Best places by clouds @ eclipse time
The strongest candidate sites re-ranked by the live eclipse-hour cloud forecast (selected model), with the 26-year climatology alongside and distances from your spot. Until the forecast horizon opens, the ranking falls back to climatology.
Your observing spot
Your spot and tapped points are kept in the page link β hit π sync and open the link on your phone/laptop to carry the exact setup across devices.
Cloud coverage β every dataset @ eclipse hour
One row per point β your observing spot plus every point you tap on the map β one column per dataset: the 26-year ERA5 climatology, the repo's auto-refreshed cloud snapshot, and six live forecast models at the eclipse hour (~20:30 CEST). Β± is the model spread (small = the models agree); βββ is how much of your line of sight to the low Sun is blocked where it crosses the low/mid/high cloud decks (selected model).
Tapped map points
Tap anywhere inside the totality band on the Map tab β the point lands here and joins the dataset matrix above (newest first, up to 9; re-tapping a point bumps it back to the top).
Hourly cloud decks β this spot
Reading the pressure (hPa column above & the line under the decks): β₯ 1022 strong high β sinking air, the clear-evening machine Β· 1015β1021 weak high β usually fine Β· 1008β1014 flat β the number means little, trust the trend Β· < 1008 low β unstable, cloud & storm risk. A value rising run-to-run beats a pretty cloud map; falling pressure means cloud may arrive even if the sky looks good now. See the whole field with (H/L centres marked) β full interpretation in the .
The one-page brief
Totality crosses northern Spain 12 August 2026, ~20:26β20:31 CEST. In the Castilla y LeΓ³n focus area the Sun will be very low β about 10β11Β° up toward LeΓ³n, 7β9Β° over the plains, ~7Β° in Soria β sinking toward the west-north-west (azimuth β 281β284Β°). Sunset follows totality by roughly 50β60 minutes. Your #1 job: a completely unobstructed horizon toward WNW, and a sky that is clear at that horizon.
Everything below is grouped by topic β tap a section to open it. The living, spot-specific schedule (contact times, filter alarms, gear deadlines) is in the .
β±Key times & alarmsC1 β C4 in CEST, and the two alarms that protect your eyes and gear
| β 19:29β19:36 | First contact (C1) β partial phase begins |
|---|---|
| β 20:27β20:31 | TOTALITY (C2βC3) β up to 1 m 48 s on the centre line (Melgar de Fernamental); 1 m 40 s+ across most of the LeΓ³nβPalenciaβBurgosβSoria plains |
| β 21:12β21:25 | Partial ends (C4) β in the far east the Sun sets still partially eclipsed |
- β° Alarm #1 β C2 β15 s: FILTERS OFF. Camera filter comes off for totality; glasses stay on until the last Baily's bead dies.
- β° Alarm #2 β C3 β10 s: FILTERS BACK ON. This is the one that damages eyes and sensors if you miss it. Set both alarms on your phone the moment you're parked.
Exact contact times shift by a few minutes across the band. The computes them (to the second) for your chosen spot, including the two alarm times ready to copy into your phone.
βοΈWeather β maps, models & pressureOne-tap cloud tools Β· where the good odds are Β· which model to trust when
Cloud & eclipse tools β one tap
Where the weather is (ERA5, eclipse hour, 26 yrs)
- Ebro valley (Zaragoza plain): 28β31%, ~60% clear. Sun ~5β6Β°. Flat, huge road network, easy repositioning along A-2/A-68/AP-68.
- South Meseta edge of the track (Guadalajara, E Madrid): ~30β33%, sun ~6β7Β°, short-ish totality (near southern limit) β trade duration for sky.
- North Meseta (LeΓ³nβPalenciaβBurgosβValladolid): 32β38%, ~50β55% clear, longest durations (100β110 s) and the highest Sun (8β11Β°).
- Asturias & Cantabrian coast: 50β66% cloud β the longest totality on paper, the worst odds in practice. Only go with a locked-in clear forecast.
