Titlebook: Low Frequency Astrophysics from Space; Proceedings of an In Namir E. Kassim,Kurt W. Weiler Conference proceedings 1990 Springer-Verlag Berl

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Roger A. Chevaliered in the previous four chapters. However, the nature of agricultural activities means that there has had to be some response to the particular problems arising from animal husbandry and crop growth. Crops planted by one tenant may not ripen until after he has moved on, but might not ripen at all if

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Low frequency astrophysics with a space array,nge over which the Earth‘s ionosphere transmits poorly or not at all. High resolution, high sensitivity observations would open a new window in the electromagnetic spectrum for astronomical investigations and bring astronomy to the fundamental physical limit below which the Milky Way becomes optical

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The Lunar Observer radio astronomy experiment (LORAE),g the surface at high resolution and gathering new geophysical data. In its modest concept, LORAE will collect crucial data on the radio interference environment while on the near-side (to aid in planning future arrays) and will monitor bursts of emission from the Sun and the Jovian planets. LORAE w

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A very low frequency array for the lunar far-side, a maximum diameter of 1000 km. Phase 1 consists of deploying antennas over a 17 km diameter in the crater Tsiolkovsky on the lunar far-side while the outer antennas are deployed in the second phase. Array operation is over at least four bands from 1 to 30 MHz with variable bandwidths up to 5 MHz an

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