br />
HF-14915<br />
HF-15744<br />
HF-17142<br />
HF-18747<br />
HF-19746<br />
HF-21185<br />
HF-23725<br />
HF-27159<br />
HF-27160<br />
HF-27162<br />
HF-27798<br />
Calibration Cönstants<br />
C2 C3<br />
24.18<br />
31.615<br />
127.687<br />
127.549<br />
9962.6 .07 75<br />
10007. 10.<br />
19989. .07 75<br />
23/729 '<br />
22.6395<br />
23.847<br />
23i9l5<br />
23.855<br />
24.031<br />
24.0887<br />
24.095<br />
24.046<br />
1.0035<br />
10079.<br />
10024.<br />
20010.<br />
20020.<br />
20020.<br />
20014;<br />
19975.<br />
20020.<br />
19970.2<br />
20030.<br />
20030.<br />
20020.<br />
20020.<br />
.064<br />
.064<br />
.066<br />
.066<br />
.066<br />
.066<br />
066<br />
.066<br />
Table 1.2: Ratios to PM02 and WRR-WSG<br />
Comments<br />
WRR (IPC VI) 24^1546<br />
WRR (IPC VI) 31.6384<br />
WRR (IPC VI) 128.0215<br />
WRR (IPC VI) 127.4852<br />
WRR (IPC VI) 9965.59<br />
WRR (IPC VI) 10015.3<br />
WRR (IPC VI) 23.7314<br />
WRR (IPC VI) 22.7346<br />
WRR (1987)<br />
WRR (IPC VI) 23.9205<br />
Charäcterization 1982<br />
WRR (IPC VI) 24.0120<br />
Change in electronics<br />
WRR (1985)<br />
WRR (1986) 24.196<br />
WRR (IPC VI)<br />
WRR (IPC VI)<br />
WRR (IPC VI) 10052.1<br />
WRR (IPC VI) 19978.4<br />
WRR (IPC VI) 20020.6<br />
WRR (TPC VI) 19982.<br />
WRR (IPC VI) 19998.6<br />
WRR (IPC VI) 19973.8<br />
WRR (IPC VI)<br />
Ratio to PM02<br />
with C used<br />
1.00000<br />
.99881 + .00092<br />
' .99651 + .00140*<br />
1.00054 ± .00140<br />
.99917 ± .00085<br />
.99850 ± .00090<br />
(1.00022 ± .00197<br />
1.00073 ± .00417<br />
.99717 ± .00219<br />
.99320 ± .00090<br />
1.00232 ± .00090<br />
1.00044 ± .00119<br />
.99995 ± .00153<br />
.99947 + .00087<br />
1.00085 + .00189<br />
.99141 ± .00187<br />
1.00152 + .00169<br />
1.00031 + .00541<br />
.99716 + .00193<br />
1.00104 + .00129<br />
.99976 ± .00098<br />
1,00244 ± .00158<br />
1.00027 + .00132<br />
.99790 ± .00122<br />
1.00012+ .00161<br />
.99838 ± 00188<br />
1.00016 ± .00113<br />
1.00217 ±.00115<br />
, .99907 ± .00133<br />
L00107 ±.00146<br />
Ratio to Change Fig.<br />
WRRwsG PP*^ ' page<br />
-.99951 -487<br />
1.000H 113<br />
.99984 -157<br />
1.00060 603<br />
1.00003 33<br />
.99989 -107<br />
31<br />
12<br />
12<br />
12<br />
13<br />
13<br />
1.00078)') 13<br />
1.00140 1396 14<br />
1.00192 1924 14<br />
.99376<br />
14 ..<br />
L00312 3117 15<br />
1.00101 15<br />
.99969 -306 15<br />
1.00003 16<br />
1.00142 16<br />
.99816 16<br />
1.00209 2085<br />
1.00088 1 875<br />
17<br />
17<br />
1.00052 520 17<br />
1.00002 .23 18<br />
1.00035 . 354 18<br />
1.00110 1102 18<br />
1.00007 65 19<br />
.99840 -1597 19<br />
1.00069 19<br />
.99894 1056 20<br />
1.000731 20<br />
1.00274 20<br />
.99963<br />
21<br />
1.00164<br />
21<br />
') After the comparison a bug was found in the cavity; although it was not in beam the results have to be discarded.<br />
5