Which weather model to trust (and how to read it)
Weather apps blend many models; on eclipse day the differences matter. The number after each name is the grid size β smaller grid = sees smaller clouds, but only close to the event:
| AROME-HD 1.3 km AROME 2.5 km | The day-of king (β€ 2 days out). The only models fine enough to place valley fog, coastal stratus sneaking under the Cantabrians, and single convective cells over the mountains. Available in this app's Live tab and on meteoblue/Windy. |
|---|---|
| ECMWF 9 km | The planning king (2β10 days out). Statistically the best global model β use it to pick your region and watch how its eclipse-hour cloud map shifts run to run. If ECMWF and AROME agree on the day, trust them. |
| ICON-EU 7 km / ICON 13 km / NEMS 4 km / ALADIN 2.3 km | Good second opinions. When they all agree with ECMWF, confidence is high; when they scatter, the pattern is unstable β favour mobility over a "perfect" spot. |
| GFS 22 km | Coarse β use only for the long-range trend (it reaches 16 days first). Never trust GFS alone for cloud detail. |
- Read layers, not the total %: low cloud kills the view; thin high cirrus often doesn't (but smears the low sun). The Map tab's forecast overlay draws all three decks at once along the totality band β low = red, mid = green, high = violet. A single deck paints as continuous cloud; where decks overlap, thin vertical bars alternate their colours. It follows the model selector: pick ECMWF to see what Windy shows, ICON-EU for Ventusky, AROME-HD within ~2 days. Zoom in β or tap a spot to draw its sight-line β and the overlay re-samples just that window at up to ~3 km (dashed outline): on "Best match" the window automatically tries AROME-HD 1.3 km and falls back until its ~2-day horizon reaches the date, so the map sharpens itself as eclipse day approaches.
- Read the right hour: 20:00β21:00 CEST. A "sunny day" forecast is irrelevant if a sea of stratus rolls in at 20:15.
- Read the trend: a spot that improves in each successive run beats a slightly better spot that worsens.
- On the day, do it in the Live tab: the dataset matrix asks every model at once for your spot and every tapped point (the Β± column is the spread), and the βββ column weighs the layers where your sight-line actually crosses them.
Pressure: why "high" is your friend
Yes β surface pressure matters a lot. A high-pressure area (anticyclone, β³ 1020 hPa) means slowly sinking air, which suppresses convection, dries the mid-levels and typically delivers cloudless evenings β exactly what you want at 20:30. Watch for the Azores High extending a ridge over Iberia in the days before: that is the classic clear-eclipse setup.
How to read the number
| β₯ 1022 hPa | Strong high β subsiding air kills convection and dries the mid-levels. The clear-sky machine; commit with confidence. |
|---|---|
| 1015β1021 | Weak high / neutral β usually fine on the August Meseta, but check the cloud decks; a weak ridge can still let cirrus through. |
| 1008β1014 | Flat β the absolute number tells you little here. Read the trend and the model cloud maps instead. |
| < 1008 hPa | Low β unstable airmass: fronts, spreading cloud shields, evening storms. Favour mobility and the driest region on the track. |
- Trend beats snapshot. Pressure rising day over day = a ridge building = improving odds, even if today's cloud map looks mediocre. Falling = a trough approaching = deteriorating, even under a currently blue sky. The Live tab shows the same-day trend since 14 h next to the 20 h value.
- Highs and lows steer the clouds: air flows clockwise around an H and counter-clockwise around an L β so with an H east of you and an L west, expect southerly flow dragging cloud north. Where your spot sits relative to the centres matters as much as the number.
- Two Iberian caveats: (1) a summer high can still trap low marine stratus ("nortada") against the north coast β another reason to stay on the southern plains; (2) the hot interior breeds a shallow thermal low (~1010 hPa) on August afternoons β that one is heat-driven and mostly harmless, but it can spark isolated evening storms over the mountains.
- Where to see it in this app: Live tab β the hPa column in the dataset matrix (every point, selected model) and the pressure + trend line under the hourly decks; Map tab β the β― hPa overlay paints the whole field at 20:00 CEST with the H/L centres marked.
πPicking the exact spotLow-Sun rules: horizon math, facing WNW, elevation, haze
- Horizon math: at Sun altitude h, an obstacle of height H blocks it if closer than H / tan(h). At 6Β° a 20 m tree line must be β₯ 190 m away; a 200 m ridge β₯ 1.9 km away. At 3Β° double all that.
- Face WNW (az β 285Β°). Choose east rims of wide valleys, west-facing slopes, mesa edges, reservoirs' east shores, or the sea on a west coast.
- Get modest elevation over flat land β 50β200 m above the plain lifts you over haze and heat shimmer near the horizon. Avoid summits above ~1,400 m: August afternoons breed convective cloud on the peaks themselves.
- Avoid north-facing slopes, forest clearings, deep valleys, and city skylines to your west.
- Dust/haze: the low Sun shines through a long slab of atmosphere β a dry, haze-free airmass matters almost as much as cloud. Check aerosol/Calima forecasts on the day.
