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Green Building Bible, Fourth Edition
Green Building Bible, fourth edition (both books)
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    • CommentAuthortony
    • CommentTimeJan 1st 2010 edited
     
    Are these taken into account in U value calculations?

    Hot box tests when applied to glazing do not take these into account as far as I can see.

    Theses can be huge losses as radiation losses are proportional to the difference between the fourth powers of the two absolute temperatures and space is essentially at absolute zero the upper atmosphere to which some heat is radiated is very cold too over a hundred degrees below freezing!

    Even the surface temperatures of flat roofs can fall way below zero indeed -30 C is common in the night during summer where air temperatures are much warmer, in winter this will be true but less noticeable.

    Are radiation losses only something that we have to contend with in the real world but not in models?
  1.  
    U-value calcs do not. Dynamic simulation does. Though there is no requiremnt to consider this for Bregs.

    I feel the M-word may soon be mentioned:neutral:
    •  
      CommentAuthorSteamyTea
    • CommentTimeJan 1st 2010
     
    M-word ?
  2.  
    multif.....
  3.  
    told you so:fierce:
    • CommentAuthortony
    • CommentTimeJan 2nd 2010
     
    thought you meant mad as in building regs not taking them into account
  4.  
    Ah, that too.
    •  
      CommentAuthorfostertom
    • CommentTimeJan 2nd 2010 edited
     
    Edit - Ignore the following - tony's accordingly modified his opening statements, above

    Posted By: tonyradiation losses are proportional to the fourth power of the temperature difference
    A commonly quoted misconception - radiation losses are proportional to
    the difference between the fourth powers of the two absolute temperatures
    not the fourth power of the difference.
    That makes a huge difference.

    Posted By: tonyspace is essentially at absolute zero
    Yes but we on the surface don't 'see' much of the temp of deep space - otherwise we'd be in deep trouble! We mainly 'see' the radiant temp of the lower layers of the atmosphere, and only a little of our surface radiation passes unblocked thro the atmosphere to deep space.
    • CommentAuthortony
    • CommentTimeJan 2nd 2010
     
    But radiation heat losses are none the less huge in comparison to other heat losses especially through glazing.
    •  
      CommentAuthorfostertom
    • CommentTimeJan 2nd 2010
     
    Oh yes, I'm not disagreeing, just nitpicking!
  5.  
    Sorry - radiative heat losses are NOT huge compared to other losses. Consider the following
    - blackbody radiant loss from a surface at 20C is around 42W/m2
    0 is around 32W/m2
    (stefan-boltzmann law)
    A window (vertical) is radiating to and receiving radiation from its surroundings - not space - so a pane at 20C on a freezing night would lose around 10W/m2 - compare that with conductive losses for u value around 1.5 = 30W/m2 i.e. 1/3 (significant, which is why low E glass is used, but not enormous).

    a roof WILL radiate significant amounts to space, although as fostertom says, there will be an exchange with the atmosphere, so numbers will be much less than the blackbody numberrs above - additionally, must consider the fac that radiation from an opaque body only affects the surface - losses to the surface are by conduction, so losses from a dwelling depend on the surface temperature of the roof - that will drop, yes, but the cool surface will set up an air circulation across the roof limiting the temperature drop to typically a fw degrees below ambient (you get a grass frost in winter when air temp is below around 5 degrees (summer nights are much shorter). Don't know where Tony gets his -30 number from - possible for the top of a low thermal mass,highly insulated surface set up to minimise air movement, I suppose, but seems unlikely in normal conditions.
    •  
      CommentAuthordjh
    • CommentTimeJan 4th 2010
     
    -30 C is around the number I get when I point an infrared thermometer up into a clear night sky.
  6.  
    metal roof, measuring reflected radiation from above?
    • CommentAuthorRobinB
    • CommentTimeJan 4th 2010
     
    I don't understand this thread at all. I don't feel that cold when I point myself into a clear night sky so does it matter to green-builders? I mean I'm confused - the roof in summer being below zero degrees - it just doesn't feel like that. Should I point my freezer at the night sky?

    I'm kind of wishing I had a different persona for my really thick-person comments, but I am very interested in real-life energy use and measurement, so I'm posting this anyway.
    •  
      CommentAuthorfostertom
    • CommentTimeJan 4th 2010
     
    Posted By: ChrisEnglandso a pane at 20C on a freezing night would lose around 10W/m2 - compare that with conductive losses for u value around 1.5 = 30W/m2 i.e. 1/3 (significant, which is why low E glass is used, but not enormous)
    But with a Passivhaus-spec 3G window of 0.7 Uw, radiant loss rises to two thirds extra on top of conductive loss - often, as Mike says, ignored. When does significant become enormous?!

    Posted By: ChrisEnglandlosses from a dwelling depend on the surface temperature of the roof - that will drop ... to typically a fw degrees below ambient (you get a grass frost in winter when air temp is below around 5 degrees)
    That is v interesting - implies that even for straight conductive calcs (i.e. even if ignoring radiant loss), for roofs an outside temp much lower than ambient air temp should be taken, when the roof has even partial 'sight' of unclouded sky. That means clearish nights, and clearish days for roofs without direct sun (if the roof has direct sun, then the reverse is true - surface temp will then e above ambient air temp).
  7.  
    RobinB - we're looking into the numbers to determine the significance - and in many ways the radiation losses are only a small component, but may be important at times in planing eg insulation etc. Freezing in summer isn't really very likely...

