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71.
72.
Biver Nicolas Bockelée-Morvan Dominique Colom Pierre Crovisier Jacques Henry Florence Lellouch Emmanuel Winnberg Anders Johansson Lars E.B. Gunnarsson Marcus Rickman Hans Rantakyrö Fredrik Davies John K. Dent William R.F. Paubert Gabriel Moreno Raphaël Wink Jörn Despois Didier Benford Dominic J. Gardner Matt Lis Dariusz C. Mehringer David Phillips Thomas G. Rauer Heike 《Earth, Moon, and Planets》2002,90(1-4):5-14
The bright comet Hale–Bopp provided the first opportunity to follow the outgassing rates of a number of molecular species over a large range of heliocentric distances. We present the results of our observing campaign at radio wavelengths which began in August 1995 and ended in January 2002. The observations were carried out with the telescopes of Nançay, IRAM, JCMT, CSO and, since September 1997, SEST. The lines of nine molecules (OH, CO, HCN, CH3OH, H2CO, H2S, CS, CH3CN and HNC) were monitored. CS, H2S, H2CO, CH3CN were detected up to rh= 3–4 AU from the Sun, while HCN and CH3OH were detected up to 6 AU. CO, which is the main driver of cometary activity at heliocentric distances larger than 3–4 AU, was last detected in August 2001, at rh= 14 AU. The gas production rates obtained from this programme contain important information on the nature of cometary ices, their thermal properties and sublimation mechanisms.Line shapes allow to measure gas expansion velocities, which, at large heliocentric distances, might be directly connected to the temperature of the nucleus surface. Inferred expansion velocity of the gas varied as rh -0.4 within 7 AU from the Sun, but remained close to 0.4 km s-1 further away. The CO spectra obtained at large rhare strongly blueshifted and indicative of an important day-to-night asymmetry in outgassing and expansion velocity. The kinetic temperature of the coma, estimated from the relative intensities of the CH3OH and CO lines, increased with decreasing rh, from about 10 K at 7 AU to 110 K around perihelion. 相似文献
73.
Oliver Montenbruck Yago Andres Heike Bock Tom van Helleputte Jose van den Ijssel Marc Loiselet Christian Marquardt Pierluigi Silvestrin Pieter Visser Yoke Yoon 《GPS Solutions》2008,12(4):289-299
The global navigation satellite system receiver for atmospheric sounding (GRAS) on MetOp-A is the first European GPS receiver
providing dual-frequency navigation and occultation measurements from a spaceborne platform on a routine basis. The receiver
is based on ESA’s AGGA-2 correlator chip, which implements a high-quality tracking scheme for semi-codeless P(Y) code tracking
on the L1 and L2 frequency. Data collected with the zenith antenna on MetOp-A have been used to perform an in-flight characterization
of the GRAS instrument with focus on the tracking and navigation performance. Besides an assessment of the receiver noise
and systematic measurement errors, the study addresses the precise orbit determination accuracy achievable with the GRAS receiver.
A consistency on the 5 cm level is demonstrated for reduced dynamics orbit solutions computed independently by four different
agencies and software packages. With purely kinematic solutions, 10 cm accuracy is obtained. As a part of the analysis, an
empirical antenna offset correction and preliminary phase center correction map are derived, which notably reduce the carrier
phase residuals and improve the consistency of kinematic orbit determination results.
相似文献
Oliver MontenbruckEmail: |
74.
The determination of the nuclear magnitudes of comets, and with it nuclear size frequency distributions, is strongly complicated by cometary activity. By now, only nuclear size frequency distributions for Jupiter Family comets are available, and they are still subject of uncertainties. For comets of other dynamical classes, nuclear magnitudes are known for only a few comets. The size frequency distributions are thus not well constrained.In this work we study whether nuclear magnitudes of comets can be constrained from sky survey observations as published by the Minor Planet Center. Observations from sky survey programs in which the comet was classified as a point-like source are analyzed in this respect.From the available published observations from 1998 to 2008, we derive nuclear magnitudes, as well as nuclear radii, for 84 comets. Among these are comets of the Jupiter Family, dynamically old and new isotropic comets, Halley-type comets and Centaurs. For Jupiter Family comets and for isotropic comets, the size frequency distributions are presented.Uncertainties of derived nuclear magnitudes arise from photometry and from potentially undetected activity. However, a comparison with objects with well known nuclear parameters shows that, despite substantial observational uncertainties, nuclear magnitudes are constrained to ±0.6 mag, thereby providing first indications for nuclear sizes. This is particularly relevant for isotropic comets with so far ill-constrained size distributions. Exponents of the differential size frequency distributions of for Jupiter Family comets and for isotropic comets are presented. The values derived here form a basis for future, dedicated observational studies which provide higher measurement accuracy. 相似文献
75.
