The yellow hypergiants     

Cornelis de Jager 《Astronomy and Astrophysics Review》1998,8(3):145-180

We list the main stellar data of known hypergiants and similarly luminous stars, and then concentrate on a review of the yellow hypergiants. These stars are post-red supergiants evolving along blueward loops in the Hertzsprung-Russell diagram. Their properties, their location in the Hertzsprung-Russell diagram and their occasional mass ejections are related to a region of atmospheric instability in the H-R diagram, the Yellow Void. The ‘bouncing against the border of the Void’ of three objects: Cas, HR8752 and IRC+10420, is described. The apparent atmospheric instability of yellow hypergiants is related to the atmospheric pulsations. There are indications that the approach to the Void is associated with an increased amplitude of the pulsation and with enhanced mass loss. The observed small-scale motion field is only apparently strongly supersonic; the observed large stochastic velocities are the quasi-stochastically varying thermal motions in the many hot sheets that occur in the wakes of many small shocks, while the real hydrodynamic velocity component is small and subsonic. This shock-wave field is also responsible for the observed rate of mass loss and for emission in the wings of H. Most yellow hypergiants have envelopes containing gas and dust, but a thick extended envelope, presumably dissipating and showing bipolar outflow, is only known around IRC+10420. At the interface of the bipolar wind and the interstellar medium one or more stationary shocks may develop as is observed in the case of IRC+10420 and suspected with Cas. Received 1 July 1997  相似文献   

Variability of the Arctic front during the last climatic cycle: application of a novel molecular proxy     

Rosell-Melé  Weinelt  Sarnthein  Koç  & Jansen 《地学学报》1998,10(2):86-89

In the Nordic Seas, the Arctic front (AF) marks the boundary between the waters of the North Atlantic Drift/Norwegian Current and those of the Arctic domain. Long- or short-term shifts in the position of the AF may affect climate conditions in the northern hemisphere. Arctic water masses are also the loci of modern open ocean convection; hence, defining these areas in the past is important for reconstructing and modelling ocean circulation and its variability. C₃₇ alkenones are biomarkers for some algae of the Class Prymnesiophyceae (e.g. coccolitho-phorids such as Emiliania huxleyi). These alga occur in most parts of the oceans, in ice-free conditions, and are found nowadays throughout the Nordic Seas. We have related the sedimentary abundance of the tetraunsaturated C₃₇ alkenone (C_37:4) to two types of water masses in the Nordic seas. In locations affected by Atlantic water masses percentages of C_37:4 are less than 5%, whereas in Arctic type water masses these increase to more than 5%. We propose that this observation can be used as a modern analogue to reconstruct the position of the AF in North Atlantic Quaternary sediments. Using this novel molecular proxy we can infer that the southward migration of the AF in the NE Atlantic reached ≈ 50 °N during the last glacial maximum (LGM), but perhaps only 60 °N during the Younger Dryas, and that ocean conditions free of sea ice prevailed throughout the Northern North Atlantic in summer.  相似文献   

Polarimetric analysis and modeling of multifrequency SAR signaturesfrom Gulf Stream fronts     

Jong-Sen Lee Jansen  R.W. Schuler  D.L. Ainsworth  T.L. Marmorino  G.O. Chubb  S.R. 《Oceanic Engineering, IEEE Journal of》1998,23(4):322-333

Using airborne synthetic aperture radar data from the 1990 Gulf Stream Experiment, this paper investigates the polarization and wavelength dependence of radar signatures for narrow fronts with converging flows occurring within the Gulf Stream. The signal-to-background ratios of the cross-polarization backscatter return from a convergent front were found much higher than those of copolarization returns, when the flight path is crossing the front. However, a second convergent front, imaged at 45°, showed that the signal-to-background ratios are nearly equal for co- and cross-polarizations. A polarimetric procedure, which has been successfully used to measure terrain slopes and to generate elevation maps, is applied to the convergent front to explain the polarization and imaging geometry dependence of these radar responses. A theoretical modeling of radar modulation using an ocean wave model and a composite-Bragg scattering model, which incorporates the effect of breaking waves, was developed. Calculations with the model agree reasonably well with the radar measurements at various polarizations for three radar frequencies: P-band (68 cm in wavelength), L-band (24 cm), and C-band (5.7 cm)  相似文献   

