Kippzonen BSRN Scientific Solar Monitoring System Manual do Utilizador Página 131

  • Descarregar
  • Adicionar aos meus manuais
  • Imprimir
  • Página
    / 188
  • Índice
  • MARCADORES
  • Avaliado. / 5. Com base em avaliações de clientes
Vista de página 130
119
Figure C 2.2. Compared log measured and calculated circumsolar functions.
Letters A, B, C, D, E, F symbolizes different aerosol models.
Summarizing the above mentioned results it should be stated, that the circumsolar radiation is a very
variable parameter and it is almost independent of other characteristics (direct or diffuse radiation,
optical depth) of the solar radiation field.
C 2.2.3 Circumsolar diffuse irradiances
Let us suppose that the diffusometers listed in Table C 2.1 are at the same place and measure the
diffuse radiation. Let us select a situation when the
- solar elevation is 45 degrees
- the direct radiation is 700 W m
-2
- the diffuse radiation is 160 W m
-2
- the circumsolar sky function is the mean of measurements (seen in Figs.C 2.2 or C 2.3).
Using the penumbra functions (Fig. C 2.1) of diffusometers, the calculated irradiance of their sensors
seen in Table C 2.2a. For a more complete picture, in Table C 2.2b irradiances calculated for some
pyrheliometers are shown. Since their slope angles are less than that of diffusometers, therefore the
effect of circumsolar radiation on their output is less. More details regarding the pyrheliometers can
be found in Major (1995).
Four diffusometers from the ten “measure” identical value. It seems practical to declare these four
instruments as “standard group” and to relate the output of the others to that of the standard group.
Moreover, the standard group measures the highest value, so all the others have deficit compared
to the standard. In Table C 2.3 the values of deficit are shown for the diffusometers that are not in the
standard group. Since the really measured deficit of Hungary III to Hungary I is collected for a long
time and this way its variability with the conditions could be looked for, the deficits are normalized to
that of HunIII. It is expected that the normalized deficit would not change with changing solar elevation
and atmospheric conditions.
Vista de página 130
1 2 ... 126 127 128 129 130 131 132 133 134 135 136 ... 187 188

Comentários a estes Manuais

Sem comentários