- Scout at the right time: the map's β° horizon simulator and the β verdict view flag terrain blocks β but nothing beats standing on the spot at ~20:30 on any prior evening: same Sun altitude, same direction, same haze.
π·Photography β shooting a 9Β° eclipseGeneral technique + the full Canon 1200D & iPhone 16 field guide
The low sun is a gift: at ~9Β° altitude you can frame the eclipsed Sun WITH the landscape β silhouettes, ridgelines, human figures β instead of a dot in an empty sky.
- Exposure bible: use Xavier Jubier's exposure calculator β pick aperture/ISO, read off shutter speeds for every phase (partials with filter, diamond ring, chromosphere, corona 0.1β8 solar radii, earthshine).
- Partial phases: certified solar filter over the lens. Remove it only seconds before C2 β and put it back at C3.
- Totality: no filter. Bracket wildly β corona brightness spans 10+ stops. Automate if you can; you'll want your eyes on the sky.
- Focal lengths: 500β1000 mm for the corona close-up (tripod + no shake), 24β70 mm for the money shot here: eclipsed Sun + glowing horizon + landscape. A second body/phone on a wide tripod shot, started before C2, is the low-effort winner.
- Timer app: Solar Eclipse Timer (iOS) talks you through every contact for your exact GPS spot β "filters off", "diamond ring", "filters on" β so you never miss a phase while shooting.
- Practice the full sequence once at 20:28 CEST on any clear evening: same sun altitude, same light.
Field guide β Canon EOS 1200D + EF-S 18-55 IS II & iPhone 16
Checked and folded in from the kit-specific field guide. Assumed lens: EF-S 18-55 mm f/3.5-5.6 IS II, 58 mm filter thread β verify by reading the ring on the front of the lens. Exposure values are starting points from standard practice, not measured with your filter; nothing here substitutes for a test on the real Sun days before. Dated deadlines (buy β build β test) are wired into the .
π― What this kit can and cannot do
| Frame-filling solar disc | No. At 55 mm on APS-C the Sun is ~120 px across on the 18 MP sensor (a 0.53Β° subject in a 22.9Β° horizontal field). |
|---|---|
| Wide-field corona + landscape + horizon glow | Yes. Corona out to 2β3 solar radii spans roughly 350β500 px. This is the shot worth planning for β and the low Spanish Sun makes it better than at most eclipses. |
| Filtered partial-phase timelapse | Yes. Easiest win in the whole plan. |
| iPhone corona still | No. The base iPhone 16 has main + ultrawide only, no telephoto. 24 mm-equivalent produces a white dot. |
| iPhone wide video of the light collapse | Yes. Arguably the most rewatched footage anyone gets. |
Plan accordingly: the DSLR shoots the wide-field scene, the phone shoots video, and you spend the majority of totality looking at it with your own eyes.
β οΈ Filter safety β read before anything else
- Full-aperture filter on the front of the optic. Never behind, never at the eyepiece.
- Never use the 1200D optical viewfinder with the Sun in frame, filtered or not. Live View only.
- Filter comes off only during totality. Back on the instant the diamond ring reappears. Partial phases are exactly as dangerous as an ordinary day.
- Eclipse glasses β camera filter. You need both; they are different products.
- Never OD 3.8 ("FOTO" grade) for anything your eye might meet: it transmits ~16Γ more light than OD 5.0 and is photographic-only. Buy OD 5.0 β or Baader's newer ClearWhite OD 5.1, its direct successor (both meet ISO 12312-2).
- Do not use: stacked ND filters, welding glass below shade 14, exposed film, smoked glass, CDs, sunglasses, polarisers. Standard ND does not block infrared.
π Shopping list (Geneva area)
| Baader AstroSolar film, A4 (20Γ29 cm), OD 5.0 Γ2 | Optique Perret, Geneva (~30 min from Annemasse) β phone ahead to confirm physical stock. CHF 30/sheet is at or below the EU benchmark (EUR 29 FR β 36 DE): fair, unusually good for Swiss retail. |
|---|---|
| Eclipse glasses (ISO 12312-2) Γ1β2 | Same shop β they stock Bresser. |
| Wired remote β Canon RS-60E3 or clone | Any photo shop, ~EUR 8β25. 2.5 mm sub-mini jack (fits the 1200D). |
| Tripods Γ2 | Own / borrow β one per camera. |
| Black card, craft knife, matte black tape, adhesive foam strip | Any DIY shop β for the filter cells. |
- Buy two sheets. The second is insurance against the pinhole you find during inspection β CHF 30 buys more risk reduction than any price-shopping, and you cannot reorder in the last week.
