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Vergara - 1976 - Physiological and morphological adaptability of ri

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146 CLlxL-Yfl-L AND RILTE<br />

DUPLICATION OF NATURAL CONDITIONS<br />

Lighting<br />

The relevance <strong>of</strong> these heat-exchange physics to the two types <strong>of</strong> lighting <strong>and</strong><br />

their cost implications depends completely on whether the light from the artificial<br />

sources can essentially simulate that received nattirally<br />

From the physical st<strong>and</strong>point the artificial source must provide: (l) a spcetium<br />

equivalent to daylight. (Z) an intensity" range equivalent to daylight. (3) an<br />

even. diffuse light over the plant-growing area.<br />

Providing these requirements introduces a very complex subject. First, no one<br />

artificial light source, or any presently known combination <strong>of</strong> sources at reasonable<br />

cost, can completely simulate a st<strong>and</strong>ard daylight spectrum within the<br />

physiologically’ active range <strong>of</strong> radiation. Second. the important physiological<br />

characte<strong>ri</strong>stics <strong>of</strong> natural radiation conditions <strong>and</strong> <strong>of</strong> “normal" plant growth<br />

under external conditions are difficult to define with certainty The more this<br />

is examined in detail, to set operating st<strong>and</strong>ards, the more elusive absolute<br />

definitions become<br />

As to radiation. there are va<strong>ri</strong>ations in the spectral balance according to solar<br />

angle <strong>and</strong> hence by season. latitude <strong>and</strong> time <strong>of</strong> day’ (Fig. l). Some <strong>of</strong> these<br />

va<strong>ri</strong>ations become quite substantial, <strong>and</strong> they fluctuate because <strong>of</strong> presence or<br />

Spectral imam-ea (w-nrznmh<br />

4.0<br />

20<br />

O6<br />

O4<br />

O2<br />

O I .<br />

300 500 700 900 tl0O<br />

Wavelength l nrn}<br />

l. Spectral lITEldiZlHCB dist<strong>ri</strong>bution curves for sunlight<br />

xvitlt m » 0. l. 2. 3. 4. S (adapted from Fig. l0. Niloon.<br />

1940)‘

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