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Get The Cassini-Huygens Mission: Orbiter In Situ Investigations PDF

By D. T. Young, J. J. Berthelier, M. Blanc, J. L. Burch (auth.), Christopher T. Russell (eds.)

ISBN-10: 1402027745

ISBN-13: 9781402027741

ISBN-10: 9401570698

ISBN-13: 9789401570695

The joint NASA-ESA Cassini-Huygens project delivers to come back 4 (and potentially extra) years of exceptional clinical facts from the sun system’s so much unique planet, the ringed, fuel big, Saturn. better than Galileo with a far better conversation bandwidth, Cassini can accomplish in one flyby what Galileo back in a sequence of passes. Cassini explores the Saturn setting in 3 dimensions, utilizing gravity assists to climb out of the equatorial airplane to seem down at the earrings from above, to photograph the aurora and to review polar magnetospheric strategies comparable to field-aligned currents. because the radiation belt particle fluxes are even more benign than these at Jupiter, Cassini can extra adequately discover the internal areas of the magnetosphere. The spacecraft techniques the planet nearer than Galileo may, and explores the interior moons and the earrings even more completely than was once attainable at Jupiter.

This publication is the second one quantity, in a 3 quantity set, that describes the Cassini/Huygens project. This quantity describes the in situ investigations at the Cassini orbiter: plasma spectrometer, ion and impartial mass spectrometer, lively charged and impartial particle spectrometer, magnetometer, radio and plasma wave spectrometer and the cosmic dirt analyzer. This booklet is of curiosity to all strength clients of the Cassini-Huygens info, to people who desire to know about the deliberate medical go back from the Cassini-Huygens venture and people desirous about the methods taking place in this so much attention-grabbing planet. a 3rd quantity describes the distant sensing investigations at the orbiter.

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5 AU. To minimize weight but still provide adequate radiation shielding, the inner ESA hemisphere (made from aluminum) was optimized to a CASSINI PLASMA SPECTROMETER INVESTIGATION 31 TABLE VI IBS key sensor data and dimensions. 8 mm. The tolerances formanufacturing the hemispheres and aligning them relative to one another were quite stringent. Vilppola et al. (1993) have shown through simulations that inaccuracies of '"'-' few tens of j1,m are important. Normally, the interior surfaces of the hemispheres would have been grooved and blackened to suppress UV photons that could scatter into the detectors, but grooving of the large thin plates is impractical.

In the center of the assembly is the LEF Mep. Large openings between the foil assembly and the edge of the ceramic mounting ring provide ample gas conductance CASSINI PLASMA SPECTROMETER INVESTIGATION 53 during launch and afterwards. The IMS cylindrical housing is approximately 22 cm in diameter x 34 cm long. 5. ELECTRICAL DESIGN A number of key science and resource requirements drove the electrical design of IMS. 1. 75 ns over a range set by the fastest ions (H+ at 65 keY internal energy) and the slowest (heavy ions at 15 kV internal energies).

284% spacing. 5 ms). The basic operational mode consists of a 255-step voltage scan (corresponding to an 36 D. T. YOUNG ET AL. ION BEAM SPECTROMETER T - z j ~ ~ ,... g ~ .. J t- 0 !!! L" j ~ o '" 0 :! - - - 11: § :! 0 DPU lI: ~ ::i ~ '"~ .. z i ~ w p z ~ ~ ~ I Figure 16. Schematic IBS electrical block diagram. energy scan) lasting 2 s. In planned operations this may consist of a single, 255-step scan, two 127 -step scans, or half of a 51O-step, interleaved scan. Data values for generating the energy sweep are stored in CPUI memory.

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The Cassini-Huygens Mission: Orbiter In Situ Investigations Volume 2 by D. T. Young, J. J. Berthelier, M. Blanc, J. L. Burch (auth.), Christopher T. Russell (eds.)


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