- Fallbacks if Perret is out: Optique Unterlinden (Colmar, ~EUR 29, usually in stock) β Astroshop.de / Teleskop-Express.de (3β5 days to France). Pierro-Astro's small ECO sheet is cheapest (~EUR 15.50) but shows hors stock, 1β4 semaines β too slow to rely on.
π§ Building the filter cells (Canon + iPhone)
One A4 sheet (20Γ29 cm = 580 cmΒ²) covers both builds several times over. Cut generously. Baader's own mounting instructions ship with the film β follow theirs over these where they differ.
Universal rules
- Film mounts loose, slightly wrinkled β never drum-tight. Tension distorts the optical wavefront; a visible ripple is correct and does not degrade the image.
- Handle by the edges only. Fingerprints and creases in the coating are defects.
- Friction fit over the outside of the optic, never a screw thread β a slip-on cell cannot unscrew itself mid-shot.
- Tape everything matte black on the inside to kill internal reflections.
- Inspect against a bright lamp before every use. Any pinhole, scratch or crease that transmits light β discard that piece and cut a fresh one.
Canon lens cell (58 mm thread, ~60 mm outer barrel)
- Cut two card rings: outer Γ 80 mm, inner aperture Γ 62 mm. The aperture must clear the full front element with a few mm margin β you are not stopping the lens down.
- Cut a film square ~85Γ85 mm.
- Sandwich: ring β film (loose) β ring. Tape the perimeter. Do not stretch.
- Cut a card strip ~25 mm wide, long enough to wrap the lens barrel; line the inside with foam. Roll to a snug slip fit β firm enough not to fall off pointing down, loose enough to pull off in one motion.
- Tape the collar to the ring sandwich.
- Safety tether: a loop of string from the cell to the tripod head β if it drops during totality it must not roll away in the dark.
- Test: point at a bare lightbulb and check Live View β you should see the filament and near-black surround. Stray light around the collar β add foam.
iPhone 16 plate
- The phone build is a plate covering the entire rear camera island, not one lens. Measure your actual island with a ruler β both lenses and the flash β not a spec sheet.
- Cut a card plate ~20 mm larger than the island on every side; cut one single window spanning both main and ultrawide with a few mm margin β one window, no alignment risk.
- Mount the film loose behind the window, same sandwich method.
- Attach with removable tape or an elastic band around the body. Nothing adhesive touches the lens glass.
- Why cover both lenses: the phone switches to the ultrawide automatically at certain zoom levels β an uncovered ultrawide means an unfiltered Sun, blown exposure, wrecked shot.
Reality check: even filtered, the partial Sun at 24 mm-equivalent is a tiny bright dot β the phone filter is a novelty-shot nice-to-have. The phone's real job is unfiltered wide video of the landscape, filter off, pointed away from the Sun.
βοΈ Canon 1200D settings & exposures
Setup (at home, not in the field)
- Mode M, format RAW β you need the latitude for the corona.
- Manual focus. AF fails on a filtered Sun. Focus at 10Γ Live View on a sunspot or the lunar limb, then tape the focus ring β the 18-55's infinity stop is not reliable.
- White balance Daylight (~5200β5500 K), manual. Auto WB drifts badly as the light collapses.
- IS off on the tripod. Wired remote or 2 s self-timer.
- The 1200D has no built-in intervalometer, and AEB is limited to Β±2 EV / 3 frames β insufficient for totality. Bracket manually by turning the shutter dial.
- Drift: at 88 mm-equivalent the Sun moves ~1 px/second on this sensor. Exposures up to ~2 s trail negligibly on a static tripod β you are not shutter-limited.
Partial phases β FILTER ON
f/8 Β· ISO 100 Β· 1/125 β 1/500 s as the starting bracket. Test on the real Sun days beforehand with your actual filter β transmission varies by an order of magnitude between products. Bracket Β±2 EV, read the histogram, write the working value on tape stuck to the camera.
Totality β FILTER OFF
Dynamic range spans roughly 12 EV. Fix aperture and ISO, vary shutter only: f/5.6 (wide open at 55 mm) Β· ISO 400.
| 1/2000 β 1/500 | Diamond ring, chromosphere, prominences |
|---|---|
| 1/250 β 1/60 | Inner corona |
| 1/30 β 1/8 | Mid corona |
| 1/4 β 1 s | Outer corona, earthshine on the lunar disc |
- Add ~1 EV when the Sun is below ~10Β° altitude (atmospheric extinction) β in Spain it will be, everywhere on the track.
