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East Asia and Western Pacific METEOROLOGY AND CLIMATE

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258<br />

start from October 1990 <strong>and</strong> end in the same month (October) of 1992.<br />

Intensive Observing Periods CIQP) The formal observing period will<br />

include 4 intensive observing periods, scheduled to take place in four<br />

different seasons in 1991, each lasting 15 days. The scientific<br />

objectives for the four lOPs are as follows:<br />

(1) In winter (December or January), observational study on the<br />

behaviour of the energy exchange between air <strong>and</strong> l<strong>and</strong> surface, i.e.<br />

whether the l<strong>and</strong> surface is a heat sink or a heat source; <strong>and</strong> the<br />

physical mechanisms of the energy exchange between air <strong>and</strong> l<strong>and</strong><br />

surface when ground surface is a heat sink.<br />

(2) In spring (April), two major scientific problems will be<br />

studied: Air-mass transformation Atmospheric dust formation<br />

(3) In summer (July), the main scientific objective is to observe<br />

<strong>and</strong> study the structure of the PEL <strong>and</strong> the advection effect in the<br />

PEL.<br />

(4) In autumn (October), the seasonal transition of surface energy<br />

budget*<br />

Pilot Observing Period (]pOP) One pilot field observation was<br />

conducted in August <strong>and</strong> September 1988 before the FOP. The aims of<br />

the POP are to test the automatic data collecting <strong>and</strong> transmitting<br />

system, <strong>and</strong> to carry out the field observational plan in order to<br />

explore the scientific results <strong>and</strong> learn the logistical lessons.<br />

VI* Measurements<br />

(1) Measurements during JFOp Radiation — The radiation<br />

measurements can be divided into two parts. Some are long term<br />

measurements (lasting for two years) concerned with estimating the<br />

radiative energy budget of the ground surface. Additional special<br />

measurements of atmospheric <strong>and</strong> surface radiation properties are<br />

directed towards providing corrections for satellite data. For this<br />

reason, the measurements of the spectral solar <strong>and</strong> infrared radiations<br />

at a well-chosen set of discrete wavelength b<strong>and</strong>s should be made

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