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<strong>Long</strong>-<strong>term</strong> <strong>variations</strong> <strong>of</strong> <strong>atmospheric</strong><br />

<strong>transmittance</strong> <strong>from</strong> pyrheliometer<br />

measurements<br />

Nozomu Ohkawara<br />

Atmospheric Environment Division,<br />

Global Environment and Marine Department,<br />

Japan Meteorological Agency (JMA)<br />

12 th BSRN Science and Review and Workshop, 1 Aug. 2012, Potsdam, Germany


Background<br />

• The long-<strong>term</strong> variation <strong>of</strong> the <strong>transmittance</strong> was reported for North<br />

America and for Europe<br />

• The long-<strong>term</strong> change in the <strong>transmittance</strong> measured over Japan is<br />

presented.<br />

• The weight <strong>of</strong> aerosol in de<strong>term</strong>ining the variation in <strong>transmittance</strong> is<br />

also analyzed.<br />

How was it<br />

change? <br />

Martin Wild, Hans Gilgen, Andreas Roesch, Atsumu Ohmura, Charles N. <strong>Long</strong>,<br />

Ellsworth G. Dutton, Bruce Forgan, Ain Kallis, Viivi Russak, Anatoly Tsvetkov (2005)


Direct solar radiation measurements in Japan<br />

• JMA has been conducting direct solar radiation measurements by<br />

pyrheliometers since International Polar Year (I.P.Y.) in 1932.<br />

• Although the number <strong>of</strong> observation stations differs by age, the<br />

measurements were conducted at 14 stations, which covered all<br />

climatic zones in Japan, for a long time.<br />

• The direct solar radiation was measured 3 times a day at 09, 12 and 15<br />

Local Apparent Time (LAT) when there was no cloud in the direction <strong>of</strong><br />

the sun.<br />

BSRN station <br />

A map <strong>of</strong> 14 stations <strong>of</strong> direct solar radiation measurement in Japan used in this study.


Station list used in this study (14 stations)<br />

Station <br />

WMO<br />

identifier <br />

Start <strong>of</strong><br />

observation <br />

Sapporo 47412 Aug.1932 - <br />

Nemuro 47420 Sep.1953 - <br />

Akita 47582 Aug.1932 - <br />

Miyako 47585 Jun.1952 - <br />

Wajima 47600 May 1953 - <br />

Matsumoto 47618 Jan. 1936 - <br />

Tateno 47646 Dec.1957 - <br />

Yonago 47744 Feb.1940 - <br />

Shionomisaki 47778 Aug.1932 - <br />

Fukuoka 47807 Aug.1932 - <br />

Kagoshima 47827 Apr.1940 - <br />

Shimizu 47898 Aug.1932 - <br />

Ishigakijima 47918 Jan.1941 - <br />

Naha 47936 Sep.1932 - <br />

BSRN station


Data rescue<br />

Recently, the results <strong>of</strong><br />

direct solar radiation<br />

measurements by<br />

pyrheliomaters were<br />

digitized, providing the<br />

basis for the study <strong>of</strong> long<strong>term</strong><br />

<strong>variations</strong> <strong>of</strong><br />

<strong>atmospheric</strong> <strong>transmittance</strong><br />

for more than 70 years. <br />

An original record <strong>of</strong> pyrheliometer measurements<br />

(at Fukuoka station in Aug. 1932)


Traceability to the international solar radiation scale<br />

Before 1970<br />

• Several Ångström pyrheliometers calibrated in Stockholm, Sweden<br />

were imported and used as national standard pyrheliometers.<br />

• Ångström scale 1905 was transfered to operational standard siver<br />

disk pyrheliometers, and then scale was converted to Smithsonian<br />

scale.<br />

Smithsonian scale (JMA) = Ångström scale 1905 x 1.035<br />

“The operational standard silver disk pyrheliometer used for<br />

calibration <strong>of</strong> operational pyrheliometers in early times was<br />

extremely stable and its sensitivity remained virtually unchanged<br />

for more than 35 years since the start <strong>of</strong> the observation in 1932”<br />

