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<DIV><FONT face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007>Gulsu,</SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007></SPAN></FONT> </DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>the
problem in ESP-r is that the g-value is not calculated (and used)
explecitly.</SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>A more
sophisticated model is used: 1-D-finite differences together with heat
sources</SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>in the
glaz panes; the heat source is the absorption of solar radiation within
the</SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>glaz
panes. But nevertheless you could get a g-value from the results
library</SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007>(varying with time) in the </SPAN></FONT><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>following
way:</SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007></SPAN></FONT> </DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>In
common the g-value shows two parts: The transmission of solar radiation
and</SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>the so
called secondary heat gain, which represents the heatflux from the
inner</SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007>surface of the glazing into the room. The sum of solar
radiation transmission and</SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007>secondary heat flux is the g-value.</SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007></SPAN></FONT> </DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>In
ESP-r the solar radiation transmission is calculated </SPAN></FONT><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>depending on the
angle of </SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007>incidence of the sun (based on the </SPAN></FONT><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>values given in
the optics-lib). The problem is </SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>that
ESP only calculates the entering </SPAN></FONT><FONT face=Arial color=#0000ff
size=2><SPAN class=984255106-01022007>solar radiation as the sum over all
glazing </SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>(see
toggle solar process in <FONT face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007>the res-modul). So you can use this value for
</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>solar radiation
transmission for the first part of the g-value only if you have
one</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>single window -
otherwise you have to splitt this value in several parts and
assign</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>them to the
different glazings. And be aware that this value varies with time -
as</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>the sun is
changing it´s incidence angle during day .....</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007></SPAN></FONT></SPAN></FONT> </DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>The second part
of the g-value - the secondary heat gain - must also be
extracted</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>a little bit
elaborately: You have to look at the surface balance of the
glazing</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>(inner surface
towards the room) </SPAN></FONT></SPAN></FONT><FONT face=Arial color=#0000ff
size=2><SPAN class=984255106-01022007><FONT face=Arial color=#0000ff
size=2><SPAN class=984255106-01022007>and the sum of convective and longwave
radiative </SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>heatflux is the
secondary heat </SPAN></FONT></SPAN></FONT><FONT face=Arial color=#0000ff
size=2><SPAN class=984255106-01022007><FONT face=Arial color=#0000ff
size=2><SPAN class=984255106-01022007>flux of the g-value.
</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>But be aware that
this heat fluxes also vary with time, as the</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>absorption of
solar radiation within the glaz panes varies with time
(again </SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007>corresponding to the incident angle of the sun)
and also the convective and</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>radiative heat
fluxes into the </SPAN></FONT></SPAN></FONT><FONT face=Arial color=#0000ff
size=2><SPAN class=984255106-01022007><FONT face=Arial color=#0000ff
size=2><SPAN class=984255106-01022007>room vary with time, corresponding to
cooling,</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>internal heat
gains, etc.</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007></SPAN></FONT></SPAN></FONT> </DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>Overall you can
get a variable g-value for your glazing, which is a little bit
elaborately</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>to calculate.
Thus you might ask the ESP development team to include an
additional</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>output - the
g-value - for each glazing in future versions of
ESP-r.</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007></SPAN></FONT></SPAN></FONT> </DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007>-Gunter</SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007></SPAN></FONT></SPAN></FONT> </DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN class=984255106-01022007>
<P><FONT size=2>--------------------------------------------<BR>Dr.-Ing. Gunter
Pültz<BR>Müller-BBM GmbH<BR>Robert-Koch-Str. 11<BR>82152 Planegg bei
München<BR>Telefon +49 (89) 85602-336<BR>Telefax +49 (89) 85602-111<BR><A
href="http://www.mbbm.de/"
target=_blank>http://www.mbbm.de</A><BR>email:plz@mbbm.de</FONT>
</P> </SPAN></FONT></SPAN></FONT></DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007></SPAN></FONT></SPAN></FONT> </DIV>
<DIV><FONT face=Arial color=#0000ff size=2><SPAN class=984255106-01022007><FONT
face=Arial color=#0000ff size=2><SPAN
class=984255106-01022007> </SPAN></FONT></SPAN></FONT></DIV>
<BLOCKQUOTE dir=ltr
style="PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #0000ff 2px solid; MARGIN-RIGHT: 0px">
<DIV class=OutlookMessageHeader dir=ltr align=left><FONT face=Tahoma
size=2>-----Original Message-----<BR><B>From:</B>
esp-r-bounces@lists.strath.ac.uk
[mailto:esp-r-bounces@lists.strath.ac.uk]<B>On Behalf Of </B>Gulsu Ulukavak
Harputlugil<BR><B>Sent:</B> Wednesday, January 31, 2007 8:52 PM<BR><B>To:</B>
esp-r@lists.strath.ac.uk<BR><B>Subject:</B> [esp-r] g-value
analysis<BR><BR></FONT></DIV>
<DIV>hi,</DIV>
<DIV>for a sensitivity analysis, one of my parameter is g-value of glazing.
But I could not modify "only" g-value to check its effect on energy
consumption in Esp-r v.11.2.I could be able to make visible
transmittance modification and u-value modification of glazing
separately. If I am not wrong there was a discussion held about
g-value before here in this list. Will you remind me if this subject is
explained before? </DIV>
<DIV>Moreover will someone explain me calculation procedure of heat gain from
glazings in Esp-r? (specific question is: how is g-value calculated for
a particular glazing in Esp-r and when/where is g-value used in calculations?)
</DIV>
<DIV> </DIV>
<DIV>Thanks in advance.</DIV>
<DIV> </DIV>
<DIV>Gulsu</DIV></BLOCKQUOTE></BODY></HTML>