Home |
Search |
Today's Posts |
![]() |
|
uk.sci.weather (UK Weather) (uk.sci.weather) For the discussion of daily weather events, chiefly affecting the UK and adjacent parts of Europe, both past and predicted. The discussion is open to all, but contributions on a practical scientific level are encouraged. |
Reply |
|
|
LinkBack | Thread Tools | Display Modes |
|
#1
![]() |
|||
|
|||
![]()
Hi All
I have a question regarding solar radiation measurements, I am building a DIY weather station, and one of the things i wish to record is Solar radiation and Sunshine Hours. I am useing a photodiode to measure Global (Total) radiation and have done some initial calibration against a photographic light meter,and i am curently measuring daily maximum levels of around 500w/m2 (in NE england) which agrees with my light meter (EV 13.5) however, i have a local weather station with a web site, and this suggests the the maximum levels are arround the 900w/m2 level. I have looked into calculating the 'clear sky radiation' and have writen a program to calculate this. These calculations sugest a maximum for this location for noon today of 830w/m2, i have seen some web sites quoting almost 1280w/m2? Considering i am useing a solar constant of 1353w/m2 how can these figures be correct? or is it me , not understanding the figures corectly? Any help would be appreciated Graham |
#2
![]() |
|||
|
|||
![]()
On 08/05/2012 21:50, Graham wrote:
Hi All I have a question regarding solar radiation measurements, I am building a DIY weather station, and one of the things i wish to record is Solar radiation and Sunshine Hours. I am useing a photodiode to measure Global (Total) radiation and have done some initial calibration against a photographic light meter,and i am curently measuring daily maximum levels of around 500w/m2 (in NE england) which agrees with my light meter (EV 13.5) however, i have a local weather station with a web site, and this suggests the the maximum levels are arround the 900w/m2 level. I have looked into That sounds about right to me if the detector is always facing the sun square on and remains perpendicular to the incident light. Pointing vertically upwards or using a diffuser you have to compensate for the cos of the angle between the detector and the sun. calculating the 'clear sky radiation' and have writen a program to calculate this. These calculations sugest a maximum for this location for noon today of 830w/m2, i have seen some web sites quoting almost 1280w/m2? Considering i am useing a solar constant of 1353w/m2 how can these figures be correct? or is it me , not understanding the figures corectly? I'd be surprised if we ever got above 1000W/m^2 peak insolation in the UK at ground level. It probably can happen with the right combination of an unobscured sun and the right sorts of clouds elsewhere. Back of the envelope numbers for the UK are 800W/m^2 direct solar flux at normal incidence and upto 200W/m^2 diffuse radiation. So 1kW/m^2 is a good engineering approximation to peak flux if you are tracking the sun at normal incidence. -- Regards, Martin Brown |
#3
![]() |
|||
|
|||
![]()
Martin Brown wrote:
I'd be surprised if we ever got above 1000W/m^2 peak insolation in the UK at ground level. It probably can happen with the right combination of an unobscured sun and the right sorts of clouds elsewhere. Back of the envelope numbers for the UK are 800W/m^2 direct solar flux at normal incidence and upto 200W/m^2 diffuse radiation. So 1kW/m^2 is a good engineering approximation to peak flux if you are tracking the sun at normal incidence. Hi Martin I am measuring the Global radiation in the horizontal plane with a diffuser, The reason i was querieing the figures of 1280W/m2 is that they seem to be very high considering that the station is a Vantage Pro2 which also measures global radiation in the horizontal plane. Is it possible that the vantage weather stations apply a 'cosine correction' to its global figures? Even my two local weather stations (both vantage) give reading close to my calculated clear sky values My calculations are as follows 54.68N 1.17W 9/5/2012 10:21 Zenith = 48.13 Altitude = 41.87 Air mass 1.4578070793017819 Rayleigh 0.8840397820849082 Ozone 0.9783478706011384 mixed gasses 0.9860899862234945 water vapour 0.8872604163686801 tubidity 0.08813662821376192 Direct Normal 855.6833892378154 Direct Horizontal 572.5643950674784 Direct 573 Diff 108 Total 681 Local stations 746 & 766 W/m2 My readings 390W/m2 weather - Sunny intervals 6/8 cloud I just want to confirm that my figures are approximatly correct or do i need a re-think? Graham |
#4
![]() |
|||
|
|||
![]()
On 09/05/2012 10:35, Graham wrote:
Martin Brown wrote: I'd be surprised if we ever got above 1000W/m^2 peak insolation in the UK at ground level. It probably can happen with the right combination of an unobscured sun and the right sorts of clouds elsewhere. Back of the envelope numbers for the UK are 800W/m^2 direct solar flux at normal incidence and upto 200W/m^2 diffuse radiation. So 1kW/m^2 is a good engineering approximation to peak flux if you are tracking the sun at normal incidence. Hi Martin I am measuring the Global radiation in the horizontal plane with a diffuser, The reason i was querieing the figures of 1280W/m2 is that they seem to be very high considering that the station is a Vantage Pro2 which also measures global radiation in the horizontal plane. Yes. That sounds more like an estimate of the solar flux *above* the atmosphere. Is it possible that the vantage weather stations apply a 'cosine correction' to its global figures? If it knows the time of day and station latitude then I would expect it to use that info to compute effective solar flux at normal incidence. Even my two local weather stations (both vantage) give reading close to my calculated clear sky values My calculations are as follows 54.68N 1.17W 9/5/2012 10:21 Zenith = 48.13 Altitude = 41.87 Air mass 1.4578070793017819 Rayleigh 0.8840397820849082 Ozone 0.9783478706011384 mixed gasses 0.9860899862234945 water vapour 0.8872604163686801 tubidity 0.08813662821376192 Direct Normal 855.6833892378154 Direct Horizontal 572.5643950674784 Direct 573 Diff 108 Total 681 Local stations 746& 766 W/m2 My readings 390W/m2 weather - Sunny intervals 6/8 cloud I just want to confirm that my figures are approximatly correct or do i need a re-think? I think your measured figures at a shade under 800W/m^2 are in the right ball park. I'd be suspicious of anything above 1kW/m^2. If you can tweak your detector so it also measures the normal incidence component near to noon on a nice sunny blue sky day. If you get something like 950 measured then you are quids in. Some charlatans selling solar panels claim 1kW/m^2 solar flux... -- Regards, Martin Brown |
