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Yoshida - 1981 - Fundamentals of Rice Crop Science

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84 FUNDAMENTALS OF RICE CROP SCIENCE<br />

2.11. Relationship between grain number<br />

and amount <strong>of</strong> nitrogen absorbed by heading<br />

(<strong>Yoshida</strong> et al 1972. Data for Japan are<br />

adapted from Murayama 1967).<br />

Table 2.10. Effects <strong>of</strong> temperature on spikelet number and efficiency<br />

<strong>of</strong> nitrogen to produce spikelets (minicrop experiment in<br />

the phytotron). a<br />

Day/night<br />

Spikelets<br />

temperature Spikelets (10 2 /m 2 ) (no./mg N absorbed)<br />

(ºC)<br />

150 N b 100 N 50 N 150 N 100N 50 N<br />

35/27 278 280 244 1.4 2.0 2.9<br />

32/24 299 308 275 1.6 2.2 3.0<br />

29/21 376 313 288 2.1 2.3 3.3<br />

26/18 482 409 326 2.2 2.5 3.2<br />

a lRRl (1978). b Kg N/ha.<br />

c. Low temperature-induced sterility and phosphorus. The adverse effects <strong>of</strong><br />

high nitrogen under low temperatures during the reproductive stage can be<br />

alleviated by increasing the amount <strong>of</strong> phosphate applied (Fig. 2.13). This experiment<br />

confirms a common observation in northern Japan that the effect <strong>of</strong> phosphorus<br />

on rice yield is more significant in cool than in warm years (Ishizuka<br />

1971).<br />

2.4. SOLAR RADIATION<br />

2.4.1. Physical aspects<br />

Most <strong>of</strong> the radiant energy from the sun has a wavelength between 0.3 and 3 µm,<br />

<strong>of</strong>ten referred to as short-wave radiation. The earth emits radiation with<br />

wavelengths ranging from 3 to 50 µm, which is referred to as long-wave radiation.<br />

Solar radiation penetrating the earth’s atmosphere is reflected, absorbed, and<br />

scattered by clouds, gases, and aerosols in the form <strong>of</strong> soil and salt particles,<br />

smoke, insects, and spores. The reflection and scattering occur at all angles, and the<br />

downward component is usually referred to as diffuse sky radiation. Thus, incoming<br />

solar radiation takes the forms <strong>of</strong> direct radiation and diffuse sky radiation. The<br />

sum <strong>of</strong> these two is called global radiation or simply incident solar radiation.

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