Sonnenobservatorium Kanzelhöhe
Sonnenobservatorium Kanzelhöhe since 20.8.2009 Web: http://www.kso.ac.at/
The original sensor was the number L19 of the original International Year of Astronomy 2009, prototype series. It recorded from August 2009 to June 2017. The new sensor is a Mark 2.3l, recording since 2019-04-18 12:00 UTC.
at_KSO_4
1.40033 nahe Globalstrahlungs-Instrumentengruppe W-Dach;
Montiert auf Geländer bei der Stiege
Fertig positioniert 11:10h MESZ
kleine Zelle im Süden
--Swenig (talk) 20:31, 31 March 2023 (CEST)
at_KSO_3
LP045 nahe Globalstrahlungs-Instrumentengruppe W-Dach; Achtung als Stationskennung wird derzeit weiter at_KSO_2 übertragen.
Getauscht gegen Mittag auf Kaminstutzen;
To get more distance from the Aeronet and a french experiment, the position was moved about 2m to the SW end of the platform, just south of the total radiation multiple radiometers, and 1,5 m W of the star-pyrrheliometer.
Fertgi positioniert 14h MESZ
--GW (talk) 12:31, 18 April 2019 (CEST)
at_KSO_2
Same Sensor but with PCDuino after Computer Hardware failure in operation until lightning strike
Kennung: AT_KSO_1 / L19
(until Juni 2009 in Davidschlag/Linz-LAG (Hamburger Sternwarte?) destroyed by lightning before 2017-06-22 .
19 TLS 2.7
Destruction image at top: The Lightmeter at_KSO_1 after a Lightning strike near 2017-06-22. Bild (right) Werner Poetzl, KSO, 2017-06-22 08:42:52
Data-set 2009-10-20 to 2017-06-30.
destroyed by lightning 2017-06-30. --GW (talk) 17:20, 30 June 2017 (CEST)
Hier die gesammelten Kalibrationskoeffizienten für AT_KSO_1
X = c ( b (a exp (n(1+dT)/a) - 1) + n )
n ... counts (sensor output)
X ... physical quantity (total radiation in [W/m²]
or horizontal illumination [Lux])
a = 1.1282e+05, b = 1.0924e-03, c = 5.7836e-09, d = 3.9002e-03 [W/m²] a = 1.1282e+05 b = 1.0924e-03 c = 5.1146e-07 d = 3.9002e-03 [Lux] Background X0= 0.444 mlx
Conversion factors determined from total radiation model and independent total radiation measurments.
Log:
Data: 20/21 Okt In [296]: SJD=(X.JD > mx.DateTime.DateTime(2009,10,20,4,10).jdn) & (X.JD < mx.DateTime.DateTime(2009,10,20,17,13).jdn) In [297]: X.fit_em1_to_natLight(Lux_range=[0.0001, 300000], JD_select=SJD, type='em1c0T') Out[297]: (array([ 1.12824157e+05, 1.09241434e-03, 5.11458483e-07, -4.44001757e-04, 3.90019899e-03]), 1) In [308]: plot_date(X.JD-X.pylab_JD0,X.Sunlight_Watt_per_square_meter_from_JD_DM(X.JD,surface_pressure=840.0, T_dew_C=2.0)*0.85/X.Watt_per_square_meter_per_Lux ,'c,', label='DM model,84.0/T_d=2.0/k=2.78')
In [309]: 5.11458483e-07/(0.85/X.Watt_per_square_meter_per_Lux Out[309]: 5.174756416235294e-09 ~ 5.18E-9
--GuentherWuchterl 20:25, 2. Mai 2010 (UTC)
20:28, 2. Mai 2010 GuentherWuchterl
WH --GW (talk) 22:22, 28 April 2016 (CEST)
Kontrollbesuch SW 26.Oktober 2020
