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Vergara - 1976 - Physiological and morphological adaptability of ri

Vergara - 1976 - Physiological and morphological adaptability of ri

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5 l2 CLIMATE AND RICE<br />

tently flooded water regime. The maximum yield <strong>of</strong> 11.7 tfha obtained with 1R8<br />

was at 480 kg N/ha. Within a specific plant type. the earlier-matu<strong>ri</strong>ng cultivar<br />

produced a higher response to N than its later-matu<strong>ri</strong>ng counterpart. The data<br />

from Peru suggest a significant interaction between plant type <strong>and</strong> growth duration<br />

as factors affecting N response in a high solar radiation environment.<br />

Sanchez et al. (1973) reported the weather pattern du<strong>ri</strong>ng the cropping season in<br />

relation to growth stages <strong>of</strong> the eultivars tested in the expe<strong>ri</strong>ment conducted in<br />

Peru. temperatures were low at the seedling <strong>and</strong> <strong>ri</strong>pening stages (particularly<br />

the night temperature) but were around 20°C du<strong>ri</strong>ng tille<strong>ri</strong>ng stages. This helped<br />

in obtaining high tiller number in each va<strong>ri</strong>ety The main reason for marked<br />

response to up to 320 kg N/ha was p<strong>ri</strong>ma<strong>ri</strong>ly the high solar radiation du<strong>ri</strong>ng the<br />

entire growing pe<strong>ri</strong>od. The average solar radiation value for the <strong>ri</strong>cegrovviitg<br />

season in Peru was 488 cal - sq curl - day“ which is 19% higher (Sanchez et al..<br />

1973) than we reported as an average value for a dryt-season <strong>ri</strong>ce cropping in<br />

Los Bafios. Philippines (De Datta <strong>and</strong> Zarate. 1970). High solar radiation <strong>and</strong><br />

low night temperature <strong>and</strong> intermittent flooding in Peruvian conditions (Sanchez<br />

et al.. 1973) are in direct contrast to low solar radiation <strong>and</strong> high temperature<br />

in the hot, tropical Asian conditions (De Datta et al.. 1966. 1968', De Datta<br />

<strong>and</strong> Zarate. 1970).<br />

Correlation between nitrogen response <strong>and</strong> solar radiation<br />

Institute expe<strong>ri</strong>ments have revealed strong positive correlations between grain<br />

yield <strong>and</strong> solar radiation values du<strong>ri</strong>ng the last 30 days <strong>of</strong> crop growth. The<br />

planting date should be adjusted so that the crop will receive maximum solar<br />

energy’ du<strong>ri</strong>ng the reproductive stage, particularly du<strong>ri</strong>ng the <strong>ri</strong>pening pe<strong>ri</strong>od<br />

(Moomaw et al.. 1967). This is explained by Tanaka et al. (1966) who found that<br />

the increase in dry matter following flowe<strong>ri</strong>ng <strong>of</strong> <strong>ri</strong>ce is p<strong>ri</strong>ma<strong>ri</strong>ly in the fonn <strong>of</strong><br />

grain. lt is also dependent on the amount <strong>of</strong> solar energy received by the crop<br />

du<strong>ri</strong>ng that pe<strong>ri</strong>od. Later expe<strong>ri</strong>ments at IRRI. though. showed that correlations<br />

were recorded between solar energy total for the last 45 day's before harvest <strong>and</strong><br />

dry-matter production for that pe<strong>ri</strong>od (De Datta et al.. 1968). This pe<strong>ri</strong>od corresponds<br />

to the particle initiation to mani<strong>ri</strong>ty’ stage. Since photosynthesis for<br />

grain production is also important for the pe<strong>ri</strong>od between panicle initiation <strong>and</strong><br />

heading (Murata. 1966). high correlation values for grain yield response to solar"<br />

energy total. which include that pe<strong>ri</strong>od. are underst<strong>and</strong>able.<br />

Expe<strong>ri</strong>ments conducted du<strong>ri</strong>ng 1968 <strong>and</strong> 196‘) showed that in l2 harvests<br />

<strong>of</strong> the four va<strong>ri</strong>eties tested. the highest nitrogen response <strong>and</strong> grain yield o1‘<br />

9.3 t/ha were obtained with 1R8 when harvested in May (Fig. 2). In each <strong>of</strong> 12<br />

harvests, 1R8 produced at least 5 tfha indicating its consistent high yielding<br />

ability’. On the other h<strong>and</strong>. the tall tropical va<strong>ri</strong>ety Il—4 produced its highest<br />

grain yield <strong>of</strong>6.3 tfha in the May harvest. but gave a yield <strong>of</strong> only 2 tfha in the<br />

August harvest. 1n the dry season. as the solar radiation received du<strong>ri</strong>ng the<br />

45-day pe<strong>ri</strong>od before harvest increased from ll kcal/sq cm for the January<br />

harvest to about 20 kcal/sq em for the May harvest, the ititrogcn response <strong>of</strong> 1R8

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