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131.
The H2CO production rates measured in Comet C/1995 O1 (Hale-Bopp) from radio wavelength observations [Biver, N., and 22 colleagues, 2002a. Earth Moon Planets 90, 5-14] showed a steep increase with decreasing heliocentric distance. We studied the heliocentric evolution of the degradation of polyoxymethylene (formaldehyde polymers: (CH2O)n, also called POM) into gaseous H2CO. POM decomposition can indeed explain the H2CO density profile measured in situ by Giotto spacecraft in the coma of Comet 1P/Halley, which is not compatible with direct release from the nucleus [Cottin, H., Bénilan, Y., Gazeau, M.-C., Raulin, F., 2004. Icarus 167, 397-416]. We show that the H2CO production curve measured in Comet C/1995 O1 (Hale-Bopp) can be accurately reproduced by this mechanism with a few percents by mass of solid POM in grains. The steep heliocentric evolution is explained by the thermal degradation of POM at distances less than 3.5 AU. This study demonstrates that refractory organics present in cometary dust can significantly contribute to the composition of the gaseous coma. POM, or POM-like polymers, might be present in cometary grains. Other molecules, like CO and HNC, might also be produced by a similar process. 相似文献
132.
The potential role of tropical Pacific forcing in driving the seasonal variability of the Arctic Oscillation (AO) is explored
using both observational data and a simple general circulation model (SGCM). A lead–lag regression technique is first applied
to the monthly averaged sea surface temperature (SST) and the AO index. The AO maximum is found to be related to a negative
SST anomaly over the tropical Pacific three months earlier. A singular value decomposition (SVD) analysis is then performed
on the tropical Pacific SST and the sea level pressure (SLP) over the Northern Hemisphere. An AO-like atmospheric pattern
and its associated SST appear as the second pair of SVD modes. Ensemble integrations are carried out with the SGCM to test
the atmospheric response to different tropical Pacific forcings. The atmospheric response to the linear fit of the model’s
empirical forcing associated with the SST variability in the second SVD modes strongly projects onto the AO. Idealized thermal
forcings are then designed based on the regression of the seasonally averaged tropical Pacific precipitation against the AO
index. Results indicate that forcing anomalies over the western tropical Pacific are more effective in generating an AO-like
response while those over the eastern tropical Pacific tend to produce a Pacific-North American (PNA)-like response. The physical
mechanisms responsible for the energy transport from the tropical Pacific to the extratropical North Atlantic are investigated
using wave activity flux and vorticity forcing formalisms. The energy from the western tropical Pacific forcing tends to propagate
zonally to the North Atlantic because of the jet stream waveguide effect while the transport of the energy from the eastern
tropical Pacific forcing mostly concentrates over the PNA area. The linearized SGCM results show that nonlinear processes
are involved in the generation of the forced AO-like pattern. 相似文献
133.
Thomas G. Müller Emmanuel Lellouch Hermann Böhnhardt John Stansberry Antonella Barucci Jacques Crovisier Audrey Delsanti Alain Doressoundiram Elisabetta Dotto René Duffard Sonia Fornasier Olivier Groussin Pedro J. Gutiérrez Olivier Hainaut Alan W. Harris Paul Hartogh Daniel Hestroffer Jonathan Horner Dave Jewitt Mark Kidger Csaba Kiss Pedro Lacerda Luisa Lara Tanya Lim Michael Mueller Raphael Moreno Jose-Luis Ortiz Miriam Rengel Pablo Santos-Sanz Bruce Swinyard Nicolas Thomas Audrey Thirouin David Trilling 《Earth, Moon, and Planets》2009,105(2-4):209-219
Over one thousand objects have so far been discovered orbiting beyond Neptune. These trans-Neptunian objects (TNOs) represent the primitive remnants of the planetesimal disk from which the planets formed and are perhaps analogous to the unseen dust parent-bodies in debris disks observed around other main-sequence stars. The dynamical and physical properties of these bodies provide unique and important constraints on formation and evolution models of the Solar System. While the dynamical architecture in this region (also known as the Kuiper Belt) is becoming relatively clear, the physical properties of the objects are still largely unexplored. In particular, fundamental parameters such as size, albedo, density and thermal properties are difficult to measure. Measurements of thermal emission, which peaks at far-IR wavelengths, offer the best means available to determine the physical properties. While Spitzer has provided some results, notably revealing a large albedo diversity in this population, the increased sensitivity of Herschel and its superior wavelength coverage should permit profound advances in the field. Within our accepted project we propose to perform radiometric measurements of 139 objects, including 25 known multiple systems. When combined with measurements of the dust population beyond Neptune (e.g. from the New Horizons mission to Pluto), our results will provide a benchmark for understanding the Solar debris disk, and extra-solar ones as well. 相似文献
134.
Giuseppe D. Saldi Guntram Jordan Jacques Schott Eric H. Oelkers 《Geochimica et cosmochimica acta》2009,73(19):5646-5657
Magnesite growth rates and step velocities have been measured systematically as a function of temperature from 80 to 105 °C and saturation state in 0.1 M NaCl solutions using hydrothermal atomic force microscopy (HAFM). The observations indicate that at these conditions magnesite precipitation is dominated by the coupling of step generation via spiral growth at screw dislocations and step advancement away from these dislocations. As these two processes occur in series the slowest of these dominates precipitation rates. At 100 °C magnesite growth rates (r) determined by HAFM are consistent with
r=k(Ω-1)2,