Serendipity and The
Citizen Scientist
Forrest M. Mims III
This and the past issue of The
Citizen Scientist were largely assembled in Hawaii,
where I recently spent three weeks teaching atmospheric
science to a class of university students from eight
nations and calibrating instruments during treks to
the famous Mauna Loa Observatory at 3,400 meters (11,200
feet) over the Pacific Ocean.
Serendipity played unexpected roles
in assembling this issue.
My students this year included several
accomplished photographers, including Ji Hyun Chang
from Brazil. Ji used his digital Nikon SLR to make sequences
of images that he stitched together to form beautiful
panoramic views from Hawaii's Mauna Kea. Three of his
panoramas appear in this issue's "Gallery."
Then there was the ultraviolet study
conducted by two of my students. The same day they began
a science project to measure the UV-B wavelengths that
promote the synthesis of vitamin-D in the skin of vertebrates,
former NASA scientist Bill Grant submitted a feature
article on his measurements of the vitamin-D action
spectrum for a year in San Francisco. Dr. Grant's article
appeared as the lead feature in the 02 June 2006 issue
of TCS ("Rates
of Vitamin D Production from Solar Ultraviolet B Irradiance
in San Francisco During One Year"). Dr. Grant
and my students used the same model vitamin D radiometer
for their studies, a Vitamin D3 meter from Solartech,
Inc.
During his one-year study, Dr. Grant
measured peak (solar noon) vitamin D production rates
(VDPR) of about 15 International Units/minute in winter
and about 67 I.U./min vitamin D production rates during
summer.
The student measurements in Hawaii
were made by Tsion A. Alemayehu (Ethiopia) and Chelsa
Kallis (USA), both at the University of the Nations
(Fig. 1). Because of cloud cover and the ever present
layer of volcanic emissions known locally as vog, their
measurements near sea level fluctuated wildly. At the
high-altitude Mauna Loa Observatory, they measured as
much as 97 I.U./min vitamin D. Clouds prevented measurements
at solar noon on the mountain, so we assumed that the
clear sky solar noon value would be higher. I confirmed
this several days later on a day when the sky was totally
clear at the observatory. The meter indicated 113 I.U./min
vitamin D at solar noon.
Studies of vitamin D production rates
by natural sunlight have become increasingly important
because of a range of new medical studies that report
widespread vitamin D deficiency in people living within
the temperate latitudes. Various other studies have
reported on previously unexpected beneficial effects
of vitamin D including reducing the rates of several
of the most serious cancers.
There is considerable irony in this,
for it is well known that too much sunlight exposure
can cause skin cancer. Some of the same wavelengths
of UV-B that cause skin cancer promote the synthesis
of vitamin D with high efficiency. Scientists like Bill
Grant and others are now exploring safe levels of sunlight
exposure that will provide the benefits of desirable
levels of vitamin D without the risk of skin cancer.
Some of Dr. Grant's suggestions are discussed in his
article.
The long-term measurements by Bill
Grant and the short term project by the two students
in Hawaii demonstrate how a professional scientist and
students can study the same phenomenon using identical
instruments. Citizen scientists can contribute to this
research by making their own measurements. How, for
example, are vitamin D production rates affected by
air pollution, cloud cover and the seasons? Are there
any trends at particular locations? How much vitamin
D production occurs in shaded spots?
If you take a vitamin D meter on vacation,
you can study how vitamin D production rates are affected
by latitude. Of special interest would be measurements
made in the Southern Hemisphere, for the elliptical
orbit of the earth around the sun places the Earth closer
to the sun during summer in the Southern Hemisphere
than when the Northern Hemisphere is in summer. Assuming
the same ozone conditions and a clear sky, this is why
UV-B rates at sea level in Australia can be around 7
percent higher at the summer solstice than at the summer
solstice at the same latitude in the northern hemisphere.

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