Solar considerations in the development of cutaneous melanoma.

On the basis of these considerations, the possible action spectrum for melanoma can be narrowed considerably, but not confined to any one solar emission band. The physical factors discussed eliminate all but UV, visible, and NIR radiation as possible solar agents. Ionizing radiation fits neither the epidemiologic data nor first-order physical considerations. Wavelengths longer than the NIR wavelengths, although they could conceivably account for the occurrence of melanoma under clothed parts of the body, carry so little energy that they are probably unimportant. Epidemiologic evidence regarding the effects of skin pigment favors UV or visible radiation. A distinction between these two components is not obvious; UV-C and UV-B photons carry greater energy and are more likely to induce biochemical cutaneous effects, but the total flux in the UV-A and visible radiations is far greater. That UV-B radiation may play a role in melanoma is supported; at the same time, one cannot exclude the possibility that the action spectrum for melanoma is, instead, the UV-A, the visible, or even the NIR portion of the sunlight spectrum. The strong differential effect of altitude on the transmission of light of different wavelengths might serve as an important discriminating variable. If solar UV radiation is implicated in the development of melanoma, then altitude should emerge as a significant factor in epidemiologic studies. If visible or IR radiation is the active agent, then differences on the basis of altitude should be small or negligible. Intrinsic solar variations that follow the annual sunspot number appear inadequate in either the UV or the visible band to account directly for the apparent 11-year modulation of melanoma incidence found in some registries. Secondary atmospheric effects brought about by the action of solar UV changes on the ozone layer may be adequate to explain a weak 11-year modulation in melanoma incidence, although continuous measurements of UV-B flux made at sites in the United States through a full solar cycle have shown no such effect. Nor do these early measurements reveal the long-term increase in UV-B intensity expected from the destruction of stratospheric ozone by industrial pollutants over the last 10 years.

Edison the scientist.

This year marks the 100th anniversary of Edison's invention of the electric lamp, one of many heralded accomplishments that brought him lasting fame. For much of life Edison enjoyed a popular reputation as a laboratory genius who personified the spirit of scientific discovery. Was he really a scientist, or only an inventor? His participation in the Draper Expedition to the solar eclipse of 1878, told here, offers a chance to evaluate the youthful Edison as an astronomer and infrared physicist.

Anomalous solar rotation in the early 17th century.

The character of solar rotation has been examined for two periods in the early 17th century for which detailed sunspot drawings are available: A.D. 1625 through 1626 and 1642 through 1644. The first period occurred 20 years before the start of the Maunder sunspot minimum, 1645 through 1715; the second occurred just at its commencement. Solar rotation in the earlier period was much like that of today. In the later period, the equatorial velocity of the sun was faster by 3 to 5 percent and the differential rotation was enhanced by a factor of 3. The equatorial acceleration with declining solar activity is in the same sense as that found in recent Doppler data. It seems likely that the change in rotation of the solar surface between 1625 and 1645 was associated with the onset of the Maunder Minimum.

Far infrared airborne spectroscopy.

Equipment and techniques employed in an airborne far ir (80-400 micro) spectral measurement of the solar brightness temperature are described, with particular attention paid to the scanning Michelson interferometer and the radiometric calibration. The airborne performance of several telescopic guiding systems, a liquid helium cooled bolometer, and golay cells are discussed, summarizing experience gained on twenty-five jet aircraft flights.