Solar Path Tracker

Solar guide · Directional shot plan

Golden Hour Direction in Brisbane

Place a camera for front, side, or back light using Brisbane’s reproducible winter and summer golden-hour bearings.

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Solar Path Tracker · Editorial and technical review by the site maintainer
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A golden-hour time without a direction is incomplete planning information. The Sun may be low and warm, yet sit behind the subject, behind the photographer, or behind a blocked horizon. Combining the window with its azimuth explains which side of a scene is geometrically positioned for direct low-angle light.

Solar Path Tracker defines the morning window from sunrise until the Sun reaches +6° altitude, and the evening window from +6° down to sunset. This is an astronomical boundary, not a guarantee of colour. Atmosphere, cloud, smoke, haze, terrain, buildings, trees, and exposure choices shape the visible result.

These windows use SunCalc event-time estimates. Boundary altitudes are calculated separately with its position formula, so displayed values can differ slightly from the nominal +6° threshold. Standard sunrise and sunset also use a horizon/refraction convention and do not require a displayed altitude of 0°.

Read the beginning and end as two bearings

The Sun continues moving throughout a golden-hour window. The starting bearing and ending bearing therefore form a directional span rather than one fixed compass point. A location with a narrow opening between buildings may receive only part of the calculated window.

Morning light approaches from the eastern side of the sky and evening light from the western side, but the north-south component changes by season. That seasonal movement can decide whether a city street, river edge, facade, or landscape has a clear line of sight.

Use altitude to anticipate shadow character

Between 0° and 6°, direct rays meet level ground at a shallow angle. Unobstructed vertical objects cast long shadows, and small changes in terrain or skyline height can remove the direct beam entirely.

The main Solar Path Tracker labels whole-hour samples between 0° and 6° as an approximate golden state. The dedicated Golden Hour Calculator uses the exact SunCalc event boundaries, so it is the appropriate tool for start and end times.

These are fixed seasonal reference dates, not the exact local dates of the solstices or equinoxes.

Directional shot plan

Brisbane winter and summer directional shot plan

This fixed planning sheet applies Solar Path Tracker’s explicit definition: morning golden hour runs from sunrise to +6° altitude, and evening golden hour runs from +6° altitude to sunset. The live calculator handles other dates and locations; this guide focuses on repeatable field preparation for Brisbane’s two seasonal reference dates.

Brisbane golden hour boundary bearings for winter and summer
SeasonWindowBoundaryTimeDirectionAltitude
Winter reference2026-06-21MorningStart06:3863.7° North-east-0.6°
Winter reference2026-06-21MorningEnd07:1359.5° North-east6.2°
Winter reference2026-06-21EveningStart16:27300.2° North-west5.8°
Winter reference2026-06-21EveningEnd17:02296.1° North-west-1.0°
Summer reference2026-12-21MorningStart04:50117.0° South-east-0.6°
Summer reference2026-12-21MorningEnd05:24113.2° South-east6.2°
Summer reference2026-12-21EveningStart18:09246.6° South-west5.8°
Summer reference2026-12-21EveningEnd18:43242.8° South-west-1.0°
Golden hour field compassA compass measured clockwise from true north with example arrows toward the north-east and north-west quadrants. Exact bearings are provided in the table.NESW
Use true-north bearings from the table. Arrive before the first boundary, check the actual horizon, and allow for cloud and setup time.

Calculated example — not a field measurement

A task you can reproduce

Use the winter-reference evening golden-hour bearing to place a camera for front, side, or back light, then compare that setup with the summer direction.

Observation point
Brisbane, Queensland, Australia
Coordinates
-27.4698°, 153.0251°
Timezone and model
Australia/Brisbane · SPT-SUN-V1
Reference dates
2026-06-212026-12-21

Place the camera around the subject

The winter evening window begins at 16:27, with the Sun at 300.2° North-west. Each diagram keeps that calculated Sun direction fixed and changes only the camera position.

Front light

Keep the camera on the Sun-facing side of the subject, with the Sun generally behind the photographer.