The deviation from stoichiometry, δ, in spinel solid solutions of the type (Ti
x
Fe
1−x
)3−δ O4 with x=0.1, 0.2 and 0.25 was studied thermogravimetrically as a function of oxygen activity, a
O2, at 1100, 1200 and 1300 ∘C. The experimental results, S-shaped curves for δ vs. log aO2, are presented and discussed with regard to the type of point defects prevailing under different conditions in the deviation
from stoichiometry. It is concluded that cation vacancies are the predominant point defects at high oxygen activities, while
cation interstitials prevail at low oxygen activities. The temperature and composition dependencies of point defect concentrations
are also discussed.
Received: 1 October 1996 / Accepted: 15 September 2002
Acknowledgements The authors thank the US Department of Energy for support of this work under Grant no. DE-FGO2–88ER45357. This work made
use of the Cornell Center of Materials Shared Experimental Facilities, supported through the National Science Foundation Materials
Research Science and Engineering Centers program (DMR-0079992). 相似文献
76.
On the phenology of North Sea ichthyoplankton 总被引:2,自引:1,他引:2
Greve Wulf; Prinage Sabine; Zidowitz Heike; Nast Jutta; Reiners Frank 《ICES Journal of Marine Science》2005,62(7):1216-1223
77.
Groundwater risk intensity mapping in semi-arid regions using optical remote sensing data as an additional tool 总被引:2,自引:1,他引:2
Due to semi-arid to arid climatic conditions, Jordan has limited groundwater resources. As a result of agricultural activities
and untreated wastewater, most of the groundwater in the karstic areas is microbiologically contaminated. Groundwater vulnerability,
hazards, and risk intensity were mapped (scale 1:50,000) at a test site near the Jordan Rift Valley. The mapping included
the use of optical remote sensing to complement conventional data in areas with poor data. LANDSAT ETM+ data, and colour and
panchromatic aerial photographs at different scales were incorporated using visual image interpretation and digital image
processing. The applicability of the different remote sensing data sources is discussed and recommendations for their usage
are given. Information derived from digital images offers new opportunities for vulnerability and hazard assessment, particularly
when related to land use, vegetation cover, urbanisation and infrastructure. The resulting maps indicate clearly the vulnerable
areas and the “hot spots” of potential contamination in the test site and form an important basis for integrated groundwater
management studies and the long-term planning of protective measures. The application and transferability of the European
vulnerability approach (COST Action 620) to the test site in Jordan proved to be good, in general, although modifications
were necessary to suit local conditions.
Electronic supplementary material The online version of this article (doi:) contains supplementary material, which is available to authorised users.
Electronic supplementary material The online version of this article (doi:) contains supplementary material, which is available to authorised users.
Résumé La Jordanie ne dispose que de ressources limitées en eaux souterraines, étant donné le climat semi-aride à aride prévalant dans ce pays. La contamination microbiologique de la plupart des eaux souterraines des régions karstiques est due aux activités agricoles et l’absence de traitement des eaux usées. La vulnérabilité des eaux souterraines, et le danger et l’intensité du risque de leur contamination ont été cartographiés (à l’échelle de 1:50 000) pour un site d’étude situé près de la vallée du Rift du Jourdain. La cartographie inclut l’utilisation de données optiques de télédétection pour complémenter les sources de données conventionnelles, dans les zones où la couverture est déficiente. Des données de LANDSAT ETM+ et des photographies aériennes en couleur et panchromatiques à différentes échelles ont été incorporées en utilisant des méthodes d’interprétation visuelle et informatique de l’image. La qualité des différentes sources de données de télédétection est discutée et évaluée, et des recommandations pour leur utilisation sont suggérées. L’informations obtenue des images digitales offre de nouvelles opportunités pour l’évaluation des vulnérabilités et des dangers, surtout reliés à l’usage du sol, la couverture végétale, l’urbanisation et les diverses infrastructures. Les cartes ainsi obtenues indiquent clairement les zones vulnérables et les points critiques potentiels pour la contamination du site d’étude et forment une base importante pour l’étude de la gestion intégrée des eaux souterraines et pour la planification à long terme des mesures de protection. L’applicabilité de l’approche européenne de cartographie de la vulnérabilité et des risques (COST action 620) au site d’étude jordanien est généralement approprié, même si certaines modifications ont été nécessaires pour s’ajuster aux particularités régionales.