(Japan Meteorological Agency, 1975).


transfer the<br />

pyrheliometric scale<br />

Ångström pyrheliometer<br />

(national standard ) <br />

Silver disk pyrheliometer<br />

(operational standard & operational pyrheliometer)


1970-<br />

JMA has been participating IPC to calibrate national(regional)<br />

standard pyrheliometers against international scale since IPC-III in<br />

1970.<br />

IPC-III<br />

1970<br />

IPC-XI<br />

2010


Used pyrheliometer & scale <strong>of</strong> solar radiation measuremnents<br />

Period <br />

Type <strong>of</strong><br />

pyrheliometer <br />

Scale <strong>of</strong> solar radiation<br />

measurements <br />

Conversion factor to<br />

WRR <br />

1932- Silver disk<br />

pyrheliometer <br />

1957-1<br />

970 <br />

Silver disk<br />

pyrheliometer <br />

Smithsonian scale (JMA)<br />

(Ångström scale 1905 x1.035) <br />

1.026 / 1.035<br />

=0.9913 <br />

IPS-1956 (JMA)<br />

1.026 / (1.035x0.98)<br />

(Ångström scale 1905 x1.035x0.98) =1.012 <br />

1971-1<br />

977 <br />

1978-1<br />

980 <br />

Silver disk<br />

pyrheliometer <br />

Thermoelectric<br />

pyrheliometer <br />

1981- Thermoelectric<br />

pyrheliometer <br />

IPS-1956 <br />

IPS-1956 <br />

WRR <br />

1.022 <br />

1.022 <br />

1.000 <br />

All <strong>of</strong> the measurements were converted in WRR, before calculating<br />

the <strong>transmittance</strong>.<br />

As for the solar constant, a fixed value <strong>of</strong> 1367 W/m 2 recommended<br />

by World Meteorological Organization (WMO) was used.


Diurnal and seasonal variation <strong>of</strong> <strong>transmittance</strong><br />

Results<br />

annual <strong>variations</strong> <strong>of</strong> monthly mean <strong>transmittance</strong> averaged among selected 7 stations.<br />

Monthly mean <strong>transmittance</strong> values at each observation time (09, 12 and 15LAT) and<br />

diurnal mean values averaged over the whole data period <strong>from</strong> 1932 to 2005 are<br />

plotted.


• Diurnal <strong>variations</strong> between 09, 12 and 15LAT for each month are<br />

smaller than the range <strong>of</strong> the annual <strong>variations</strong> <strong>of</strong> monthly mean<br />

values.<br />

• The difference in the <strong>transmittance</strong> among each observation time<br />

within the same month is less than 0.02, while the difference between<br />

the largest and smallest months is much larger and reaches 0.13.<br />

• If a prolonged missing observations existed for several months, the<br />

seasonal <strong>variations</strong> could influence the annual means. This tendency<br />

must be taken into account for calculating the annual means.


<strong>Long</strong>-<strong>term</strong> <strong>variations</strong> <strong>of</strong> <strong>transmittance</strong><br />

Methods<br />

To analyze the long-<strong>term</strong> <strong>variations</strong> <strong>of</strong> <strong>atmospheric</strong> <strong>transmittance</strong>,<br />

the seasonal <strong>atmospheric</strong> <strong>transmittance</strong> was first calculated <strong>from</strong><br />

monthly mean for each year, so that each season has the same<br />

weight in the annual mean value.<br />

• spring: March-May<br />

• summer: June-August<br />

• fall: September-November<br />

• winter: January and November-December<br />

If there was any missing seasonal <strong>transmittance</strong> in a year, annual<br />

mean would not calculated.


Results<br />

• From 1933 to late 1940s, the <strong>transmittance</strong> remained stable at around<br />

0.74 to 0.75.<br />

• Decreasing phase followed to the mid-1980s when it reached 0.69.<br />

• It then turned into be increasing phase till the early 2000s marking the<br />

level <strong>of</strong> 0.71.<br />

<strong>Long</strong>-<strong>term</strong> <strong>variations</strong> <strong>of</strong> annual mean <strong>transmittance</strong> at 14 stations in Japan.<br />

A black thick line shows average among 14 stations.