    Consider a 'thin' roof, no thermal mass, with an approximate balance between radiation loss and heat conducted in from the outside air - using djh's -30 for sky temperature gives a heat input of roughly 20W/m2, whereas a roof at 10C would be emitting 37ish, giving a net loss of 17 W/m2. Assuming a surface resistance of around .1 (seems reasonable for a still night, with only downwelling drifting air across the roof). then balancing the heat input from the air suggests a temperature difference of around 2 degrees (surface u value =10). Obviously some assumptions here, but should be the right area and agrees roughly the the points about frost. Conclusion is that the radiative heat losses primarily cool the air and hence are taken into account in normal heat loss calcs, with the exception of a few 'stray' degrees.
    Fostertom - surely Passivhaus spec 3G glass is low E - hence low radiative loss?
    and yes it does suggest a lower value should be taken into account - but if you have 'reasonable' (whatever reasonable is' ) thermal mass then I would imagine the (also not included) solar gain would cancel out the differences.
    • CommentAuthortony
    • CommentTimeJan 17th 2010
     
    If the sky is sometimes at -30C shouldn't a proportion of the background in the hot box be at this temperature too -- or a proportion of a U value heat loss calculation done with outside at -30?

    Something in the theory is not getting done right

    Even thermal models dont quite get this point as i ass it.
  8.  
    cite>Posted By: tonyIf the sky is sometimes at -30C shouldn't a proportion of the background in the hot box be at this temperature too -- or a proportion of a U value heat loss calculation done with outside at -30?

    Tony,
    Short answer is no - u-values (or perhaps more correctly k-values) are intrinsic properties of the materials in question and are independent of the surroundings - should be measured in the best way possible. Radiation or other losses should be incorporated in heat loss calculations separately from conduction losses, where it is appropriate to do so - although the examples above suggest they are limited vs conduction losses, although worth some consideration for roofs.
    • CommentAuthortony
    • CommentTimeJan 18th 2010
     
    I would say and for windows and more especially glass roofs?

    I was suggesting a way to try get (quote) "Radiation or other losses should be incorporated in heat loss calculations separately from conduction losses" as these are completely ignored at present as far as I can see.

    Like by everyone, SAP, TAS, Building Regs, all heat loss calculations, Hot 3000, PHPP, AECB etc....
  9.  
    Posted By: tonyas these are completely ignored at present as far as I can see. [ ... ] Like by everyone ... Hot 3000


    Tony,

    why don't you download the code for ESP-r and see what models are in there? I know that hot2000/3000 have been verified against real buildings so I suspect that either the radiation losses are modeled or, if not, they are not significant. Certainly windows are modeled correctly as the type of coating is used, together with the SGHC, to account for incidental solar gains etc. It's thing for you to opine that these radiation losses are "huge" and that they're not modeled so it would be interesting if you would report back for us as the ESP-r engine is open source. Indeed, the emails of the developers are there so perhaps you could engage in a dialog with them?

    Paul in Montreal.
    • CommentAuthorMike George
    • CommentTimeJan 18th 2010 edited
     
    Tony, It is possible to output radiation gains and losses from any surface drawn in the geometry file in TAS - walls, windows -anything, though longwinded and time-consuming
    • CommentAuthorfuncrusher
    • CommentTimeJan 18th 2010
     
    Your car gets quickly frosted overnight and an uninsulated roof (esp metal roof) on an unheated shed frosts inside and out easily. Anyone who doubts the importance of radiation should consider three anecdotes. (1) walk across your bedroom in the nude on a cold night, passing in front of the window with curtains open. As well as getting attention from the neighbours, you will instantly notice your net radiation loss as you pass the cold window (2) offer a dog the choice of a very cold room with a blazing fire and a warm room with no fire, and he'll promptly lie down in front the fire. (3) Think how pleasant the radiation from the sun was during the recent very cold snap.

    Obsession with increased insulation ignores not only diminishing returns but also the fact that other matter which are ignored become the dominant cause of energy loss. Radiation is one. The stupid behaviour of humans is another eg failing to close doors and windows.
    • CommentAuthorBrendan
    • CommentTimeJan 26th 2010
     
    Below is how i have calculated radiant heat transfer across a single foil with nice round numbers. I have been racking my brain to do the same calculation but with insulation rather than a perfect conductor so that the heat loss from the radiant component can be applied to a normal roof in a cloudless sky. If i have any success i will return.
    So here are my calcs. Someone please stop me if i am talking rubbish.

    Radiant heat flow from room to outside:
    Room background radiation at 300K assuming air temp = radiant temp (pretty warm, imagine an old folks home!) assuming 0.9 emissivity = 413w per sqm
    This is worked out from:
    emissivity x s-b constant x absolute temp^4
    In this case:
    0.9 x 5.67x10-8 x 8100,000,000 = 413watts incident on 1sqm of foil assuming direct radiant transfer from room

    Assuming foil has an emissivity of 0.1:
    10% absorbed = 41.3w
    Assuming foil a perfect conductor, the 41 watts will be re-emitted on each side in proportion to the ratio of the emissivities of each side. Thus if the cold side has emissivity of 0.1 then it will emit equally each side, ie approx 20.7 watts. Therefore 20.7 watts would be lost to the outside.

    Radiant heat 'Flow' from outside into building (obviously it doesnt flow from cold to hot but energy of the cold side needs to be subtracted from the flow from the warm side):
    External radiation at 280K assuming 0.9 emissivity = 314w incident on 1sqm of foil
    10% absorbed (90% reflected) = 31.4w / 2 = 15.7w per face.

    Average flow out of building = 20.7 - 15.7 = 5w per sqm.
    U value equivalent = 5w/20K = 0.25 w/m2K for the radiant component
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