SMITHSONIAN MISCELLANEOUS COLLECTIONS
VOLUME
95 NUMBERISHrtbur ^unb
FURTHER EVIDENCE ON
THE DEPENDENCE OF TERRESTRIAL TEMPERATURES ON THE VARIATIONS
OF SOLAR RADIATION
BY G. G.
ABBOT
Secretary, SmithsonianInstitution
(Publication 3397)
CITY
OF WASHINGTON
PUBLISHED BY
THE
SMITHSONIAN INSTITUTIONAUGUST
12,1936I
SMITHSONIAN MISCELLANEOUS COLLECTIONS
VOLUME
95,NUMBER15Hrtbur jfunb
FURTHER EVIDENCE ON
THE DEPENDENCE OF TERRESTRIAL TEMPERATURES ON THE VARIATIONS
OF SOLAR RADIATION
BY G. G.
ABBOT
Secretary,SmithsonianInstitution
(Publication 3397)
GUY
OFWASHINGTON
PUBLISHED BY
THE
SMITHSONIAN INSTITUTIONAUGUST
12,1936BALTIMORE,MD., U.8.A.
Hrtbur jfun^
FURTHER EVIDENCE ON THE DEPENDENCE OF TERRESTRIAL TEMPERATURES ON THE
VARIATIONS OF SOLAR RADIATION
By
C. G.abbot
Secretary, SmitJisonianInstitution
A
former paper onthis subject'showed how
the temperatures of Washington, St. Louis,and
Helena seem to depend on therise andfall of solar radiation. Table i of that publication gave a series of datesinall monthsof theyear
from
theyear 1924to 1935 on which the solar radiation apparently began either to rise or to fall for a succession of several days. Infigure2 (herereproducedas figurei)was shown
the oppositeaverage marches of temperature atWash-
ington for 16 days after such opposite changes of solar radiation began.On
the basis of the evidence contained in this paper, Dr. R. A.Millikan composed,andothers, includingDr. K.T. Compton, Dr.I.
Bowman,
andthe Chief of theUnitedStatesWeather
Bureau,signed with him, the followingmemorandum
:
The workonsolarradiationthathas been carriedonfor a considerablenumber ofyearsunderthe leadershipofDoctorCharles G.Abbothas apparentlybrought to lightgoodevidence,
First,thatthe rateatwhich radiant energy comes toearthfrom the sunis notentirely constant butsometimesrisesandother times fallsthroughperiods ofanumberof days;and
Second, thatthese rising orfalling periods of solar radiation arefollowed through as muchas sixteen days by measurable temperature variations inthe atmosphereasdeterminedbyordinarythermometerreadings.
Theseeffectsareofsomuchscientificandpracticalinterest for theproblem ofpredictingat least someelementsof the"weather" asmuch astwo weeks aheadthatitisourunanimous judgmentthat there should be not only a continua- tionofthisresearch but considerable enlargementandrefinementof theprogram, soasto subject these preliminaryfindings toexceedinglycarefulanddependable verificationandextension.
The Smithsonian Institution has been for atleast half a century the agent whichhasspecializedmostsuccessfully onsolar radiation problems.
No
other institutionisinasgoodapositionas isittocontinuetolead in thisfield. The'Smithsonian Misc.Coll.,vol.95,no.12,
May
1936.Smithsonian MiscellaneousCollections, Vol.95, No. 15 I
SMITHSONIAN MISCELLANEOUS
COLLECTIONS VOL. 95undersignedtherefore, afteramostcarefulstudyofDr.Abbot'sprogram,endorse
itunreservedlyandexpress the earnesthopethathemayreceivetheappropria- tionsthathe needstomakeitefifective.
An
attemptwas made
toobtain aFederalappropriation of$200,000 toestablishseven additional solar-radiationstations and toundertakeMEANRESULTS1924-1935
TEMPERATURE CHANCES FOLLOAINCRISINGSOLARRADIATION
OAYSAFTERSOLAR CHANGE BEGINS SHOWN BY FULL CURVES, FALLIN6 Bv DOTTED CURVES.
NO. 15
TEMPERATURES AND
SOLAR RADIATION ABBOTwho
with the cooperation of the University of Rochester, theEastman Kodak
Co., and other friends will undertake tests of the automatic measurementofultravioletsolarraysathighaltitudes.In order to
more
thoroughly buttress the proposition that solar variationisamajor factor in thetemperature changesof terrestrialDAYS
4 SMITHSONIAN MISCELLANEOUS
COLLECTIONS VOL. 95but allOther datesfound in Table i of
my
former publicationwere usedasdates ofincipient solarchanges.To
obtain departuresfrom
approximatedailynormalsat Potsdam, the values of the dailymeans
of temperature at y^, 14*', 21^ were employed.Monthly means
of these dailymeans
were available for the years 1921to 1934,inclusive.^Average
monthlyvalueswerecom- puted for this interval and plotted on a sufficient scale.A
smooth curvewas drawn from
these monthly averages, and the dififerences between it and the observed dailymean
temperatures were used as temperaturedepartures.Itisrecognizedthatthenormalsthus obtained are onlyapproximate.
But
this will not impair the value of the departures for the purpose proposed.For
instance, if the normals thus obtained were a littlelowfor a givenmonth,the departures forallyearsduringthat
month would
be prevailinglypositive, but thecurve oftheir fhictuationover an intervalof 16days would l)e almost precisely thesame
as if the normalshad beenperfect.Proceedingtheninexactly the
same way
asdescribedinmy
former publication, cited above,we
arrive at the resultsshown
in figure 2.Except for the
months
ofMay
and June,^ the results seemto beas emphatically favorable forPotsdam
as forWashington
tothe former conclusions, as follows: Opposite changesof solarradiation are asso- ciated for at least 2 weeks after theircommencement
with opposite marchesoftemperaturedeparturesinweather.These
averageeffects are of the order of several degrees Centigrade, although the solar changeson whichtheydependareonly of theaverage rangeofabout 0.7 percent. Ifdailyexcellent values of thesolarconstant ofradiation, trustworthy to 0.2 percent, were available, certain weather features might probablybe predicted for 2weeksormore
inadvance. Since theoryandobservation indicate that thesolarradiation changes frac- tionallyperhapstentimes asmuch
near3.too angstromsasinthesolar constant, thereisgreathopethat automatic records ofultraviolet solar radiationatgreataltitudesmay
be offirstrateimportanceforweather forecasting.'Beob. Obs.Potsdam,Deutsch. Meteorol.Jahrb.,Teil4,Hefti.
'In thesetwo monthsconsiderabletemperaturechanges are foundat Potsdam, but theyrunparallel foropposite variationsofthesun.