Observations of Sun light inside Treasury of Atreus
Use a good clock
When doing these observations it is important to have the time as
accurate as possible, so try to synchronize your clock
(watch/mobile/camera) with an accurate time source; like the time-peeps
on the radio/TV or some other accurate source (e.g. GPS or Internet
Time source). This link
provides the GTM time (same as UTC), which is three hours less then
Greek local
summer time [UTC+3].
Write in the below table the date and time and the amount of change
made,
when you adjust the time on your clock. Do this at least once; before
your start with your very first observation.
I would propose to check it every 5 days. If you think your clock is
changing very fast, say more then a few minutes in 7 days; do this
synchronization every 2 days; or better use another clock;-)
Below is a table that can be printed and used as a log sheet for the
time synchronization:
Date
of synchronization
[yyyy/mm/dd]
New
time [hh:mm:ss]
Change
made [sec]
Source
[radio/TV/GPS/Internet]
2007/08/29
2007/09/03
2007/09/08
2007/09/13
2007/09/18
2007/09/23
2007/09/28
2007/10/03
Finding the first day the Sun gets throught the triangular structure
When starting to observe a solar event in a monument, the first moment
that the Sun gets into the chamber is always difficult to predict
accurately from a model (due to possible inaccuracies when modeling the
triangular
structure). So one has to start looking from a certain date (I propose
August 30th, 2007) from around 08:00 local time [UTC+3]. Due
to these geometrical unknowns of the relieving triangular structure,
one needs to keep on looking until 9:15 local time [UTC+3].
Hopefully in this time period (between 08:00 and 09:15) the Sun light
peeps in the chamber. If not; one has to repeat this procedure each
day, until the
Sun light gets in the chamber. At that moment one has a better idea
when it starts and ends.
It is best to repeat the same time period (between 08:00 and
09:15) for the next two days, because the start time might be
much earlier then in the rest of the month (when 5
minutes is oke).
Make sure (look outside the chamber) that when the Sun light starts to
get in the chamber, it is not because clouds just went out of the way
of the Sun. Comparable with last Sun light; make sure (look outside
the chamber) that the Sun light did not stop due to clouds in front of
the
Sun.
As soon as one has had a good three observation
days, one can easily 'predict' the time for the next day; be there 5
minutes earlier then the start time on the previous day. In that case
one certainly does not miss the start of the event. The end time is
simple, just wait until the Sun light is gone from the chamber (check
that it is not due to clouds).
The observations
Below is a table that can be printed and used as a log sheet for the
observations. The green dates are the predicted dates (Sept. 1st
upto and including Sept 28th, 2007) that the sun could be in
the chamber, but again be prepared to be there a few days earlier
(proposed Aug. 30th, 2007) and a few days later (until
totally no Sun is visible anymore in the chamber):
Date
[yyyy/mm/dd]
First
time Sun in chamber
[hh:mm:ss]
using local time
Clouds
before?
[yes/no]
Last
time Sun in chamber
[hh:mm:ss]
using local time
Clouds
after?
[yes/no]
Picture
number+ time [hh:mm:ss]
2007/08/30
2007/08/31
2007/09/01
2007/09/02
2007/09/03
2007/09/04
2007/09/05
2007/09/06
2007/09/07
2007/09/08
2007/09/09
2007/09/10
2007/09/11
2007/09/12
2007/09/13
2007/09/14
2007/09/15
2007/09/16
2007/09/17
2007/09/18
2007/09/19
2007/09/20
2007/09/21
2007/09/22
2007/09/23
2007/09/24
2007/09/25
2007/09/26
2007/09/27
2007/09/28
2007/09/29
2007/09/30
2007/10/01
2007/10/02
version
0.1
Making pictures
If you make pictures, please note also the time (as shown by the same
clock you used for the observations). Put this information also in the
above table (last column).