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11.
Martin Connors Paul Chodas Seppo Mikkola Paul Wiegert Christian Veillet Kimmo Innanen 《Meteoritics & planetary science》2002,37(10):1435-1441
Abstract— The newly discovered asteroid 2002 AA29 moves in a very Earth‐like orbit that relative to Earth has a unique horseshoe shape and allows transitions to a quasi‐satellite state. This is the first body known to be in a simple heliocentric horseshoe orbit, moving along its parent planet's orbit. It is similarly also the first true co‐orbital object of Earth, since other asteroids in 1:1 resonance with Earth have orbits very dissimilar from that of our planet. When a quasi‐satellite, it remains within 0.2 AU of the Earth for several decades. 2002 AA29 is the first asteroid known to exhibit this behavior. 2002 AA29 introduces an important new class of objects offering potential targets for space missions and clues to asteroid orbit transfer evolution. 相似文献
12.
Equations are presented for the computation of tangent maps for use in nearly Keplerian motion, approximated by use of a symplectic
leapfrog map. The resulting algorithms constitute more accurate and efficient methods to obtain the Liapunov exponents and
the state transition matrix, and can be used to study chaos in planetary motions, as well as in orbit determination procedures
from observations. Applications include planetary systems, satellite motions and hierarchical, nearly Keplerian systems in
general.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
13.
Numerical integrations have been performed for orbits of Venus', Earth's and Mars' Trojan-asteroid test particles in a self consistent model of the solar system to study the stability of inclined Trojan orbits. In the case of Mars low inclination orbits tend to be unstable while the contrary seems to apply to Venus and Earth, although the stability of some very high inclination orbits may not be excluded on the basis of these computations. 相似文献
14.
Martin Connors Christian Veillet Ramon Brasser Paul Wiegert Paul Chodas Seppo Mikkola Kimmo Innanen 《Meteoritics & planetary science》2004,39(8):1251-1255
Abstract— The newly discovered asteroid 2003 YN107 is currently a quasi‐satellite of the Earth, making a satellite‐like orbit of high inclination with apparent period of one year. The term quasi‐satellite is used since these large orbits are not completely closed, but rather perturbed portions of the asteroid's orbit around the Sun. Due to its extremely Earth‐like orbit, this asteroid is influenced by Earth's gravity to remain within 0.1 AU of the Earth for approximately 10 years (1997 to 2006). Prior to this, it had been on a horseshoe orbit closely following Earth's orbit for several hundred years. It will re‐enter such an orbit, and make one final libration of 123 years, after which it will have a close interaction with the Earth and transition to a circulating orbit. Chaotic effects limit our ability to determine the origin or fate of this object. 相似文献
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16.
Kimmo?T.?TolonenEmail author Klaus?P.?Brodersen Tanya?A.?Kleisborg Kerstin?Holmgren Magnus?Dahlberg Ladislav?Hamerlik Heikki?H?m?l?inen 《Journal of Paleolimnology》2012,47(4):531-547
We sampled living and subfossil phantom midge (Diptera: Chaoboridae) larvae from surface sediments of 21 small lakes in Southern
Sweden to examine the influence of fish and selected abiotic variables on the abundance and species composition of chaoborid
assemblages. We expected total Chaoborus abundance to be inversely correlated with fish abundance and Chaoborus species most sensitive to fish predation to be found only in fishless lakes. We aimed to use the observed relationships to
develop models to reconstruct past fish abundances from chaoborid remains and the abiotic environment. C. flavicans occurred in almost every lake, whereas subfossil C. obscuripes were found in the surface sediments of only one fishless lake. The density of living C. flavicans larvae correlated negatively with fish abundance, lake order and size. The concentration of C. flavicans subfossils was negatively associated with pH, lake size, water transparency and fish abundance. Regression models that included
lake morphometry and landscape position as additional predictors of fish abundance performed better than models that used
only Chaoborus predictors. The explained variance in fish abundance varied from 52 to 86%. Leave-one-out cross-validation indicated moderate
performance of the two best models. These models explained 51 and 56% of the observed untransformed fish density and biomass,
respectively. In addition, all Chaoborus models were unbiased in closely following the 1:1 reference line in plots of observed versus predicted values. These results
are a promising step in developing midge-based paleolimnological reconstructions of past fish abundance, and the approach
might be improved by including chironomid remains in the models. 相似文献
17.
