Heat budget of Flakevatn,a subpolar lake     

Kaare Strøm 《Aquatic Sciences - Research Across Boundaries》1966,28(1):43-45

Zusammenfassung Durch Kenntnis von Sommer- und Wintertemperaturen in dem südnorwegischen Gebirgssee Flakevatn (Meeresh?he 1448 m) konnte die Thermik des subpolaren Seetypus charakterisiert werden. Im Sommer herrscht in Flakevatn wiederholte Isothermie bei relativ hohen Temperaturen, im Winter wird der See ganz ausserordentlich abgekühlt (Fig. 1, Tabelle). Die sommerliche W?rmespeicherung betr?gt +5800, die winterliche −22500 cal/cm².   相似文献   

A Three-Dimensional Global Model Study of Carbonyl Sulfide in the Troposphere and the Lower Stratosphere   总被引：4，自引：0，他引：4  

Erik Kjellström 《Journal of Atmospheric Chemistry》1998,29(2):151-177

Global distributions of carbonyl sulfide and carbon disulfide have been calculated with a three-dimensional global model of the atmospheric general circulation (ECHAM). The model calculates a global sink strength for carbonyl sulfide of 0.3 Tg S yr^-1, with vegetation uptake being the largest sink. With this sink strength, the sources have to be close to the lower limit of the present estimate in the literature. The calculated mixing ratios are higher in the Southern Hemisphere than in the Northern Hemisphere. This interhemispheric gradient is the opposite of what is observed demonstrating that the present knowledge of the distribution of sinks and sources is not fully adequate. The model calculations support the idea that the open oceans could act as a net sink of carbonyl sulfide. The calculated stratospheric photolysis of carbonyl sulfide constitutes about 4% of the total sink of carbonyl sulfide. A stratospheric production of sulfate from carbonyl sulfide of 0.013 Tg S yr^-1 is obtained, which is 3 to 12 times less than what is needed to maintain the stratospheric sulfate aerosol layer. Although these results are associated with uncertainties, due to the low upper boundary and coarse vertical resolution of the model, they support recent findings of a low stratospheric production of sulfate from carbonyl sulfide. Instead, sulfur dioxide transported from the troposphere is calculated to be the most important precursor for the stratospheric sulfate aerosol layer.  相似文献   

Refractional influences in astrometry and geodesy     

Prof. Erik Tengström 《Journal of Geodesy》1978,52(4):329-334

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Meeting of the Special Study Group V.49 of IAG on “Use of Geodetic Data for Studies of the Earth-moon System”     

Prof. Erik Tengström 《Journal of Geodesy》1978,52(4):335-336

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Correlation and spectrum properties of the potential gradient and space-charge density in the atmospheric surface layer     

C. O. Oluwafemi  E. Ungethüm  S. Israelsson  E. Knudsen 《Pure and Applied Geophysics》1974,112(3):533-543

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Vertical profiles of aerosol scattering and absorption measured in situ during the North Atlantic Aerosol Characterization Experiment (ACE‐2)     

Elisabeth Öström  Kevin J. Noone 《Tellus. Series B, Chemical and physical meteorology》2000,52(2):526-545

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Long-term infrared variability of the UX Ori-type star SV Cep     

A. Juhász  T. Prusti  P. Ábrahám  C. P. Dullemond 《Monthly notices of the Royal Astronomical Society》2007,374(4):1242-1252

We investigate the long-term optical–infrared variability of SV Cep and explain it in the context of an existing UX Ori (UXOR) model. A 25-month monitoring programme was completed with the Infrared Space Observatory in the 3.3–100 μm wavelength range. Following a careful data reduction, the infrared light curves were correlated with the variations of SV Cep in the V band. A remarkable correlation was found between the optical and the far-infrared light curves. In the mid-infrared regime, the amplitude of variations is lower, with a hint for a weak anti-correlation with the optical changes. In order to interpret the observations, we modelled the spectral energy distribution of SV Cep assuming a self-shadowed disc with a puffed-up inner rim, using a two-dimensional radiative transfer code. We found that modifying the height of the inner rim, the wavelength dependence of the long-term optical–infrared variations is well reproduced, except the mid-infrared domain. The origin of variation of the rim height might be fluctuation in the accretion rate in the outer disc. In order to model the mid-infrared behaviour, we tested adding an optically thin envelope to the system, but this model failed to explain the far-infrared variability. Infrared variability is a powerful tool to discriminate between models of the circumstellar environment. The proposed mechanism of variable rim height may not be restricted to UXOR stars, but might be a general characteristic of intermediate-mass young stars.  相似文献   

Simulation of Quiet-Sun Hard X-Rays Related to Solar Wind Superhalo Electrons     

Wen Wang  Linghua Wang  Säm Krucker  Iain Hannah 《Solar physics》2016,291(5):1357-1367

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The design and flight performance of the PoGOLite Pathfinder balloon-borne hard X-ray polarimeter     

M. Chauvin  H.-G. Florén  M. Jackson  T. Kamae  T. Kawano  M. Kiss  M. Kole  V. Mikhalev  E. Moretti  G. Olofsson  S. Rydström  H. Takahashi  J. Lind  J.-E. Strömberg  O. Welin  A. Iyudin  D. Shifrin  M. Pearce 《Experimental Astronomy》2016,41(1-2):17-41

In the 50 years since the advent of X-ray astronomy there have been many scientific advances due to the development of new experimental techniques for detecting and characterising X-rays. Observations of X-ray polarisation have, however, not undergone a similar development. This is a shortcoming since a plethora of open questions related to the nature of X-ray sources could be resolved through measurements of the linear polarisation of emitted X-rays. The PoGOLite Pathfinder is a balloon-borne hard X-ray polarimeter operating in the 25-240 keV energy band from a stabilised observation platform. Polarisation is determined using coincident energy deposits in a segmented array of plastic scintillators surrounded by a BGO anticoincidence system and a polyethylene neutron shield. The PoGOLite Pathfinder was launched from the SSC Esrange Space Centre in July 2013. A near-circumpolar flight was achieved with a duration of approximately two weeks. The flight performance of the Pathfinder design is discussed for the three Crab observations conducted. The signal-to-background ratio for the observations is shown to be 0.25 ±0.03 and the Minimum Detectable Polarisation (99 % C.L.) is (28.4 ±2.2) %. A strategy for the continuation of the PoGOLite programme is outlined based on experience gained during the 2013 maiden flight.  相似文献   

Wind Statistics from a Forested Landscape     

Johan Arnqvist  Antonio Segalini  Ebba Dellwik  Hans Bergström 《Boundary-Layer Meteorology》2015,156(1):53-71

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