Gut content analyses of three dominant Antarctic copepod species during an induced phytoplankton bloom EIFEX (European iron fertilization experiment)     

Svenja Kruse  Sandra Jansen  Sören Krägefsky  & Ulrich Bathmann 《Marine Ecology》2009,30(3):301-312

The diet of three Antarctic copepods, Calanus simillimus , Rhincalanus gigas and Pleuromamma robusta , was studied from samples collected during the European iron fertilization experiment (EIFEX) in austral fall 2004. The diet was investigated using microscopical gut content analysis. The food spectra of the three copepod species showed a clear overlap. The pennate diatom Fragilariopsis kerguelensis was commonly found in all guts. Large numbers of cells were fractured, but some were found complete when arranged as chains. The same was true for the genus Chaetoceros , a centric diatom, of which even their long and complete setae could be observed. In general the ingested food particles extended over a wide size range up to a few 100 μm. The copepod C. simillimus , for example, fed on large foraminifera and swallowed them whole. Compared to C. simillimus and R. gigas , P. robusta guts contained a higher percentage and larger diversity of hard-shelled protozoa including tintinnids, Radiolaria and Acantharia.  相似文献   

Tracing mechanisms controlling the release of dissolved silicon in forest soil solutions using Si isotopes and Ge/Si ratios     

J.-T. Cornelis  B. Delvaux  L. André  S. Opfergelt 《Geochimica et cosmochimica acta》2010,74(14):3913-289

The terrestrial biogenic Si (BSi) pool in the soil-plant system is ubiquitous and substantial, likely impacting the land-ocean transfer of dissolved Si (DSi). Here, we consider the mechanisms controlling DSi in forest soil in a temperate granitic ecosystem that would differ from previous works mostly focused on tropical environments. This study aims at tracing the source of DSi in forest floor leachates and in soil solutions under various tree species at homogeneous soil and climate conditions, using stable Si isotopes and Ge/Si ratios. Relative to granitic bedrock, clays minerals were enriched in ²⁸Si and had high Ge/Si ratios, while BSi from phytoliths was also enriched in ²⁸Si, but had a low Ge/Si ratio. Such a contrast is useful to infer the relative contribution of silicate weathering and BSi dissolution in the shallow soil on the release of DSi in forest floor leachate solutions. The δ³⁰Si values in forest floor leachates (−1.38‰ to −2.05‰) are the lightest ever found in natural waters, and Ge/Si ratios are higher in forest floor leachates relative to soil solution. These results suggest dissolution of ²⁸Si and Ge-enriched secondary clay minerals incorporated by bioturbation in organic-rich horizons in combination with an isotopic fractionation releasing preferentially light Si isotopes during this dissolution process. Ge/Si ratios in soil solutions are governed by incongruent weathering of primary minerals and neoformation of secondary clays minerals. Tree species influence Si-isotopic compositions and Ge/Si ratios in forest floor leachates through differing incorporation of minerals in organic horizons by bioturbation and, to a lesser extent, through differing Si recycling.  相似文献   

Instability regions in the upper HR diagram     

Cornelis de Jager  Alex Lobel  Hans Nieuwenhuijzen  Richard Stothers 《Monthly notices of the Royal Astronomical Society》2001,327(2):452-458