Seppo Mikkola Kimmo Innanen Karri Muinonen Edward Bowell 《Celestial Mechanics and Dynamical Astronomy》1994,58(1):53-64
Observations and results of orbit determination of the first known Mars Trojan asteroid (5261) Eureka are presented. We have numerically calculated the evolution of the orbital elements, and have analyzed the behavior of the motion during the next 2 Myr. Strong perturbations by planets other than Mars seem to stabilize the eccentricity of the asteroid by stirring the high order resonances present in the elliptic restricted problem. As a result, the orbit appears stable at least on megayear timescales. The difference of the mean longitudes of Mars and Eureka and the semimajor axis of the asteroid form a pair of variables that essentially behave in an adiabatic manner, while the evolution of the other orbital elements is largely determined by the perturbations due to other planets. 相似文献
18.
Leena K. L. Nurminen Jukka A. Horppila 《Aquatic Sciences - Research Across Boundaries》2002,64(2):198-206
The objective of the present study was to investigate the importance of emergent macrophytes as refugia in lakes of different trophic status. Furthermore, the effect of water quality on diel changes in the distribution of littoral cladocerans was of interest, with special attention paid on diurnal fluctuations of filter feeder communities, induced by pH changes under a heavy phytoplankton bloom. The study was conducted by investigating littoral cladoceran populations in different zones (inside, at the edge and outside the macrophyte stands) in two basins with divergent water quality. No tendency towards diurnal migration related to emergent macrophytes was observed in the clear-water, mesotrophic Isontalonselkä basin. The dominating cladoceran, Daphnia spp., formed highest densities during daytime in the outer zone. Meanwhile, strong nocturnal cladoceran density peaks in all zones, simultaneous with lowered pH, were witnessed in the very turbid, hypertrophic Kirkkojärvi basin. Reverse horizontal migration was observed in large-bodied filter feeders, Limnosida frontosa and Sida crystallina, conceivably due to predation avoidance from young-of-the-year fish aggregating within the vegetation during the day. 相似文献
19.
Data from a research tower in Lake Ontario are used to study the validity of Monin--Obukhov scaling in the marine atmospheric boundary layer under various wave conditions. It is found that over pure wind seas, the velocity spectra and cospectra follow established universal scaling laws. However, in the presence of swells outrunning weak winds, velocity spectra and cospectra no longer satisfy universal spectral shapes. Here, Monin–Obukhov similarity theory, and the classical logarithmic boundary layers, are no longer valid. It is further shown that, in the presence of such swells, the momentum flux can be significantly modified in comparison to pure wind sea values. The implications of these findings for bulk flux estimations and on the inertial dissipation method for calculating fluxes are discussed. 相似文献
20.
Why we study the geological record for evidence of the solar oscillation about the galactic midplane
John J. Matese Patrick G. Whitman Kimmo A. Innanen Mauri J. Valtonen 《Earth, Moon, and Planets》1996,72(1-3):7-12
The Solar System oscillates about the plane defined by the disk of matter in our Galaxy. This oscillatory motion gives rise to a substantial modulation in the tidally induced flux of Oort cloud comets. An observational determination of the quasi-periodicity of this motion carries with it significant information about the population, distributions, dynamics and origins of short-period and long-period comets. An additional incentive for emphasizing such a study is the information about dark disk matter that a period can yield. If dark disk matter is completely negligible, the amplitude of the solar motion will be sufficiently large that the peak-to-trough flux ratio will be ≈ 2.5 and the plane-crossing period will exceed 40 Myr. Dark disk matter comparable in mass to bright disk matter and distributed in any manner is inconsistent with K-dwarf distributions and can be rejected as a working hypothesis. But if a modest fraction of the disk matter is dark and distributed like the interstellar medium, as is consistent with limits deduced from K-giant and K-dwarf velocity distributions, the peak-to-trough flux ratio can increase to a factor of 4 even though the solar z amplitude is decreased. In that case the period can be as little as 30 Myr and the implied Oort population is smaller by a factor of 3. We should carefully reconsider the geological record as a potential discriminator of these options. 相似文献