Solar Eclipse Diary (Part II)

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1991: OUR FIRST TOTAL ECLIPSE


        Joined by my wife Tammy, I prepared for my first total solar eclipse. In addition to observing the eclipse with eclipse glasses (for partial phases) and binoculars (for totality), I planned to photograph all aspects of the eclipse with a 35mm camera equipped with a telephoto lens.  This image scale would allow complete coverage of the corona, and might capture a prominence or two if they were large enough. Thursday, July 11, 1991 (Eclipse Day) dawned clear and remained that way. Along with several dozen other people, our observing site encircled an emptied swimming pool on a hilltop behind our hotel. This location was chosen because of close proximity to our hotel and to provide a higher elevation from which to observe the western horizon and the approaching lunar shadow.
 

Bart and his camera set-up at the 1991 total eclipse.
Totality caused a profound change to the local landscape, as shown in this pair of photographs taken before (top) and during (bottom) totality.

        First contact occurred at 10:23 a.m. For the next 84 minutes, we watched the moon swallow more and more of the sun's disk. During this time, we observed the change in ambient light, the reduction in solar radiation upon our skin, and the sharpening of our shadows as the sun was reduced to a point source of light. As totality approached, the western sky began to darken.  This darkening was subtle at first, but accelerated dramatically in the last few seconds before total eclipse. Suddenly, we saw the distant mountains darken as the shadow of the moon enveloped them. We knew that the lunar shadow, racing toward us at supersonic speeds, would soon envelop us as well. We were ready and willing! Overhead, as the last vestiges of the sun's disk shrank to become the glorious "diamond ring effect," the voices of nearby skywatchers were joined by distant voices and animal-like shrieks not normally heard from human throats. Everyone was wild with anticipation as the climax of the eclipse unfolded.
 

The 1991 total solar eclipse.
For close-up views of each image, click on the picture.

        Finally, at 11:47:40 a.m. on July 11, 1991, I beheld the spectacle of totality for the first time in my life! It was far more beautiful than I could have ever imagined! During totality, the sky was a deep, electric blue. Nearly overhead, the coal black moon resembled a black hole to infinity, with the pearly white corona encircling it in such a way as to beckon such a journey. Contrasting with the deep blue sky were some very large, pink solar prominences extending from beyond the dark edge of the moon. Like a Rorschach test, I instinctively tried to see recognizable shaped within the tendrils of luminous solar gas.  That way, I reasoned, I would later be better able to recall their glorious detail. There were definitely prominences to be seen! I saw "twin swirls" (as I called them) on the eastern limb and an even larger prominence resembling a seahorse on the opposite, northwestern limb. As totality progressed, the "twin swirls" gradually shrank and the "seahorse" grew as the moon slowly advanced across the cross section of solar atmosphere. Surrounding the solar limb and its prominences was the solar corona. Extending nearly four solar diameters toward the northeast and southwest, the pearly corona exhibited far more structure than in any photograph I'd ever seen. It was a spectacular and breathtaking sight to behold! Not wanting to miss anything, I tried to balance the time I spent taking pictures with binocular and naked eye views of the surrounding landscape and sky. Most of my pictures of totality were taken during the first three minutes; I reserved as much of the second half of totality for visual observation. I had heard too many horror stories about people who are so intent on taking pictures that they never bothered to watch the eclipse. I did not want to be one of them. My equipment included a Nikon FM2 camera equipped with a 600mm (E.F.L.) lens mounted on a small tripod. All photos were shot on ASA 125 Kodacolor print film. I bracketed my exposures to capture as wide a range of solar phenomena as possible. During totality, I exposed a total of 15 frames. Despite the fact that this total solar eclipse would be the longest one in my lifetime, it still seemed far too short. As the moon's motion revealed more and more of the "seahorse" prominence, the solar limb beneath it began to exhibit a thin red line. I heard someone exclaim "chromosphere" and I immediately recognized what I was seeing -- the thin layer of the sun's atmosphere immediately above the dazzlingly bright photosphere. I also knew that if I was seeing the chromosphere, then totality was just about to end. I took one final, intense look through the binoculars and savored the moment.  Like a bolt out of the blue, an intense point of light dazzled my eyes. The final "diamond ring" was beginning. Shouts of "no, no, not yet" filled the air as people tried in vain to stall the eclipse's inevitable ending. I checked to make sure that the sun was still in my camera's frame and took what would become my best eclipse photograph.  As the "diamond ring" grew brighter and larger, it was time to re-attach the solar filter to the camera, put the binoculars away, and reach for my eclipse glasses.
 
Bart observes the totally eclipsed sun with binoculars. Note the high altitude of the sun. 
Bart gives an enthusiastic "thumbs up" after successfully observing and photographing totality!
A very happy "Cernan Center delegation" -- Dan, Bart and Dan -- celebrate a highly successful eclipse. 

        Totality had lasted 6 minutes and 22 seconds from our location, ending at 11:54:02 a.m.  Overhead, the sky was cut in two by the receding lunar shadow. In the east were the last remnants of the deep, blue eclipse sky. In the west was the approaching sunlight. The remainder of the eclipse -- the partial phases -- was anticlimactic, yet euphoric. It was anticlimactic because the beauty of totality was over, but euphoric because the pressure was off.  We had witnessed totality in all its glory! Still, I wanted to photo-document the complete eclipse, and that included taking some partial phase photographs after totality. Finally, at 1:18 p.m., last contact occurred, and the full circle of the sun's disk returned. The entire eclipse had lasted five minutes short of three hours.
        All around me, jubilant chaos reigned! Some groups treated their people to champagne, while others simply congratulated one another and shared enthusiastic stories. "Wow, that corona was beautiful," was a common exclamation, and "did you see those huge prominences?" was a question repeated many times that afternoon.  Someone had recorded the eclipse on video, and they were sharing their footage with anyone near enough to watch. As nice as it was to watch the video replay, it couldn't hold a candle to the real thing. The full realization of just how much better a solar eclipse can be in real life than in magazine illustrations was the most valuable lesson I learned that day. I gained a new appreciation for human eyesight. In one glorious view, the human eye can simultaneously capture all the beauty of the pink prominences, inner corona, outer corona, rich sky color, nearby planets, and more. A photographer would be hard pressed to capture any one of these features on film, let alone all of them at once!
 
 

Continue to Solar Eclipse Diary (Part III)






Last updated October 20, 2001