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The purpose of the Country Scientist column is to provide projects that will encourage readers to do science. Whether you’re a student looking for a good science fair project, or an adult wanting to begin a personal science study, I hope that you’ll find this or a future project worthy of pursuing.

The Solar Aureole

Dust and other kinds of particulate matter cause the sun to be surrounded by a bright glow in the sky known as the solar aureole. The aureole is often faint or even nonexistent when the sun is viewed from a mountaintop. But it’s almost always present at lower elevations, especially during spring, summer, and fall.

The diameter and brightness of the aureole is related to the scattering of sunlight caused by particulate matter. This means a record of solar aureole photographs can provide a good indication of the transmission of sunlight through the atmosphere. The color of the sky beyond the aureole also provides clues about stuff in the air.

Since 1990 I’ve made almost daily measurements of the ozone layer, solar ultraviolet radiation, haze, total water vapor, and other sun and sky measurements from a field adjacent to the small farmhouse that serves as my South Texas office. In 1998, I bought my first digital camera, a 1.5-megapixel Fuji MX-700. To date this camera has provided 4,465 images (1,280×1,024 pixels) of the solar aureole and the sky over the north horizon. While the resolution is low by today’s standards, it’s more than adequate for a record of sky images.

These solar aureole images provide important information about my electronic sun and sky measurements, for they quickly reveal the presence of thin clouds or haze that might have affected the measurements. They also provide a visually convenient way to compare the clarity of the sky across the seasons and years.

Photographing the Aureole

Solar aureole photos can be made with virtually any kind of digital camera. For serious studies, you’ll want to use a camera that allows you to set the same exposure duration and f-stop for all your aureole photos. This will provide a record of the sky without unwanted automatic adjustments by the camera that alter or even remove the changes in sky brightness and color caused by dust, smoke, and other forms of air pollution.

The aureole is washed out if the sun is photographed directly. Worse, your eyes and a digital camera’s image sensor can be permanently damaged by the focused image of the sun. Therefore, it’s necessary to design an occulting device that blocks the direct sun when making solar aureole photos. To protect your eyes, it’s also necessary to use a method that does not require you to look anywhere near the sun.

I’ve developed various methods for photographing the solar aureole in which you need only look at your camera. My favorite occluder rig is a simple camera platform that keeps the sun and occluder in the same position for each photograph. This greatly simplifies the comparison of photos.

You can design your own platform or you can try my simple version, the Solar Photography Occluder Rig, explained in the DIY on the following page.

Making a solar aureole photo with the occluder in place is simple. If the sky is not overcast, put on sunglasses and a hat and go outdoors with your camera mounted on the occluder. If it’s awkward to sit in a chair or on the ground, brace the occluder rig against a stable object such as a fence or wall.

Switch on the camera, point it toward the sky away from the sun, and adjust its position so that the occluder is centered in the display. Then look at the front of the camera — not at the sun — while pointing the camera toward the sun. When the shadow of the occluder ball falls directly over the lens, press the shutter button and quickly move the camera away from the sun.

Forrest M. Mims III

Forrest M. Mims III (forrestmims.org), an amateur scientist and Rolex Award winner, was named by Discover magazine as one of the “50 Best Brains in Science.” His books have sold more than 7 million copies.


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