Titlebook: Exploration of the Polar Upper Atmosphere; Proceedings of the N Charles S. Deehr,Jan A. Holtet Conference proceedings 1981 D. Reidel Publis

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Middle Atmosphere Dynamics and Compositionstratosphere temperatures are cooler than at middle latitudes and that mesopause temperatures are warmer during the darkness of winter than during the continual sunlight of summer. We will see that the additional physics needed to explain these features involve the dynamics of the middle atmosphere.

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Polar Cap Optical Emissions Observed from the ISIS2 Satelliteet which limit the quantity of useful data. Nevertheless, there have been a sufficient number of satisfactory observations to allow the characteristic features of high latitude emissions to be identified. In the sections that follow, a summary of results of observations of dayside aurora and polar cap arcs is given.

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Plasma Sheet Dynamics: Effects on, and Feedback from, the Polar Ionosphereing the inner magnetosphere from the geomagnetic tail and at the same time separating the two lobes of the magnetotail from each other. Figure 1 schematically illustrates the configuration of the plasma sheet in the noon-midnight meridian plane.

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1389-2185 tudy Institute (ASI) on "The Exploration of the Polar Upper Atmosphere" held at Lillehammer, Norway, May 5-16, 1980. The polar cap is an important part of the high latitude atmosphere not only because of circulation and horizontal trans­ port in the neutral atmosphere and convection in the ionospher

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14–16: Austrians and the Holocaust (2)of in­coherent scatter observations also in the D region is pointed out. Better spatial resolution is obtained with probes carried on rockets. Some probes, which have been used successfully in the E region, are described.

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