Roughness of the lunar soil     

Kari Lumme  Hannu Karttunen  William M. Irvine 《Earth, Moon, and Planets》1985,33(1):19-29

In situ measurements at the lunar surface at millimeter resolution by the Apollo astronauts have been analyzed. Several statistical parameters have been determined for the landing site. The surface roughness has been found to be very nearly gaussian. The root-mean-square slopes have been obtained over scales between 0.5 mm and 5 cm. They steadily decrease with increasing scale length from 58° to 2° and are in reasonable agreement with radar-measured values. The autocorrelation coefficient of the height distribution has also been obtained. It has a scale-length of 0.7 mm.Adjunct Professor at the University of Massachusetts.Visiting Scholar at the University of Massachusetts.  相似文献   

A Critical review of theoretical models of negatively polarized light scattered by atmosphereless solar system bodies     

Yu. G. Shkuratov  K. Muinonen  E. Bowell  K. Lumme  J. I. Peltoniemi  M. A. Kreslavsky  D. G. Stankevich  V. P. Tishkovetz  N. V. Opanasenko  L. Y. Melkumova 《Earth, Moon, and Planets》1994,65(3):201-246

About a dozen physical mechanisms and models aspire to explain the negative polarization of light scattered by atmosphereless celestial bodies. This is too large a number for the reliable interpretation of observational data. Through a comparative analysis of the models, our main goal is to answer the question: Does any one model have an advantage over the others? Our analysis is based on new laboratory polarimetric and photometric data as well as on theoretical results. We show that the widely used models due to Hopfield and Wolff cannot realistically explain the phase-angle dependence of the degree of polarization observed at small phase angles. The so-called interference or coherent backscattering mechanism is the most promising model. Models based on that mechanism use well-defined physical parameters to explain both negative polarization and the opposition effect. They are supported by laboratory experiments, particularly those showing enhancement of negative polarization with decreasing particle size down to the wavelength of light. According to the interference mechanism, pronounced negative branches of polarization, like those of C-class asteroids, may indicate a high degree of optical inhomogeneity of light-scattering surfaces at small scales. The mechanism also seems appropriate for treating the negative polarization and opposition effects of cometary dust comae, planetary rings, and the zodiacal light.  相似文献   

Rare species, habitat diversity and functional redundancy in marine benthos   总被引：1，自引：0，他引：1  

Kari E. Ellingsen  Judi E. Hewitt  Simon F. Thrush 《Journal of Sea Research》2007,58(4):291-301

Macro-ecological theories relating species richness, abundance, range size, biological traits and environmental tolerance have rarely been tested in marine soft-sediments, despite the spatial extent of these habitats and the inherent richness of resident communities. This study examines the contribution of rare species to marine soft-sediment communities from New Zealand, focussing on the relationships of range size with abundance, environment, habitat diversity and life history traits. 54% of the 351 species sampled exhibited restricted ranges (found at ≤ 2 sites). In contrast to many terrestrial systems, we observed only a weak positive relationship between abundance and frequency of occurrence. Restricted-range species were not randomly distributed, with their distribution related to habitat characteristics, suggesting an important link between habitat diversity and rarity. They exhibited a similar range of traits to the total observed species pool, suggesting that they are not only important to biodiversity but could play a role in stability. Restricted range species were generally not small and this, together with the number of different biological traits represented, suggests that rare species are important to the functioning of marine systems. Thus, our results highlight the importance of considering rare species in habitat-based approaches to conservation.  相似文献   

Organochlorine contaminants in fish and polycyclic aromatic hydrocarbons in sediments from the Barents Sea   总被引：2，自引：0，他引：2  

Stange  Kari; Klungsoyr  Jarle 《ICES Journal of Marine Science》1997,54(3):318-332

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Shape of the Cassini division in different colors     

Karl Lumme 《Icarus》1975,24(4):483-491

The true shape of the Cassini division of Saturn's rings in red, yellow, green, and blue light has been derived from photographs of high quality, taking into account the correction due to the spreading of light. It is evident that the division is not completely dark. Its minimum brightness is about 20% of that of ring B and the width of the division 0″.44±0″.05.  相似文献   

Mid‐Weichselian interstadial in Kolari,western Finnish Lapland     

Veli‐Pekka Salonen  Julien Moreau  Outi Hyttinen  Kari O. Eskola 《Boreas: An International Journal of Quaternary Research》2014,43(3):627-638

Finnish Lapland is known as an area where numerous sites with sediments from Pleistocene glacial and interglacial periods occur. Recent sedimentological observations and dating call for reinterpretation of the record, which shows a complicated Mid‐Weichselian ice‐sheet evolution within the ice‐divide zone. Here, a large, previously unstudied section from a former Hannukainen iron mine was investigated sedimentologically and dated with optically stimulated luminescence (OSL). Ten sedimentary units were identified displaying a variety of depositional environments (glacial, glaciolacustrine, fluvial and aeolian). They are all – except for the lowermost, deeply weathered till – interpreted to be of Mid‐ or Late Weichselian/Holocene age. Five OSL samples from fluvial sediments give ages ranging from 55 to 35 ka, indicating two MIS 3 ice‐free intervals of unknown duration. The Mid‐Weichselian interstadial was interrupted by a re‐advance event, which occurred later than 35 ka and caused glaciotectonic deformation, folding and stacking of older sediments. This new evidence emphasizes the importance of the Kolari area when unravelling the complex Late Pleistocene glacial history of northern Finland and adjacent regions.  相似文献   

On induction effects at EISCAT and IMAGE magnetometer stations     

Ari Viljanen  Kirsti Kauristie  Kari Pajunpää 《Geophysical Journal International》1995,121(3):893-906

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Performance of ERNE in particle flux anisotropy measurement     

E. Riihonen  J. Torsti  A. Anttila  J. Kuusela  M. Lumme  E. Valtonen 《Annales Geophysicae》1996,14(5):503-509

The HED particle detector of the ERNE experiment to be flown on the SOHO spacecraft is unique compared to the earlier space-born detectors in its high directional resolution (better than 2°, depending on the track inclination). Despite the fixed view cone due to the three-axis stabilization of the spacecraft, the good angular and temporal resolution of the detector provides a new kind of opportunity for monitoring in detail the development of the anisotropies pertaining, for example, to the onset of SEP events, or passage of shock fronts related to gradual events. In order to optimize the measurement parameters, we have made a preflight simulation study of the HED anisotropy measurement capabilities. The purpose was to prove the feasibility of the selected measurement method and find the physical limits for the HED anisotropy detection. The results show HED to be capable of detecting both strong anisotropies related to impulsive events, and smoother anisotropies associated with gradual events.  相似文献   

On the formation of Saturn's rings     

Kari Lumme 《Astrophysics and Space Science》1972,15(3):404-414

It is shown that the formation of Saturn's ring C can be explained by the action of solar radiation pressure on the small ring particles. If the age of the rings is 1.6×10⁸ yr, the predicted optical thickness of ring C, as a function of the distance from the planet, can then be shown to be in agreement with the measured one. The disruption of a solid satellite as the origin of the rings is shown to be quite plausible. If, in Roche's limit, the molecular cohesion is taken into account, the disruption distance of a satellite having the mass of the rings seems to be in agreement with the average distance of the ring system.  相似文献   

Glacial Geology. An introduction for engineers and earth scientists: edited by N. Eyles,Pergamon Press,Oxford 1983. 409 pp. ISBN 0-08-030264-5 (Hardcover) £33.50 ISBN 0-08-030263-7 (Flexicover) £9.95     

Kari Garnes 《Quaternary Science Reviews》1985,4(1):xvii-xviii

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