Technical challenges recording the solar eclipse and how to address them, using example pictures taken on March 20, 2015 in Vienna, Austria.
On March 20, 2015 I was able to capture three different stages of the solar eclipse. From left to right, the stages are:
- 10:30 CET: The moon covers about 40% of the sun
- 10:51 CET: The moon covers about 63% of the sun, this was the maximum coverage visible from Vienna, Austria
- 11:17 CET: The moon covers about 30% of the sun
1.Solar Eclipse Challenges
Basically, there are two challenges when taking pictures of a solar eclipse:
- Focal length: you need a long lens to produce a picture of the sun filling a significant part of the frame. The same is true for moon photography, as both are about the same size.
- Filters: you need a filter strong enough to prevent your sensor from being fried
You will need a lens with a focal length of at least 800 mm (35 mm equivalent), better 1000 mm. Using my trusty Nikon V1 on a 80-400 mm Nikkor resulted in a focal length equivalent of 1080 mm. The sun was big enough with this combination. I could have added a 1.4x teleconverter, but I felt it was not needed.
The bigger challenge are the filters. I started with a Lee Big Stopper (a 10 stop ND filter), but I had to add another 4 stop ND filter to finally get pictures where the sun was not overexposed.
This solved the exposure problem, but you can imagine what happens when you point a lens with two filters in front of it directly towards the sun – LOTS of flares. You can solve solve this by positioning the sun off-center. This will move the flares the opposite side of the frame.
In the end, I did cut out the sun from three different pictures and combined them to the picture shown above.
Honestly, solar eclipse pictures are pretty boring when you record them using visible light – it is just the shape that makes the picture interesting. You can get much more interesting pictures of a solar eclipse using a Hydrogen-Alpha (Hα) filter – just look at some solar eclipse pictures using a Hα filter.
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