Cause <strong>of</strong> long-<strong>term</strong> <strong>variations</strong> <strong>of</strong> <strong>transmittance</strong><br />

• Besides the large volcanic eruptions, the variation is caused<br />

mostly by the aerosol and the precipitable water vapor (PWV) in<br />

the atmosphere.<br />

• Japan has a dense coverage <strong>of</strong> the rawinsonde observation<br />

starting in 1955.<br />

• The impact on the long-<strong>term</strong> variation <strong>of</strong> <strong>transmittance</strong> by that <strong>of</strong><br />

water vapor content in the atmosphere was estimated using<br />

precipitable water vapor (PWV) <strong>from</strong> rawinsonde measurements.


Bias correction for rawinsonde measurements<br />

During the period <strong>from</strong> 1957 to 2005,<br />

three types <strong>of</strong> rawinsonde were used for<br />

upper air observation.<br />

The biases among them were reported as<br />

the intercomparison results, beforehand<br />

(Japan Meteorological Agency, 1983;<br />

World Meteorological Organization,<br />

1996). <br />

<br />

<br />

<br />

<br />

<br />

<br />

<br />

<br />

pressure <br />

humidity <br />

temperature


Monthly mean precipitable water vapor <strong>from</strong> rawinsonde data<br />

Monthly mean precipitable water vapor (PWV) was calculated <strong>from</strong><br />

rawinsonde measurements at 00 and 12 UTC.<br />

It was confirmed bias correction for rawinsonde data worked well. <br />

<br />

Annual mean precipitable water vapor calculated <strong>from</strong> rawinsonde<br />

measurements at Tateno station.


Calculation <strong>of</strong> <strong>transmittance</strong> due to water vapor<br />

Transmittance due to water vapor content in the atmosphere was<br />

calculated <strong>from</strong> monthly mean PWV at 09, 12 and 15LAT on 15th day <strong>of</strong><br />

each month by Gueymard’s method (1998).<br />

Then monthly mean and annual mean <strong>transmittance</strong> were calculated.


Results<br />

• The variability <strong>of</strong> annual mean PWV is about 5 mm around the long<strong>term</strong><br />

mean <strong>of</strong> 22.13mm on average among the stations during the<br />

period <strong>from</strong> 1957 to 2005.<br />

• The variation in PWV would cause the <strong>transmittance</strong> change <strong>of</strong><br />

only about 0.01. <br />

<strong>Long</strong>-<strong>term</strong> <strong>variations</strong> <strong>of</strong> annual mean precipitable water vapor (PWV), <strong>transmittance</strong><br />

due to PWV (Tw) and total zenith <strong>transmittance</strong> (T) averaged among 7 stations in<br />

Japan. PWV and Tw are plotted for the period <strong>from</strong> 1957 to 2005 while T is plotted<br />

for the whole analyzed period.


Results (cont.)<br />

• Main cause <strong>of</strong> the variation <strong>of</strong> <strong>transmittance</strong> is due to the direct<br />

effect by aerosols in the atmosphere.<br />

• Among all aerosols in the atmosphere, the contribution <strong>of</strong> natural<br />

sources to the variation <strong>of</strong> the total aerosol concentration is very<br />

small (Streets et al., 2009) leaving the possiblity to anthropogenic<br />

aerosols.


Summary<br />

• From 1933 to late 1940s, total <strong>transmittance</strong> remained stable<br />

at around 0.74 to 0.75, followed by the decreasing phase to<br />

the mid-1980s when it reached 0.69. It then turned into be<br />

increasing phase till the early 2000s marking the level <strong>of</strong><br />

0.71.<br />

• Both mean <strong>transmittance</strong> and its variable range are smaller<br />

than those in Europe.<br />

• The majority <strong>of</strong> these <strong>variations</strong> is caused by aerosol, and<br />

water vapor changes making only a minor contribution.<br />

• The aerosol changes are considered to be due to changes in<br />

anthropogenic sources.


Danke!!

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