SUNSET ECLIPSE IN SPAIN
Total Solar Eclipse of 12 August 2026
Spain, Villahoz, Ermita de la Virgen de Matrigal, +42°05'30.5" N, 3°54'16.3" W, 848 m a.s.l.
Local circumstances: C1 17.33.49, C2 18.28.52, max 18.29.45, C3 18.30.37, Sunset 19:21 (effective 19.15), C4 19.22.12 UT, duration 1 min 45 s
by Lorenzo Comolli

Updates:
24/8/2026: First upload of some images:
video of totality with GoPro, sequence with 50 mm lens, logs of temperature, relative humidity, and illumination data, wide-field group image, all-sky image.
Coming in the next weeks/months: HDR corona with TEC140 + ASI6200, timelapses of totality with 50 mm, 14 mm, and 8 mm lenses, C2 and C3 contact composition and timelapse, ...
Come back here in the future to see more images.



Video of totality with GoPro

Recommended: 1080p, full screen, audio on.
The video of totality showing my setup and the eclipsed Sun in the background. The video starts about 1 minute before C2 contact and shows my friend Emmanuele Sordini and me moving around the telescopes, removing the solar filters 30 seconds before C2, checking the camera data recording, observing visually with 10x50 binoculars, taking ambient measurements, and posing for a group photo.
The video setup is a GoPro Hero5 camera at 2.7K resolution, wide field of view, and automatic exposure and sensitivity.



Sequence of the complete eclipse with a 50 mm lens
 
Click for high-res
Sequence of the full eclipse from C1 to sunset captured on a single image at 3-minute intervals. This is a classic goal for eclipse astrophotography, which at the time of film photography was captured on a single piece of film, and now with digital imaging is compiled from many frames added together via software with the strict requirement that camera pointing remains fixed.
Sequence obtained with a modified Canon 6D (Baader), Canon 50 mm f/1.8 lens used at f/5.6, exposure 1/13 s during C1-C2 partiality and 0.6 s or 5 s during C3-C4 (with solar filter D=6) and HDR of 1/13-0.6-5 s during totality (without filter), ISO 100, 3 min intervals.
Because the framing of totality was not perfectly centered in the frame, I slightly expanded the field on the left using a reference image taken outside of the eclipse, so that the image retains the real landscape.


Large field HDR group photo during totality

 
Click for high-res
Lorenzo Comolli (me) and my friend Emmanuele Sordini in a group photo taken during totality. This was a key objective of our expedition, something to take with us in the future as a reminder of the expedition. Taken near mid-totality, with the eclipsed Sun behind, with Venus visible at the top-left, showing my setup on the left (TEC140), the authors in the middle (Lorenzo and Emmanuele), Emmanuele's setup on the right (Pentax 75) and on the far right our friends Giuseppe, Valeria, Barbara, Luisa.
HDR composition obtained at mid-totality with a Canon 6D, Samyang 14 mm f/5.6, exposure 0.2-0.8-3.2 s, ISO 800.



All-Sky HDR during totality
 
Click for high-res
An all-sky shot captures all the sky in a single image, a very important feature when the time is limited like during totality!
HDR composition obtained near mid-totality with a modified Canon 5D (Baader), Peleng 8 mm f/5.6, exposure 0.4-1.6-6 s, ISO 800.


Rectangular projection of the above all-sky image. The orange horizon is mainly on the left and right of the totality. My setup (TEC140) is at the left and Emmanuele's setup (Pentax 75) at the right, while Emmanuele and I are posing for the group photo with the 14 mm lens.



Environmental measurements
A solar eclipse greatly influences Earth's atmosphere. The temperature, relative humidity, and luminance data show typical trends, peculiar to each eclipse and location.
During this eclipse I used a T/RH datalogger with the sensors positioned at 1 meter in height on a small tree, with sensors shaded from direct sunlight.
For this eclipse I recorded only a 2°C decrease relative to the trend, to be compared to 5°C in 2024 in Arkansas, USA, 9°C in 2017 in Wyoming, USA, to 4°C in Egypt 2006, to 7°C in Hungary 1999. Clearly the eclipse near the horizon greatly reduced the temperature drop
.
A digital luxmeter measured the horizontal luminance: this is a really interesting measurement, which shows the tremendous fall in light, dropping between full Sun at 30000 lux at C1 and totality at only 1.7 lux (to be compared to 1.8 lux in Arkansas 2024, 3.4 lux in Wyoming 2017, 4.1 lux in Egypt 2006). The value is the lower of my measurements, clearly due to the low altitude Sun, but in truth I expected much lower due to this; this is nearly similar to Arkansas 2024 with the eclipse very high in the sky. Maybe the shorter duration of the totality (only 1 min 45 s) was the key factor. To be better understood!
During totality I measured the sky brightness with an SQM-L, obtaining 14.29 mag/arcsecē, which is equivalent to the twilight sky when the Sun's altitude is -6°, i.e. civil twilight. Do you want to know how dark the sky is during totality? Wait for civil twilight, that is about 30 minutes after sunset!

Here are the plots of:
  • temperature
  • relative humidity
  • luminance (full period, linear)
  • luminance (eclipse+twilight, log)





Landscape and instrumentation images

Click on the image to view many landscape and instrumentation photos of the author and telescopes.



HDR image processing of a Total Solar Eclipse

Click for the PDF presentation
If you're interested in processing your HDR corona, I invite you to follow the tutorial that Lorenzo Comolli prepared after the 2017 USA eclipse. On January 27, 2018 Lorenzo was invited by the VVS association in Belgium to present at the Astrofotografiedag 2018, a conference about astrophotography. One of the presentations was on how to process the great American eclipse. Look also at the other presentation on the dedicated page.




Any comment about the images is highly appreciated, email me at comolli@libero.it


HTML Editing and Publishing by Lorenzo Comolli. Email me at comolli@libero.it.
Back to Main Page