THE ISOTHERMAL REGION
95
TABLE 23
Mean Thermodynamic Values for the Atlantic Tropics
a
T
P
p
CP
3
Qi-Qo
Si-So
Wi-
Wo
Ui-Uo
Kio
20000
19000
18000
17000
227.0
9894
0.2256
668.93
8.0
-3012
-13.359
4911
-7922
17488
16000
217.3
11213
.2513
709.00
7.4
-2570
-10.292
5203
-7774
18647
15000
209.9
13331
.2788
788.87
8.8
-1898
- 8.567
5609
-7506
19328
14000
212.8
15665
.3128
814.91
8.5
-1584
- 7.361
5750
-7334
21544
13000
215.9
18398
.3502
835.84
14.3
-1470
- 6.697
5911
-7381
24731
12000
221.6
21442
.3911
855.58
13.8
-1345
- 5.949
6024
-7369
28286
11000
230.3
24942
.4355
861.08
13.3
-1302
- 5.545
6060
-7362
32588
10000
238.9
28853
.4830
865.62
12.4
-1250
- 5.135
6086
-7336
37288
9000
247.7
33204
.5338
869.26
12.0
-1182
- 4.699
6127
-7309
42938
8000
254.9
38038
.5879
878.51
11.8
-1100
- 4.252
6199
-7298
47822
7000
260.1
43413
.6459
887.63
10.7
-1000
- 3.769
6271
-7271
53935
6000
268.3
49379
.7079
899.98
9.9
- 881
- 3.247
6368
-7248
59582
5000
274.1
56008
.7742
913.55
6.6
- 700
- 2.534
6473
-7173
65980
4000
278.5
63380
.8453
931.88
6.5
- 532
- 1.907
6591
-7123
72304
3000
283.9
71569
.9217
946.73
6.5
- 397
- 1.388
6694
-7091
78606
2000
288.8
80625
1.0031
963.44
5.8
- 187
- 0.641
6846
-7033
86055
1000
292.4
90699
1.0908
984.35
4.4
- 24
- 0.081
6911
-6935
93656
000
299.5
101753
1.1837
993.58
5.8
In the Europe group 9,000 to 10,000 is omitted, and in the
tropic group 10,000 to 12,000 is omitted, as being regions of
special local supply. It appears that heat is lost at about three
times greater rate in the isothermal region than in the lower
levels. This occurs at the same time the temperature is rising
in the isothermal region but falling in the lower levels. The
Victoria Nyanza ascensions give A (Qi — Qo) = — 144 through
out the region 3,000 to 18,000, but in this case no inversion
of T was found. (4) The principal fact to be explained is the
slow rate of loss of heat in the convectional region, 140 per
1,000 meters, as compared with that in the isothermal region,
about 400. This is easily accounted for by the following facts:
The incoming solar radiation is of short wave lengths, and pen
etrates to the earth’s surface, having only a small amount of