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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

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