Front light camera placement for a winter evening Sun bearingA top-down relative-position diagram. The subject is in the centre, the Sun is at a bearing of 300.2 degrees, and the camera is at 300.2 degrees. Amber shows incoming light and the dashed blue line shows the camera view toward the subject.TRUE NORTHSUNCAMSUBJECTCamera bearing 300.2° · relative layout only
Sun 300.2° North-west; camera 300.2° North-west relative to the subject.

Side light

Move the camera about 90° around the subject so the direct light crosses the frame from one side.

Side light camera placement for a winter evening Sun bearingA top-down relative-position diagram. The subject is in the centre, the Sun is at a bearing of 300.2 degrees, and the camera is at 30.2 degrees. Amber shows incoming light and the dashed blue line shows the camera view toward the subject.TRUE NORTHSUNCAMSUBJECTCamera bearing 30.2° · relative layout only
Sun 300.2° North-west; camera 30.2° North-east relative to the subject.

Back light

Place the camera opposite the Sun, leaving the subject between the camera and the incoming light.

Back light camera placement for a winter evening Sun bearingA top-down relative-position diagram. The subject is in the centre, the Sun is at a bearing of 300.2 degrees, and the camera is at 120.2 degrees. Amber shows incoming light and the dashed blue line shows the camera view toward the subject.TRUE NORTHSUNCAMSUBJECTCamera bearing 120.2° · relative layout only
Sun 300.2° North-west; camera 120.2° South-east relative to the subject.

Read the winter span

From 16:27 to 17:02, the Sun moves from 300.2° North-west to 296.1° North-west. Treat the setup as a moving directional range, not one permanent arrow.

Recheck in summer

The summer evening window starts with the Sun at 246.6° South-west, in a different compass sector from winter. Recalculate the camera plan instead of reusing the winter placement.

Reproduce the case

  1. 1. Open the Golden Hour Calculator.
  2. 2. Enter the coordinates shown in the case inputs and select the winter-reference date.
  3. 3. Read the Evening golden hour start and end times, bearings, and altitudes.
  4. 4. Use the winter start bearing to choose the relative camera setup shown in the diagrams.
  5. 5. Check the real horizon before the window begins, then repeat with the summer-reference date rather than reusing the winter direction.

Assumptions and stop conditions

  • The diagrams show relative positions around one subject and are not maps of a real location.
  • All directions are true-north bearings measured clockwise from north.
  • The Sun is treated as an unobstructed direction; skyline, terrain, weather, exposure, and lens choice remain field decisions.

Download the evidence dataset

Winter and summer SunCalc event boundaries: sunrise to the morning +6° event, and the evening +6° event to sunset. The UTF-8 CSV uses a fixed column order and contains calculated values only.

Plan a location check before the shoot

Plot or stand facing the boundary bearing, then inspect whether the horizon is clear. For an evening shoot, arrive before the Sun falls into the 0–6° band so composition and exposure can be tested while the light is still changing.

For front light, place the photographer on the Sun-facing side of the subject, with the Sun generally behind the photographer. For backlight or rim light, place the subject between the camera and the solar bearing. These are compositional starting points, not safety guidance for viewing or photographing the Sun.

Responsible use

Practical uses and model limits

Terrain and buildings may be displayed in the 3D view for visual context where available. They are not inputs to the solar engine, which reports an unobstructed astronomical baseline without terrain, building, or tree shading.

Useful for

  • • Checking whether a city-street axis aligns with the low Sun.
  • • Planning front light, side light, or backlight for an outdoor portrait.
  • • Comparing winter and summer horizon access at the same Brisbane location.

Do not overlook

  • • The model does not forecast cloud, colour, aerosol, smoke, visibility, or camera exposure.
  • • It assumes an unobstructed astronomical horizon and does not use terrain elevation profiles.
  • • Never look directly at the Sun through an optical viewfinder or unapproved equipment.

Sources and reproducibility

Evidence and calculation sources

  • USNO Astronomical Applications API documentation

    Independent event-time reference used by the site validation report; the sunrise-to-+6° and +6°-to-sunset golden-hour windows are this site’s stated convention.

  • SunCalc

    Solar position and astronomical event calculations used by this site.

  • Luxon

    IANA timezone-aware conversion between the selected local time and UTC.

  • Solar Path Tracker methodology

    Definitions, angle normalization, polar handling, precision, and model limits.