Sunrise & Sunset
Sunrise and Sunset
- The tilt of spin axis of the earth with the orbital plane results in seasonal variation in duration of daylight
- The time of sunrise and sunset are affected by certain factors
- A combination of Sun’s Declination and observer’s latitude affects the duration of daylight
- Semi-diameter or radius of the sun also affects sunrise and sunset
- Refraction of light in the atmosphere increases daylight time
Effect of Sun’s Declination on Sunrise and Sunset
- Declination of the sun affects the time of sunrise and sunset
- Consider the sun’s position in summer during northerly declination of sun
- Sun’s northerly declination results in longer daylight in northern hemisphere
- Sun would be above horizon before sun reaches observer’s meridian
- Sun remains above horizon after sun crosses from observer’s meridian
- Sunrise is earlier than 0600 LMT and sunset is later than 1800 LMT
- Declination effect would reverse in the case of southerly declination of the sun
Effect of Latitude on Sunrise and Sunset
- Latitude of the observer affects the time of sunrise and sunset
- Consider the sun’s position in summer when sun’s declination is 23.5 North
- An observer at the Equator experiences equal periods of day and night
- An observer above 66.5° North experiences constant daylight
- An observer above 66.5° South experiences constant night time
- Latitude effect would reverse in the case of southerly declination of the sun
Semi-Diameter of Sun
- Semi-diameter of sun and atmospheric refraction affects sunrise and sunset
- Semi diameter of the sun is 16 minutes of arc
- Atmospheric refraction of 34 minutes of arc
Sunrise and Visual Horizon
- Sensible horizon is the horizon which is tangential to the earth surface while the visual horizon is 34 minutes below the sensible horizon
- Sun light is visible when the sun is below sensible horizon due to bending of light
- Centre of sun at sunrise is 16 minutes of arc below visual horizon
- Centre of sun at sunrise is 50 minutes below sensible horizon
- At sunrise and sunset times the sun is three minutes in terms of time below the horizon
Civil Twilight
- Twilight is the period of partial light before sunrise and after sunset
- Night flying starts from end of ECT to beginning of MCT
- Regulations prescribe half hour after sunset to half hour before sunrise
Morning and Evening Civil Twilight
- Evening civil twilight is the period of sufficient light after sunset
- ECT extends from sunset to sun at 6 degrees below sensible horizon
- Morning civil twilight is the period of sufficient light before sunrise
- MCT extends from sun at 6 degrees below sensible horizon to sunrise
Nautical and Astronomical Twilight
- Nautical twilight is the time when sky is dark but stars and planets are visible
- Centre of sun is between 6 to 12 degrees below sensible horizon
- Astronomical twilight is actually total darkness and only used by astronomers
- Centre of sun is between 12 to 18 deg below sensible horizon
Duration of Twilight
- Duration of twilight varies due a combination of the Declination of the sun and Latitude of the observer
- Altitude of the observer and Meteorological conditions also affect the twilight duration
Value of Civil Twilight Duration
- Civil twilight is at minimum value if observer and sun are at the equator
- Minimum time of civil twilight is 21 minutes at an angular distance of 5 degrees 10 minutes
Effect of Declination on Twilight
- Duration of twilight increases with increase in declination of sun
- Sun spends more than 21 minutes in the twilight zone at solstice
Effect of Latitude on Twilight
- Duration of twilight increases with increase in observer’s latitude
- Sun spends more than 21 minutes in the twilight zone
- Maximum duration is seen above Arctic and Antarctic circles
- Summer sun never sets or civil twilight extends until mid-night
- Winter sun never rises or civil twilight does not start until mid-noon
Effect of Altitude on Twilight
- Sunrise, sunset and twilight published in air-almanac are for mean sea levels
- Increase in altitude sun would rise early and set later due to increase in Visual horizon with altitude
- Therefore, increase in altitude results in a decrease in the duration of civil twilight
- Reduction in atmosphere at higher levels reduces refraction and hence duration of twilight
Effect of Scattering on Twilight
- Volcanic eruptions increase the duration of twilight due to increase in volcanic ash pollution
- Polluted atmosphere increases refraction due to scattering of light