#5
![]() |
|||
|
|||
![]()
Martin Brown wrote:
If you can tweak your detector so it also measures the normal incidence component near to noon on a nice sunny blue sky day. If you get something like 950 measured then you are quids in. I have been looking on the net this afternoon, and found a document on 'Derived Variables used in Davis weather instruments' This calls the Solar radiation figure, 'Net Radiation', that is the measured visible spectrum from the sensor PLUS a calculated amount for the Thermal part of the spectrum. Not shure if this would account for all of the aditional w/m2 but it makes more sense now, and you guys have restored my faith in my calculations, just need a nice clear day to test out the theory.... Might even try the thermometer idea... Thanks Graham |
#6
![]() |
|||
|
|||
![]()
"Martin Brown" wrote in message
... That sounds about right to me if the detector is always facing the sun square on and remains perpendicular to the incident light. Pointing vertically upwards or using a diffuser you have to compensate for the cos of the angle between the detector and the sun. Incidentally, how does one allow for the increased absorption when the sun is lower in the sky and the radiation path through the atmosphere is longer? I am specifically interested in knowing how the radiation on a vertical surface (eg a window) varies with solar altitude. Is there a (perhaps empirical) formula for this? |
#7
![]() |
|||
|
|||
![]()
"Gavino" wrote:
"Martin Brown" wrote in message ... That sounds about right to me if the detector is always facing the sun square on and remains perpendicular to the incident light. Pointing vertically upwards or using a diffuser you have to compensate for the cos of the angle between the detector and the sun. Incidentally, how does one allow for the increased absorption when the sun is lower in the sky and the radiation path through the atmosphere is longer? I am specifically interested in knowing how the radiation on a vertical surface (eg a window) varies with solar altitude. Is there a (perhaps empirical) formula for this? i = I cos (Altitude) where i = incident intensity on the window I = intesity of radiation square to the Sun |
#8
![]() |
|||
|
|||
![]()
On 10/05/2012 01:58, Sleepalot wrote:
wrote: "Martin wrote in message ... That sounds about right to me if the detector is always facing the sun square on and remains perpendicular to the incident light. Pointing vertically upwards or using a diffuser you have to compensate for the cos of the angle between the detector and the sun. Incidentally, how does one allow for the increased absorption when the sun is lower in the sky and the radiation path through the atmosphere is longer? I am specifically interested in knowing how the radiation on a vertical surface (eg a window) varies with solar altitude. Is there a (perhaps empirical) formula for this? i = I cos (Altitude) where i = incident intensity on the window I = intesity of radiation square to the Sun And what you have called "Altitude" is the angle between the normal to the window surface and the direction of the sun. -- Regards, Martin Brown |
#9
![]() |
|||
|
|||
![]()
"Martin Brown" wrote in message
... On 10/05/2012 01:58, Sleepalot wrote: wrote: Incidentally, how does one allow for the increased absorption when the sun is lower in the sky and the radiation path through the atmosphere is longer? I am specifically interested in knowing how the radiation on a vertical surface (eg a window) varies with solar altitude. Is there a (perhaps empirical) formula for this? i = I cos (Altitude) where i = incident intensity on the window I = intesity of radiation square to the Sun And what you have called "Altitude" is the angle between the normal to the window surface and the direction of the sun. Yes, that's right, I'd already worked all that out for myself. But what I am asking for is the correction to 'I' for atmospheric absorption. The lower the solar altitude, the further the rays have to travel through the atmosphere to reach the surface, hence intensity there is reduced. A naive analysis using only cos(altitude) would give maximum intensity (for a vertical surface facing the sun) when the sun is on the horizon. Everyday experience shows this is false. |
#10
![]() |
|||
|
|||
![]()
Martin Brown wrote:
I'd be surprised if we ever got above 1000W/m^2 peak insolation in the UK at ground level. It probably can happen with the right combination of an unobscured sun and the right sorts of clouds elsewhere. 1000W/m^2 equates to a blackbody temp of about 92C A record ground temperature of 70C was recorded in Death Valley (which isn't black). 60C is (too) painful to touch and 70C denatures protein (ie. fries eggs). I wonder what temperature roads start melting at. |
Reply |
|
Thread Tools | Search this Thread |
Display Modes | |
|
|
![]() |
||||
Thread | Forum | |||
Solar Radiation Measurements | uk.sci.weather (UK Weather) | |||
GW is not sunspots, solar cycle length, solar magnetic field, cosmic rays, or solar irradiance. | sci.geo.meteorology (Meteorology) | |||
Wanted - Solar radiation information for Leicester | uk.sci.weather (UK Weather) | |||
Incident Solar Radiation levels | uk.sci.weather (UK Weather) | |||
Hurricanes and solar radiation | uk.sci.weather (UK Weather) |