Sun Path: Srinagar, India

Direct answer

For Srinagar at 34.0857, 74.8055, the declination-only solar-noon altitude is approximately 79.4° at the June solstice, 55.9° at an equinox and 32.5° at the December solstice. Refine these geometry checks with the project date, civil time, facade azimuth, terrain and local horizon. The reproducible location record is GeoNames ID 1255634 in administrative area 12, at 34.0857, 74.8055; replace it with the surveyed parcel point before relying on the result. As a transparent geometry check, declination-only solar-noon altitude is about 79.4° at the June solstice, 55.9° at an equinox and 32.5° at the December solstice. Representative 21st-day geometry ranges from about 9.7 hours in December to 14.3 hours in June; this excludes atmospheric refraction, terrain and obstruction effects. The cited national authority is a discovery starting point; current local documents and a named qualified reviewer control project use of this sun path record.

Prepared by Harth · Prepared from the cited location and country sources; local project inputs remain unreviewed · Published 2026-08-26 · Updated 2026-08-31.

What must be verified for Srinagar?

Srinagar is represented here at approximately 34.0857, 74.8055 for discovery and workflow planning. A project address, parcel, elevation, exposure, authority, and submission date must replace that city-centre reference before design use.

How should sun path be established?

1. Fix the surveyed site and local time basis.
2. Select an authoritative weather source or a named solar-position algorithm.
3. Record period, percentile or scenario and units.
4. Test sensitivity to elevation, exposure, urban form and horizon.
5. Save the source file, retrieval date and checker in the model record.

What are the limits of this worksheet?

This sun-path-workflow page is a project-starting worksheet, not a design value or approval. The controlling authority and qualified professionals for the Srinagar site remain authoritative.

Which related searches does this primary location record cover?

This primary route consolidates the location evidence needed for Sun Path, Solar Altitude & Azimuth, Solar Shading Design, Daylight & Orientation. A narrower route should be released only when it adds a materially different official source, calculation, process, threshold or worked example.

Srinagar monthly solar geometry check for sun path

Month-by-month geometry interpretation

• 21 January: approximate solar-noon altitude 35.8° (zenith angle 54.2°) and 10.1 hours of geometric daylight. That is 0.4 hours longer than the preceding representative date in this annual sequence.
• 21 February: approximate solar-noon altitude 44.7° (zenith angle 45.3°) and 11.0 hours of geometric daylight. That is 0.9 hours longer than the preceding representative date in this annual sequence.
• 21 March: approximate solar-noon altitude 55.5° (zenith angle 34.5°) and 12.0 hours of geometric daylight. That is 1.0 hours longer than the preceding representative date in this annual sequence.
• 21 April: approximate solar-noon altitude 67.5° (zenith angle 22.5°) and 13.1 hours of geometric daylight. That is 1.1 hours longer than the preceding representative date in this annual sequence.
• 21 May: approximate solar-noon altitude 76.1° (zenith angle 13.9°) and 13.9 hours of geometric daylight. That is 0.9 hours longer than the preceding representative date in this annual sequence.
• 21 June: approximate solar-noon altitude 79.4° (zenith angle 10.6°) and 14.3 hours of geometric daylight. That is 0.4 hours longer than the preceding representative date in this annual sequence.
• 21 July: approximate solar-noon altitude 76.4° (zenith angle 13.6°) and 13.9 hours of geometric daylight. That is 0.3 hours shorter than the preceding representative date in this annual sequence.
• 21 August: approximate solar-noon altitude 67.7° (zenith angle 22.3°) and 13.1 hours of geometric daylight. That is 0.9 hours shorter than the preceding representative date in this annual sequence.
• 21 September: approximate solar-noon altitude 55.7° (zenith angle 34.3°) and 12.0 hours of geometric daylight. That is 1.1 hours shorter than the preceding representative date in this annual sequence.
• 21 October: approximate solar-noon altitude 44.2° (zenith angle 45.8°) and 10.9 hours of geometric daylight. That is 1.1 hours shorter than the preceding representative date in this annual sequence.
• 21 November: approximate solar-noon altitude 35.5° (zenith angle 54.5°) and 10.1 hours of geometric daylight. That is 0.9 hours shorter than the preceding representative date in this annual sequence.
• 21 December: approximate solar-noon altitude 32.5° (zenith angle 57.5°) and 9.7 hours of geometric daylight. That is 0.3 hours shorter than the preceding representative date in this annual sequence.

Harth calculation for latitude 34.0857°: Cooper declination approximation, 90° - |latitude - declination| at solar noon, and centre-to-centre sunrise hour angle. See NOAA's solar calculation details for fuller method context. This screening table excludes equation-of-time/civil-time conversion, atmospheric refraction, terrain, facade azimuth and obstructions; it is not an hourly shading result.

Where can you explore related guidance?

• Explore all solar data guidance
• Sun Path: Amritsar, India
• Sun Path: Ludhiana, India
• Sun Path: Meerut, India
• Sun Path: Najafgarh, India

Sources and method

Location data from the GeoNames IN dump (CC BY 4.0, snapshot 2026-08-31, GeoNames ID 1255634). Regulatory starting point: Bureau of Indian Standards and the applicable state or urban local body. Figures are illustrative — verify against the current locally adopted edition for the site. Solar-method context: NOAA Solar Calculation Details; the Harth monthly table uses a simpler declination and geometric-daylight approximation whose stated limitations must be retained.

Source links

• download.geonames.org

• services.bis.gov.in

• gml.noaa.gov