Global mapping comma seasonal variation and search for arcminute structure of zodiacal light comma Section 3A

scientific abstract the purpose of this proposal is twofold. first, to provide a global picture of the zodiacal light as seen by isophot. this skeleton allows us to make consistent use of the large amount of serendipity background measurements to be expected; it allows us to adopt the results obtained with the infrared satellite cobe for use or comparison with iso; it helps to determine reliable backgrounds, which is important in particular for studies of galactic and extragalactic background, but also for the study of faint objects. second, it allows us to study aspects of the spatial distribution of interplanetary dust which have not been treated sufficiently so far: the search for arcminute structure in the zodiacal light, the outofecliptic distribution, the variation of absorption cross section per unit volume with heliocentric distance, and the location of the plane of symmetry as a function of heliocentric distance, where distance is measured by the temperature of the dust. for these measurements the ability of iso to avoid stars and bright infrared cirrus and therefore to measure pure zodiacal light, is an important advantage. this proposal is part of the isophot effort to measure diffuse sky brightness. it is coordinated in some detail with the isophot proposals measurement of the extragalactic background radiation, properties of interplanetary dust and diffuse infrared emission of the galaxy. performance time overview observations priority 1 priority 2 priority 3 sum global mapping 13590 s 9060 s 22650 s (6.3 h) seasonal variation 21066 s 21066 s (5.9 h) arcminute structure 4614 s 4614 s 4614 s 13842 s (3.9 h) tot truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]