The goal of the analysis was to understand the physical causes of the observed
temperature difference between the two hygrothermometers. An initial step was to
confirm the absolute accuracy of the ASOS hygrothermometer. The NWS examined
several of the ASOS instruments at Sterling, Virginia, and found a range of 0.20
F.
Three additional comparisons were made in the field at Colorado Springs, Colorado
(COS), Oklahoma City, Oklahoma (OKC), and Tulsa, Oklahoma (TUL), which
showed a range of 0.30
F relative to a field standard (RM Young), which had
been calibrated against a secondary standard at Sterling, Virginia. Thus, ASOS does
not have a temperature bias. The model used to assess the temperature differences
had the analytic form:
DT ¼ DT
i
þ DT
l
þ DT
s
ð1Þ
where DT is the observed temperature difference of ASOS–H083, and the subscripts
are i (instr uments), l (local effect of location), and s (solar heating effect). All of the
separations between the hygrothermometers were less than 1 mile and the hygro-
thermometers were collocated at four sites, which would have no local effect, by
definition. Local effects due to site location could be different for day and night,
various weather systems, and seasons. Solar heating was included since it was
known that the H083 had a solar heating problem.
Results of the analyses are given in Table 2 for the 15-month period. Observed
differences in the maxi mum and minimum temperatures (labeled M
x
and M
n
) show
ASOS to be cooler by 1.17
F(M
x
) and 0.86
F(M
n
) averaged over all sites. Two
methods were used to determine the instrument bias of the H083 (DT
i
) assuming
ASOS had no bias. The first was to examine comparison s when wind speeds were
high enough to reduce local effects resulting in a narrow frequency distribution of
DT. A speed of nearly 15 miles per hour was required, but there were not enough
observations remaining to be meaningful at all sites. The second approach was to
have an ASOS reported overcast sky at night, which meant cloud base was 12 ,000 ft
or lower. Downward infrared radiation from an overcast low cloud would reduce
horizontal temperature differences. In fact the frequency distribution of observed
temperature differences was very narrow, which indicated the local effects were
reduced. The instrument bias determined from this analysis is given in Table 2 in
the column marked DT
i
. The average DT
i
was 0.57
F, and the range was quite large
from 0.16 to 1.06
F. The ASOS at Lincoln, Nebraska, was moved midway in our
data collection period. Two LNK sites are thus included. LNK-1was the first location
and the ASOS instrument was moved to LNK-2, which was essentially collocated
with the H083. The cloud analysis yielded the same estimate of DT
i
from the two
locations. Next the H083 bias was subtracted from the M
x
and M
n
observations, and
the remainder for the M
n
is DT
l
at night and for the M
x
is a combination of DT
l
in the
daytime plus the solar effect. Notice the resulting DT
l
from the M
x
has a wide range
of 0.56 to 1.10
F. This shows that local effects can be quite important for distances
less than 1 mile. For the daytime local effect plus solar effects, several of the sit es
showed a magnitude of 1
F or larger indicating a likely strong solar effect, which
was previously established as a problem for the H083. As a consequence of the
8 DATA CONTINU ITY STUDIES 759