- Rehearse the dial sequence blind. Spanish totality is ~1 m 40β48 s (the eclipse's global maximum, ~2 m 18 s, happens near Iceland β not here).
π± iPhone 16 plan
- Second tripod, locked off, wide, started before C2, then left completely alone.
- Lock AE/AF before totality (long-press on screen). Otherwise the phone auto-brightens and destroys the darkness you're trying to record.
- Point at the landscape and horizon, not the Sun: the 360Β° twilight ring, the light collapse, the crowd reaction, shadow bands on a white sheet.
- Filter on only for a partial-phase novelty frame; off for totality video.
- Never digital-zoom; grab stills during totality only if it doesn't cost you the view.
β Pre-eclipse checklist (tap to tick β it remembers)
Now (by 26 Jul)
Within 48 h of the film arriving
Two weeks out (by 1 Aug)
Day before (11 Aug)
On the day
π₯ Known failure modes
| Filter falls off mid-totality | Snug foam collar + string tether to the tripod |
|---|---|
| Forgot to remove filter at C2 | Alarm set to C2 β15 s |
| Forgot to replace filter at C3 | Alarm set to C3 β10 s. This one damages equipment and eyes. |
| Focus drifted | Tape the ring after setting. Verify at 100% on a test frame, not on the rear screen. |
| Phone auto-brightened the darkness away | AE/AF lock before C2 |
| Lost the whole event to fumbling | Rehearse blind. Accept fewer frames. |
| Battery died | Spares in a warm pocket |
| Horizon obstruction at low Sun | Site scout at the correct time of day |
πGetting there & moving on the dayRoutes north from Salamanca onto the track, day-of driving, and the post-eclipse jam
You are leaving from Salamanca β which sits at 99.7% partial, just outside the southern limit, so you must drive north onto the track. The good news: from here the northern Meseta β the best-odds and longest-duration zone β is your nearest totality, 1β2.5 h up the A-62 "AutovΓa de Castilla", which threads Salamanca β Tordesillas β Valladolid β Palencia β Burgos, running straight into the path.
Getting to the track (drive times from Salamanca)
- Palencia β closest full-value totality: A-62 via Valladolid, ~150 km / ~1h45, ~102 s, Sun ~8.6Β°. Valladolid is nearer (~110 km / ~1h10) but sits near the southern edge (~87 s) β fine as a bad-weather fallback, but push on to Palencia for the real thing.
- LeΓ³n β highest Sun, longest: A-66 "Ruta de la Plata" via Zamora β Benavente β LeΓ³n, ~180 km / ~2 h, ~105 s, Sun ~9.6Β° β the best altitude anywhere on the track.
- Melgar de Fernamental β the centre line / max duration: A-62 to Palencia then north-east toward Melgar, ~200 km / ~2h15, ~106 s. Burgos is a little further on the same A-62 (~225 km / ~2.5 h, ~104 s).
- Aranda de Duero / Duero valley (eastern CyL): A-62 to Valladolid then A-11 "AutovΓa del Duero" east, ~180 km / ~2 h, ~102 s β the drier, more continental side if the western Meseta clouds over.
- Ebro valley (driest climatology, but far): ~500 km / ~5 h east (A-62 to Burgos, then A-1). Only worth it if the whole Meseta forecast collapses and the Ebro is locked clear β decide the night before, it is a long haul.
- Skip the Cantabrian coast from here: over the mountains and the worst cloud odds on the track β only with a locked-in clear forecast.
- Let the forecast pick the field. Salamanca as a base keeps the entire western + central track (LeΓ³n β Burgos) reachable in a morning's drive, so you don't have to commit to a town until the day.
On eclipse day (out of Salamanca)
- Full tank in Salamanca the evening before β stations near the line will queue. Water (2 L+/person), food, hat, sunscreen: August Meseta, 35 Β°C+ in the afternoon; bring a warm layer for after sunset.
- Leave early β be on the track by Tβ3 h (β 17:30). Your spine is the A-62; the A-231 LeΓ³nβBurgos corridor hugs the centre line and will be the busiest road in Spain that evening.
- Download offline maps (and screenshot your Timeline): mobile networks near the centre line may collapse under the crowd.
- Never watch from the road shoulder β illegal, dangerous, and where eclipse-day accidents happen. Park in a field entrance, village, or mirador; park facing your exit.
- Check DGT live traffic before every leg β it's linked from each Timeline step too.
