Here’s the Atlantic Crossing eclipse in time-lapse from the deck of the spv Star Flyer.
The above image is a still frame from the time-lapse movie I took on November 3, 2013 of the 44-second-long total eclipse of the Sun from the mid-Atlantic Ocean. It shows the first diamond ring (second contact) as totality began.
Below is the full time-lapse.
The movie is from 385 frames shot from before totality until well after. It shows just how lucky were were at seeing this eclipse, with the Sun coming out into a deep blue sky moments before totality and going back into thin cloud just as the total eclipse ends.
You’ll also appreciate the rolling of the ship, sped up here in the time-lapse, with frames taken one second apart.
Below is a still frame of the final diamond ring (third contact). Notice the difference in the brightness of the distant clouds in this image versus the one above. In the main image at top the clouds below the Sun had not yet entered the Moon’s umbral shadow.
But in the image below, the clouds are immersed in the lunar shadow and are about to be lit up again as the shadow races away from us in the direction toward the Sun.
In the time-lapse you can see the shadow enter the scene at top, then depart at the bottom of the frame below the Sun. As it shoots away from us, the shadow darkens the horizon far in the distance further down the path, bringing totality to those on the path to the east.
– Alan, November 11, 2013 / © 2013 Alan Dyer
This is the “director’s cut” movie of the November 14 total eclipse of the Sun in Australia, unabridged and unedited.
I shot this movie of the eclipse through a telescope to provide a frame-filling closeup view of totality. This is the entire eclipse, from just before totality until well after. So it includes both diamond rings: at the onset of totality and as totality ends.
A few seconds into the movie I remove the solar filter which produces a flash of light until the camera readjusts to the new exposure. Then you really see the eclipsed Sun!
We got 1m28s of totality from our viewing site near Lakeland Downs, Queensland. But the movie times out at slightly less, because at several points where you hear a shutter click, I took a still frame which interrupts the movie. You can see some of those still images in earlier blog posts.
My timing was a little off, as I opened up the exposure to reveal more of the outer corona only moments before the end of totality, so the first moment of the final diamond ring is a little overexposed. During totality I was looking with binoculars, and made the mistake of going over and checking on my other wide-angle time-lapse camera. That wasted time needlessly. I should have spent more time attending to the movie camera and taking more stills at various exposures. No eclipse every goes quite as planned. Losing 30 seconds of totality in order to seek out clearer skies did cost me some images and enjoyment time in the umbra. But our experience was far less stressful than those who dodged clouds (or failed to miss the clouds, in some cases) at sites closer to or at the coast.
The original of this movie is in full 1920 x 1080 HD, shot with the Canon 60Da through the 105mm f/5.8 Astro-Physics apo refractor, on an equatorial mount tracking the Sun. I rarely have the luxury of shooting an eclipse through such extravagant gear, as I would never haul that type of hefty gear now on an aircraft to remote sites. But this equipment emigrated to Australia in 2002 for the total eclipse in South Australia and has been here down under ever since. So this is its second Australian eclipse. Mine, too!
– Alan, November 21, 2012 / © 2012 Alan Dyer
This is the sight eclipse chasers hate to see, yet celebrate the most! It is the diamond ring that ends totality.
This was the “third contact” diamond ring when the Sun returned in an explosion of light from behind the edge of the Moon.
Compare this view to my earlier blog, and you’ll see that the second diamond ring at the end of totality did not happen opposite the first diamond ring. That’s because we were well off the centreline of the Moon’s shadow, so from our perspective the Moon travelled across the Sun’s disk slightly off-centre.
From where we ended up in our chase for clear skies, we experienced 1m28s of totality, well under the 2 minutes maximum that others saw near the centreline. But we felt 1m28s of clear skies was better than 2 minutes under partly cloudy skies. Indeed, some on the coast saw the Sun only briefly during totality, or not at all.
Instead, while the last minute move was stressing, once we were set up, we had relaxed assurance we were going to see the whole show!
– Alan, November 14, 2012 / © 2012 Alan Dyer
The last bit of the Sun shines from behind the ragged edge of the Moon as the total eclipse begins in Australia.
This is “second contact,” and the first diamond ring effect that heralds the start of totality. The Moon (the dark disk) is just about to completely cover the Sun. You can see the pink chromosphere layer of the Sun’s surface and a flame-like prominence at 4 o’clock position. The Sun’s atmosphere, the corona, is just beginning to show.
I took this November 14, 2012 from a site near Lakeland Downs, Queensland, Australia. While we did look through some thin cirrus clouds, they didn’t hamper viewing at all, and were not the concern that the thicker clouds were at other sites, especially at the beaches.
– Alan, November 14, 2012 / © 2012 Alan Dyer