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  • Articles  (35)
  • Leonids 1999  (23)
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  • Articles  (35)
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  • Springer  (35)
  • American Association for the Advancement of Science
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  • 1
    ISSN: 1573-0417
    Keywords: Antarctica ; saline lakes ; weightedaveraging ; transfer function ; diatom analysis ; palaeolimnology ; climate change
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Geosciences
    Notes: Abstract The relationship between surface sediment diatom assemblages and measured limnological variables in thirty-three coastal Antarctic lakes from the Vestfold Hills was examined by constructing a diatom-water chemistry dataset. Previous analysis of this dataset by canonical correspondence analysis revealed that salinity accounted for a significant amount of the variation in the distribution of the diatom assemblages. Weighted-averaging regression and calibration of this diatom-salinity relationship was used to establish a transfer function for the reconstruction of past lakewater salinity from fossil diatom assemblages. Weighted-averaging regression and calibration with classical deshrinking provided the best model for salinity reconstructions and this was applied to the fossil diatom assemblages from one of the saline lakes in the Vestfold Hills in order to assess its potential for palaeosalinity and palaeoclimate reconstruction.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Journal of paleolimnology 20 (1998), S. 253-265 
    ISSN: 1573-0417
    Keywords: Late Quaternary ; diatoms ; climate change ; vegetation change ; shallow ; subalpine ; Crowfoot Lake ; Alberta ; paleolimnology
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Geosciences
    Notes: Abstract The late Quaternary diatom record from subalpine Crowfoot Lake, Banff National Park, Alberta (lat. 51° 61′N; long. 116° 31′W) has been analyzed. Results are related to independently inferred vegetation and climate changes. No diatoms were found in the basal diamict that predates 11330 14C yr BP. Very few occur until ca. 10 10014 C yr BP probably due to the short time between de-glaciation and an advance of the Crowfoot Glacier during the ‘Younger Dryas Chron’. Initial pioneering species were characteristic of alkaline water and calcareous organic sediments. They appeared as sediments became organic and laminated suggesting increasing water clarity, and as the Pinus-dominated forest expanded and the climate warmed. After ca. 9060 14C yr BP diatom numbers increased rapidly, reaching a maximum prior to the Mazama tephra; they remained high until ca. 3500 14C yr BP. The period between ca. 9060 and 3500 14C yr saw timberline elevation increase and the dominance of xerophytic taxa. These are consistent with early to mid-Holocene warmth and aridity. Diatom productivity reflects the warm climate and presumably longer ice-free season, a stable catchment and transparent water. Decreases in diatom productivity coincide with a vegetation change with reduction of xerophytic taxa and the appearance of a closed Picea-Abies forest, hence a cooler, wetter climate at ca. 4100 to 3500 14C yr BP. The diatom numbers during the Neoglacial were of the same magnitude as prior to ca. 9060 14C yr BP. Small species of Fragilaria (overwhelmingly Fragilaria construens v. venter) became extremely dominant during the period of high diatom productivity, and remained so thereafter. Recovery of the lake appears to have been rapid after deposition of the Mazama tephra. Maximum occurrence of Cyclotella radiosa occurred ca. 8000 14C yr BP during the warm early Holocene and may reflect this warmer climate, a longer ice-free season than presently, perhaps less turbid water, or it may reflect a subtly higher nutrient status of the lake water. The diatom record of Crowfoot Lake has responded with sensitivity, particularly in terms of productivity, to the Holocene vegetation and climate changes.