The following instability regions for blueward evolving-supergiants are outlined and compared. (1) Areas in the Hertzsprung–Russell (HR) diagram where stars are dynamically unstable. (2) Areas where the effective acceleration in the upper part of the photospheres is negative, hence directed outward. (3) Areas where the sonic points of the stellar winds (where     are situated inside the photospheres, at a level deeper than     . We compare the results with the positions of actual stars in the HR diagram and we find evidence that the recent strong contraction of the yellow hypergiant HR 8752 was initiated in a period during which     , whereupon the star became dynamically unstable. The instability and extreme shells around IRC+10420 are suggested to be related to three factors:     the sonic point is situated inside the photosphere; and the star is dynamically unstable.  相似文献   

Integrated marine and terrestrial evidence for abrupt Congo River palaeodischarge fluctuations during the last deglaciation     

Fabienne Marret  James D. Scourse  Gerard Versteegh  J. H. Fred Jansen  Ralph Schneider 《第四纪科学杂志》2001,16(8):761-766

We present a high‐resolution reconstruction of tropical palaeoenvironmental changes for the last deglacial transition (18 to 9 cal. kyr BP) based on integrated oceanic and terrestrial proxies from a Congo fan core. Pollen, grass cuticle, Pediastrum and dinoflagellate cyst fluxes, sedimentation rates and planktonic foraminiferal δ¹⁸O ratios, u₃₇^K′ sea‐surface temperature and alkane/alkenone ratio data highlight a series of abrupt changes in Congo River palaeodischarge. A major discharge pulse is registered at around 13.0 cal. kyr BP which we attribute to latitudinal migration of the Intertropical Convergence Zone (ITCZ) during deglaciation. The data indicate abrupt and short‐lived changes in the equatorial precipitation regime within a system of monsoonal dynamics forced by precessional cycles. The phases of enhanced Congo discharge stimulated river‐induced upwelling and enhanced productivity in the adjacent ocean. Copyright © 2001 John Wiley & Sons, Ltd.  相似文献   

Properties and emergence patterns of bipolar active regions     

Karen L. Harvey  Cornelis Zwaan 《Solar physics》1993,148(1):85-118

Patterns in the properties of bipolar active regions are determined throughout Cycle 21. Active regions that emerged on the visible hemisphere were identified on NSO/KP full-disk magnetograms during 29 solar rotations selected from 1975 through 1986. The bipolar active regions are included only once in this sampling; their properties are derived at the time of maximum development. In order to study an unbiased sample over the entire range of areas larger than 2.5 square degrees (or 373 Mm²), their counts are corrected for size-dependent effects that reduce the chance of their identifications.The size distribution of bipolar active regions is a well-defined function that decreases with increasing size. Except for the smallest regions, the shape of the size distribution is independent of the phase of a cycle, only the scaling factor varies. The shape of the size distribution function for bipoles emerging within existing sunspot regions is virtually the same as that for bipoles emerging outside existing regions. Over the cycle, at least 44% of the regions larger than 3.5 square degrees emerge within existing sunspot regions. Hence, the rate at which new regions emerge is much higher within the boundaries of existing sunspot regions than it is in the activity belts outside existing regions. For regions emerging outside of existing sunspot regions, this rate increases by a factor of 3.5 from cycle minimum to maximum, while for new bipoles within existing active regions, the emergence rate varies with a significantly lower magnitude.Through the cycle, for regions in all size bins, the emergence frequencies appear to vary in phase. The frequencies increase by a factor of more than 8 from minimum to maximum for regions larger than 3.5 square degrees, but no more than 4.7 for the smaller regions. Short-term variations in the emergence frequency of regions do not necessarily occur simultaneously for regions of all sizes, implying that the size distribution is variable on time scales of less than six rotations.  相似文献   

Editorial     

Mary F. Wheeler  Clint Dawson  Jan-Dirk Jansen 《Computational Geosciences》2011,15(1):1-1

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New techniques for integral field spectroscopy – II. Performance of the GNIRS IFU     

Jeremy Allington-Smith  Cornelis M. Dubbeldam  Robert Content  David Robertson  James Turner  Bernadette Rodgers  Jonathan Elias  Joris Gerssen †  Mark Swinbank 《Monthly notices of the Royal Astronomical Society》2007,376(2):785-792

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