Length of the Night

as an interval between the PM and AM moments of Sun passing a given angular height (default -6°, for the ``civil night''):

Year:   Month:   Day:
Longitude: (western as -)   Latitude:
Your Time - UTC:  h
The relevant angular height of Sun is degrees
next days will be computed as well,
with a step of day(s).
   save settings    use my saved settings

Another option is to use your own command line (ev. overriding all previous data):

(`?' gives help). 

The centre of Sun is at a place with coordinates [Lambda=16.6°, Phi=49.2°]
 in an angular height of h =-6.0°
 in the following morning and evening moments (given in UTC+ 1h):

 year-month-day  morning evening twilight decl.  >mean  night   A-W
                       h:min     / 1 min   /1°   /1min   /1h    /1°
2026-10- 5 Monday   5:28  17:56   31.9   -4.83    11.6  11.52   -0.4
         6 Tuesday  5:29  17:54   31.9   -5.22    11.9  11.58   -1.0
         7 Wednesd  5:31  17:52   32.0   -5.60    12.2  11.64   -1.6

Average for   3 days
from   3 values is  5:29  17:54   31.9   -5.21    11.9  11.58   -1.0

Meaning of remaining columns:
 Twilight    is an interval to/from h=-0.8°
 Declination of Sun is given for the moment of local mean noon,
 >Mean       says how much is the Sun ahead of the mean time,
 Night       is the time the Sun travels below h,
 A-W         is departure of solar azimuth from the west when at h afternoon.

This is a result of the programme nights (available as a part of a package pas_jh.zip (1.2 MB) -- the needed Pascal units themselves are unzipped within this directory, the whole tree of my programmes within this directory) with a command line: 
nights  d05.10.2026 t22:20 l16.6 f49.2 ut1  h-6 n2 i1