Azan Time London Free Download

Islamic Prayer Times in London (UK) and Athan (Azan) with Namaz Time of Muslim Prayer Times (Salah Times) i.e. Fajr, Dhuhr, Asr, Maghrib, Isha in London.

Contents • • • • • • • • • • • • Definitions To determine the exact time period for each prayer (and also for fasting), we need to determine nine points of time per a day. These times are defined in the following table: Time Definition Fajr When the sky begins to lighten (dawn). Sunrise The time at which the first part of the Sun appears above the horizon. Dhuhr When the Sun begins to decline after reaching its highest point in the sky.

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Asr The time when the length of any object's shadow reaches a factor (usually 1 or 2) of the length of the object itself plus the length of that object's shadow at noon. Sunset The time at which the Sun disappears below the horizon.

Maghrib Soon after sunset. Isha The time at which darkness falls and there is no scattered light in the sky. Midnight The mean time from sunset to sunrise (or from sunset to Fajr, in some schools of thought). The next section provides information on how to calculate the above times mathematically for any location if the coordinates of the location are known.

Astronomical Measures There are two astronomical measures that are essential for computing prayer times. These two measures are the equation of time and the declination of the Sun. The equation of time is the difference between time as read from a sundial and a clock. It results from an apparent irregular movement of the Sun caused by a combination of the obliquity of the Earth's rotation axis and the eccentricity of its orbit. The sundial can be ahead (fast) by as much as 16 min 33 s (around November 3) or fall behind by as much as 14 min 6 s (around February 12), as shown in the following graph. The Declination of Sun The above two astronomical measures can be obtained accurately from The Star Almanac, or can be calculated approximately.

The following algorithm from computes the Sun's angular coordinates to an accuracy of about 1 arcminute within two centuries of 2000. D = jd - 2451545.0; // jd is the given Julian date g = 357.529 + 0.98560028* d; q = 280.459 + 0.98564736* d; L = q + 1.915* sin(g) + 0.020* sin(2*g); R = 1.00014 - 0.01671* cos(g) - 0.00014* cos(2*g); e = 23.439 - 0.00000036* d; RA = arctan2(cos(e)* sin(L), cos(L))/ 15; D = arcsin(sin(e)* sin(L)); // declination of the Sun EqT = q/15 - RA; // equation of time Calculating Prayer Times To calculate the prayer times for a given location, we need to know the latitude (L) and the longitude (Lng) of the location, along with the local Time Zone for that location. We also obtain the equation of time (EqT) and the declination of the Sun (D) for a given date using the algorithm mentioned in the previous section. Dhuhr Dhuhr can be calculated easily using the following formula. Sunrise = Dhuhr - T(0.833), Sunset = Dhuhr + T(0.833).

If the observer's location is higher than the surrounding terrain, we can consider this elevation into consideration by increasing the above constant 0.833 by 0.0347 × sqrt(h), where h is the observer's height in meters. Fajr and Isha There are differing opinions on what angle to be used for calculating Fajr and Isha. The following table shows several conventions currently in use in various countries (more information is available at ). Convention Fajr Angle Isha Angle Muslim World League 18 17 Islamic Society of North America (ISNA) 15 15 Egyptian General Authority of Survey 19.5 17.5 Umm al-Qura University, Makkah 18.5 90 min after Maghrib 120 min during Ramadan University of Islamic Sciences, Karachi 18 18 Institute of Geophysics, University of Tehran 17.7 14* Shia Ithna Ashari, Leva Research Institute, Qum 16 14 * Isha angle is not explicitly defined in Tehran method.