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Journal of paleolimnology 20 (1998), S. 205-215 
    ISSN: 1573-0417
    Keywords: subarctic lakes ; diatoms ; paleolimnology ; climate change ; Cyclotella ; Finnish Lapland
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Geosciences
    Notes: Abstract Diatoms were analysed from a 30-cm long sediment core obtained from remote subarctic Lake Saanaärvi (69°03′N, 20°52′E) in order to trace possible changes in the lake. Diatom assemblages were relatively constant throughout the core, except in the top 4–5 cm (approx 1850 A.D.) where relative frequencies of Aulacoseira italica subsp. subarctica, A. lirata var. biseriata, Cyclotella comensis and C. glomerata increased markedly. No significant trends were observed in the weighted averaging (WA) reconstructed pH values. Several hypotheses, including (i) airborne pollution, (ii) climatic change, and (iii) catchment disturbances have been put forth to explain the recent changes in diatom assemblages. The diatom change coincides with a marked increase in mean annual temperature that has been documented in the area since the termination of the Little Ice Age. Our evidence favours climate change as the main causative mechanism for the observed diatom compositional changes, although other explanations cannot be ruled out.
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  • 4
    ISSN: 1573-0794
    Keywords: Early Earth ; H2O ; HCN ; Leonids 1999 ; lower thermosphere ; O3 ; mesosphere ; meteors ; micro-wave ; radio
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract To identify the effect of meteor showers on the molecular content of the upper atmosphere of the Earth, we have carried out ground-based observations of atmospheric HCN. HCN radio observations at CSO (Hawaii) on Nov 18/19, 1999, the night after the second Leonid shower maximum, show unusually low HCN abundances above 45 km altitude, which are only recovered after sunrise. We also investigated UARS/HALOE satellite data on H2O and O3. No correlation appears of year round H2O and O3 around 55 km with annual meteor showers, nor with meteor activity at the time of the 1998 Leonid shower.
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 82-83 (1998), S. 391-398 
    ISSN: 1573-0794
    Keywords: Leonids 1999 ; meteor ; meteor physics ; photon counting imager ; ultraviolet
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract During the 1999 Leonid meteor storm, a camera with a UV sensitive image intensifier and CCD readout (ICCD), was operated at the Wise Observatory in Mitzpe Ramon, Israel. The photocathode spectral response, together with the transmittance of the atmosphere, limited the sensitivity to a narrow band around 320 nm. The aim was to obtain quantitative information on emitted radiance in this band, for comparison with recordings of the same tracks in other wavelengths. The field of view of 7°.2 × 5°.7 was pointed to the East at about 60° elevation and the video recorded from 21 until 03 UT, Nov. 18, 1999. At least five clear images of meteor tracks were recorded, and compared with the signals from known stars. It was concluded that the brightest track gave an estimated monochromatic magnitude at 320 nm peaking at ∼ −4. Some of the peculiarities of astronomical observation with a photon-counting imager are discussed.
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  • 6
    ISSN: 1573-0794
    Keywords: Airglow ; FeO ; Leonids 1999 ; mesosphere ; meteors ; persistent train
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract We report the detection of a broad continuum emission dominating the visual spectrum of a Leonid persistent train. A comparison with laboratory spectra of FeO "orange arc" emission at 1 mbar shows a general agreement of the band position and shape. The detection of FeO confirms the classical mechanism of metal atom catalyzed recombination of ozone and oxygen atoms as the driving force behind optical emission from persistent trains. Sodium and iron atoms are now confirmed catalysts.
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  • 7
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 82-83 (1998), S. 555-564 
    ISSN: 1573-0794
    Keywords: lower thermosphere ; Leonids 1999 ; mesosphere ; meteors ; neutral atom debris layer ; Potassium
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract We have performed an experiment to study the impact of the 1999 Leonid meteor storm on the upper atmosphere potassium layer. For the experiment, we used a ground-based K-lidar located at the Observatorio del Teide on the island of Tenerife (28°N, 17°W). As is now known from external sources, the activity of the storm exhibited a sharp peak of activity on November 18, 1999 close to 02:05 UT with a full width at half maximum of only 45 min. Due to unfavorable weather conditions at our lidar site, we could not observe the behavior of the K layer immediately before or during the meteor storm. However, about 1 h past the peak of the Leonid storm, the clouds above the site started to show small holes. Hence, between 03:24 and 05:22 UT, we were able to perform lidar soundings of the K layer above our site. From those we can conclude that the 1999 Leonid meteor storm has not led to an outstanding enhancement of the upper atmosphere potassium layer.
