CONVECTION AND SEMI-DIURNAL WAVES
103
l 25, TABLE 24
, will The Semi-diurnal Temperature Waves in the Strata 400 to 2,500
, r Meters, Together with the Single Diurnal Temperature Wave
1 at the Surface
urnal
urnal
2
T
P
2
-(<2i-<2o)
T
P
g
— (<2i-<2o)
Z A.M.
O A.M.
in all
2500
281°.0
75464
3.0
+ 151.8
280°.8
75466
6.0
+140.2
urnal
2000
285. 0
80153
4.0
+ 131.9
284 .2
80162
7.0
+ 120.1
1500
288 .6
85080
5.0
+ 111.9
287 .5
85104
7.0
+ 97.6
, and
1000
291 .9
90230
5.0
+ 38.5
290 .6
90288
6.0
+ 34.9
wave
800
293 .6
92368
5.0
+ 40.2
292 .3
92428
5.0
+ 33.1
600
295 .0
94530
4.0
+ 30.0
294 .3
94604
4.0
+ 25.8
rface,
400
295 .8
96743
4.0
+ 16.1
295 .4
96820
4.0
+ 13.2
200
293 .7
99018
3.0
- 11.7
293 .4
99095
3.0
- 15.8
the
000
231 .7
101349
2.0
291 .0
101440
2.0
oancy
10 A.M.
2 p.m.
; that
egree.
2500
280°.7
75462
9.4
+ 144.2
280°.9
75462'
9.7
+ 146.7
Id be
2000
284 .0
80173
9.4
+ 114.2
284 .8
80162
10.3
+ 133.0
rough
1500
287 .0
85112
9.4
+ 87.4
288 .8
85084
10.6
+ 133.0
1000
289 .5
90313
8.3
+ 23.0
292 .6
90228
9.2
+ 49.2
ipera-
800
291 .0
92460
8.1
+ 19.7
294 .8
92355
8.7
+ 49.2
600
292 .5
94656
7.9
+ 18.9
296 .9
94510
8.3
+ 49.9
rlace,
400
294 .5
96886
7.6
+ 16.2
299 .0
96703
7.9
+ 52.2
stem.
200
296 .2
99154
6.0
+ 23.4
300 .5
98930
7.0
+ 52.2
•ature
000
297 .7
101459
4.0
301 .3
101214
5.0
daily
6 P.M.
10 p.m.
losses
meral
2500
281°.5
75458
8.0
+ 159.3
280°. 8
75466
5.0
+ 142.0
1 axes
2000
286 .0
80142
9.0
+ 156.5
284 .3
80170
6.0
+ 117.6
1500
290 .0
85038
9.0
+ 145.6
287 .1
85102
6.0
+ 88.5
,ce, to
1000
293 .5
90166
8.0
+ 51.9
290 .7
90294
6.0
+ 34.9
2,500,
800
296 .0
92278
8.0
+ 58.9
292 .2
92432
5.0
+ 28.0
^1 tt
600
297 .3
94426
7.0
+ 51.6
294 .2
94606
5.0
+ 29.0
400
298 .0
96636
6.0
+ 42.1
295 .1
96$35
4.0
+ 19.9
right.
200
298 .6
98867
5.0
+ 31.6
295 .7
99095
3.0
+ 3.2
rning-
000
299 .0
101149
4.0
294 .3
101414
2.0
>y the
ig air from the descending air to the ground, and an inversion of tem-
rnoon perature under ordinary circumstances. The friction and the
of the earth’s deflection have very little influence on the temperature
of the and pressure conditions, and the circulation cannot be studied
iation by itself until the radiation or heating terms have been eliminated.