The morning and evening twilight brightness are important to probe the properties of the upper atmosphere. We conducted a short survey of broad band twilight sky brightness measurements by using a portable photometer with 5 second resolution, in five places with different elevations. The darkest zenith sky brightness reached 22.9 MPASS. We found the complex twilight sky brightness variation and proposed 17 degree solar dip for Fajr prayer. The observable young crescent moon which has less than 24 hours in age has the sky brightness at the range of 8-16 magnitude/arcsec2. These correspond to telescope visual limiting magnitude of 2.9 to 9.3. The excellent quality of telescope is needed for this purpose to cope with very low contrast of young...
Photoelectric observations of twilight (evening and morning) Bahria (φ = 28° 42.94′ N, λ = 28° 59.99...
The indication of began to enter the shubuh prayer time is when emerge the morning dawn and lasted u...
This paper endeavor to describe sky brightness measurements which was carried out by a team of total...
The aim of this study is to detect elusive lightthat indicate the prayer time (Isha’). Therefore, we...
This paper summarizes ISRN’s 3-years research on the occurrence of dawn and dusk to mark the timing...
Based on data record of young lunar crescent (hilal) observations around the world, now we have basi...
The visibility of the thin crescent Moon is an important problem for the calendars of many societies...
The writer carried out sky brightness measurements at zenith on clear days beginning in March 2023. ...
In astronomy, there are three types of dawn. They are astronomical, nautical, and civil dawn. The su...
AbstractPhotoelectric observations of twilight (evening and morning) Bahria (φ=28° 42.94′ N, λ=28° 5...
The algorithm used to partition telescope time at ING into dark, grey and bright categories, which i...
Abstract The variable brightness of the night sky affects plants as well as animals and humans. Howe...
The main challenge in the young crescent moon (YCM) observation is the ability to detect the appeara...
Using the visible airglow photometer on the Atmosphere Explorer-C satellite, we have mapped the zodi...
Measuring the brightness of the night sky and determining the start of Fajr prayer times can be done...
Photoelectric observations of twilight (evening and morning) Bahria (φ = 28° 42.94′ N, λ = 28° 59.99...
The indication of began to enter the shubuh prayer time is when emerge the morning dawn and lasted u...
This paper endeavor to describe sky brightness measurements which was carried out by a team of total...
The aim of this study is to detect elusive lightthat indicate the prayer time (Isha’). Therefore, we...
This paper summarizes ISRN’s 3-years research on the occurrence of dawn and dusk to mark the timing...
Based on data record of young lunar crescent (hilal) observations around the world, now we have basi...
The visibility of the thin crescent Moon is an important problem for the calendars of many societies...
The writer carried out sky brightness measurements at zenith on clear days beginning in March 2023. ...
In astronomy, there are three types of dawn. They are astronomical, nautical, and civil dawn. The su...
AbstractPhotoelectric observations of twilight (evening and morning) Bahria (φ=28° 42.94′ N, λ=28° 5...
The algorithm used to partition telescope time at ING into dark, grey and bright categories, which i...
Abstract The variable brightness of the night sky affects plants as well as animals and humans. Howe...
The main challenge in the young crescent moon (YCM) observation is the ability to detect the appeara...
Using the visible airglow photometer on the Atmosphere Explorer-C satellite, we have mapped the zodi...
Measuring the brightness of the night sky and determining the start of Fajr prayer times can be done...
Photoelectric observations of twilight (evening and morning) Bahria (φ = 28° 42.94′ N, λ = 28° 59.99...
The indication of began to enter the shubuh prayer time is when emerge the morning dawn and lasted u...
This paper endeavor to describe sky brightness measurements which was carried out by a team of total...