Resumen Los recursos hídricos subterráneos en Jordania son limitados debido principalmente a su clima semi árido. En la mayoría de las áreas kársticas, las aguas subterráneas están contaminadas microbiológicamente a consecuencia de la actividad agrícola y de las aguas residuales. Por ello, se han realizado mapas de peligro, vulnerabilidad e intensidad del riesgo (a escala 1/50.000) de un área piloto próxima al Rift en Jordania. Los mapas han sido elaborados con el apoyo de técnicas de teledetección en aquellas zonas donde la información era escasa. Se han utilizado imágenes del LANDSAT ETM+ a y fotografía aérea, de color y pancromática, a diferentes escalas para el procesamiento de las imágenes digitales y la fotointerpretación. En este trabajo se discute y se dan recomendaciones sobre la aplicabilidad de las diferentes imágenes de satélite en los análisis de teledetección. Los datos que se pueden derivar de las imágenes digitales son un avance para la evaluación de la vulnerabilidad y los peligros de contaminación, particularmente aquellos referidos a usos del suelos, cubierta vegetal e infraestructuras urbanas. Los mapas resultantes muestran claramente la vulnerabilidad y los peligros potenciales de contaminación en la zona de estudio, lo que genera una importante base para los estudios de gestión integrada de las aguas subterráneas y de planificación de las medidas protectoras. La aplicabilidad de la aproximación europea a los estudios de vulnerabilidad en karst (COST Action 620) en la zona de estudio (Jordania) es buena, aunque fueron necesarias algunas leves modificaciones de la metodología para ajustarla a las condiciones locales.相似文献
78.
The suspected impact of climate warming on precipitation distribution is examined in the Yangtze River Basin. Daily precipitation data for 147 meteorological stations from 1961–2000 and monthly discharge data for three stations in the basin have been analyzed for temporal and spatial trends. The methods used include the Mann–Kendall test and simple regression analysis. The results show (1) a significant positive trend in summer precipitation at many stations especially for June and July, with the summer precipitation maxima in the middle and lower Yangtze River basin in the 1990s; (2) a positive trend in rainstorm frequency that is the main contributor to increased summer precipitation in the basin; and (3) a significant positive trend in flood discharges in the middle and lower basin related to the spatial patterns and temporal trends of both precipitation and individual rainstorms in the last 40 years. The rainstorms have aggravated floods in the middle and lower Yangtze River Basin in recent decades. The observed trends in precipitation and rainstorms are possibly caused by variations of atmospheric circulation (weakened summer monsoon) under climate warming. 相似文献
79.
80.
Vertical heat fluxes induced by mesoscale thermally driven circulations maycontribute significantly to the subgrid-scale fluxes in large-scale models (e.g.,general circulation models). However, they are not considered in these modelsyet. To gain insight into the importance and possible parameterisation of themesoscale flux associated with slope winds, an analytical (conceptual) modelis developed to describe the relationship between the mesoscale heat flux andatmospheric and land-surface characteristics. The analytical model allows usto evaluate the mesoscale flux induced by slope winds from only a few profilemeasurements within a domain. To validate the analytical model the resultingheat flux profiles are compared to profiles of highly resolved wind and temperaturefields obtained by simulations with a mesoscale numerical model.With no or moderate synoptic wind the mesoscale heat flux generated by the slopewind circulation may be as large as, or even larger than, the turbulent fluxes at thesame height. At altitudes lower than the crest of the hills the mesoscale flux is alwayspositive (upward). Generally it causes cooling within the boundary layer and heatingabove. Despite the simplifications made to derive the analytical model, it reproducesthe profiles of the mesoscale flux quite well. According to the analytical model, themesoscale heat flux is governed by the temperature deviation at the slope surface, thedepth of the slope-wind layer, the large-scale lapse rate, and the wavelength of thetopographical features. 相似文献