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  • 8
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 82-83 (1998), S. 575-598 
    ISSN: 1573-0794
    Keywords: Hypervelocity impacts ; Leonids 1999 ; luminous efficiencies ; lunar craters ; meteoroids ; meteors ; Moon
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract The first unambiguous detection of meteoroids impacting the night side of the Moon was obtained during the 1999 Leonid storm. Up to eight optical flashes were recorded with CCD video cameras attached to small telescopes on November 18, 1999. Six impacts were videotaped by at least two independent observers at the same times and lunar locations, which is perhaps the strongest evidence for their collisional nature. The flashes were clearly above the noise and lasted for less than 0.02 s. Although previous observational efforts did not succeed in detecting impact flashes, additional candidates have been reported in the literature. The evidence accumulated so far implies that small telescopes equipped with high speed cameras can be used as a new tool for studying meteoroid streams, sporadic meteoroids, and hypervelocity collisions. In this review we discuss the various intervening parameters for detectability of flashes on the night side of the Moon (geometrical effects, contamination by scattered light from the day side, and properties of the meteoroids such as speed and flux of particles). Particular emphasis is placed on the analysis of the observations in order to derive relevant physical parameters such as luminous efficiencies, impactor masses, and crater sizes. Some of these parameters are of interest for constraining theoretical impact models. From a simple analysis, it is possible to derive the mass distribution of the impactors in the kg range. A more elaborate analysis of the data permits an estimate of the fraction of kinetic energy converted to radiation (luminous efficiency) if the meteoroid flux on the Moon is known. Applied to the 1999 lunar Leonids, these methods yield a mass index of 1.6 ± 0.1 and luminous efficiencies of 2 × 10−3 with an uncertainty of about one order of magnitude. Predictions of visibility of the major annual meteor showers are given for the next few years. These include the forthcoming 2001 Leonid return, for which we estimate detection rates in the visible.
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  • 9
    ISSN: 1573-0794
    Keywords: Comet dust trial ; dispersion ; Leonids 1999 ; meteor ; meteor orbit ; meteor trajectory ; orbital dynamics
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Photographic multi-station observations of 47 Leonid meteors are presented that were obtained from two ground locations in Spain during the 1999 meteor storm. We find an unresolved compact cluster of radiants at α = 153.67 ± 0.05 and δ = 21.70 ± 0.05 for a mean solar longitude of 235.282 (J2000). The position is identical to that of the Nov. 17/18 outburst of 1998, which implies that both are due to comet 55P/Tempel-Tuttle's ejecta from 1899. We also find a halo which contains about 28% of all meteors. The spatial distribution of radiant positions appears to be Lorentzian, with a similar fraction of meteors in the profile wings as the meteor storm activity curve.
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  • 10
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 82-83 (1998), S. 305-312 
    ISSN: 1573-0794
    Keywords: Flux ; Leonids 1999 ; meteors ; meteor shower ; MSX ; population index ; space
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract In November 1997, the Midcourse Space Experiment satellite (MSX) was deployed to observe the Leonid shower from space. The shower lived up to expectations, with abundant bright fireballs. Twenty-nine meteors were detected by a wide-angle, visible wavelength, camera near the limb of the Earth in a 48-minute interval, and three meteors by the narrow field camera. This amounts to a meteoroid influx of 5.5 ± 0.6 10−5 km−2 hr−1 for masses 〉 0.3 gram. The limiting magnitude for limb observations of Leonid meteors was measured at Mv = −1.5 magn. The Leonid shower magnitude population index was 1.6 ± 0.2 down to Mv = −7 magn., with no sign of an upper mass cut-off.
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