- Plan the drive back south to Salamanca after dark. The 2017/2024 US eclipses jammed roads for hours the instant totality ended. Watch the partial to sunset, eat where you are, then drive home late.
πWhat to look for during the eclipseSafety rules, and the show minute by minute β before, during, after totality
Safety, always
- Eclipse glasses (ISO 12312-2) for every partial phase; naked eyes and unfiltered optics only between C2 and C3. Binoculars on the corona are stunning β but only inside totality.
The last hour (partial phase)
- Crescent projections: gaps in foliage, a colander, or crossed fingers project hundreds of little crescent Suns that thin as C2 approaches.
- The light goes wrong: shadows sharpen along one axis, daylight turns silvery-metallic, temperature drops noticeably, and a faint "eclipse wind" often picks up.
- Venus (mag β4) pops out ~15β20 min before totality, ~46Β° upper-left of the Sun. Animals hush; swallows go to roost.
- The umbra wall: in the last minutes the WNW horizon visibly darkens β that is the Moon's shadow arriving at ~2β3 km/s. From any elevated spot you can watch it race at you.
- Shadow bands: in the final 1β2 minutes faint rippling grey bands may slither over light ground and walls β rare and subtle; spread a white sheet to catch them.
Totality (~1 m 40 s)
- Diamond ring β Baily's beads as the last sliver breaks through the lunar valleys β glasses off as the last bead dies.
- The corona: 2026 comes just after solar maximum, so expect a full, petal-rich corona with streamers all around the disc, plus the red chromosphere rim and, very likely, prominences.
- Planets appear: Venus blazing high upper-left, Jupiter ~10Β° lower-right of the Sun, Mercury ~15Β° right and very low, the star Regulus ~10Β° upper-left. The β° horizon simulator draws them all in place for your spot.
- Look down and around too: a 360Β° sunset ring on every horizon (this low Sun makes it exceptional), eerie landscape colours, the crowd. Budget your ~100 seconds: corona β landscape β corona.
After C3
- Second diamond ring (filters straight back on), a second chance at shadow bands, then the whole partial sequence in reverse β with the Sun sinking toward a normal sunset ~50β60 min later, still crescent-scarred in the east of the track.
π§Day-of playbookThe four decisions, Tβ48 h to Tβ90 min
- Tβ48 h: compare every model in the Live tab's dataset matrix. Pick a primary region and a fallback β₯150 km along the track.
- Morning of: re-run the best-places ranking in the Live tab. Watch real clouds on the map's live satellite overlay (updates ~every 10 min).
- Tβ3 h: commit. Convective cloud builds over mountains in the afternoon β if in doubt, move toward the flat, dry side (from Salamanca: the Duero valley toward Aranda, or the Ebro basin as a far fallback β not the Cantabrian mountains).
- Tβ90 min: be parked. Set up and focus during the partial phase with time to spare; set the two filter alarms. Totality waits for no one.
The full dated version β with computed times for your spot β is the .
πSources & further toolsOfficial maps, climatology, exposure calculators, live satellites
- Eclipsophile β climatology deep dive (J. Anderson)
- NASA GSFC β interactive path map & Besselian elements
- ESA β official map of totality in Spain
- TheSkyLive β per-town circumstances
- Tres Eclipses (ES) β official Spanish eclipse app
- timeanddate β city times
- Junta de CyL β official observation points
- Eclipse Soria β province guide (Starlight skies)
- Hosteltur β best miradores round-up
- eclipse-solar.es β location guide
- WeatherAway β eclipse cloud forecast with low-Sun cloud layers (multi-model)
- X. Jubier β solar eclipse exposure calculator
- Solar Eclipse Timer β voice countdown app for contacts (iOS)
- Windy β visual cloud forecast maps
- Ventusky β animated cloud-cover maps (total + low/mid/high, ICON/GFS)
- AEMET β official Spanish forecasts
- EUMETSAT β live satellite of W Europe
Data: eclipse geometry computed from NASA/GSFC Besselian elements (F. Espenak), ΞT = 69.2 s; verified against the NASA path tables to <0.1 s in duration. Cloud climatology: ERA5 reanalysis via the Open-Meteo archive API, mean total cloud at 18β19 UT on 10β14 Aug 2000β2025. Live forecasts: Open-Meteo (ECMWF/GFS/ICON). Live satellite & radar overlays: RainViewer. Elevations: Copernicus DEM via Open-Meteo. This tool is for planning; always sanity-check against official sources on the day.