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Marina Krafft 《Solar physics》1968,5(4):462-470
The instrumental profile of a Lyot-filter with 0.5 Å pass-band for H has been determined from photographic spectra obtained with a large grating spectrograph and a continuous light source.After fine adjustment of the filter, the transmission profile in parallel light agrees closely with the theoretical profile as given by crystal optics. The peak transmission has been found to be 12% of the incident unpolarized radiation.Convolving the measured instrumental profile with the average solar spectral distribution near H, it can be shown that the parasitic light (transmission outside the main pass-band) contributes 10% to the total light flux with the filter centered on the line. At wavelength shifts of 0.5 and 0.8Å, the parasitic light contribution is 25% and 40%, respectively.The deformation of the line-profile of various solar phenomena (faculae, filaments, flares) by the instrumental profile is discussed quantitatively.Mitteilungen aus dem Fraunhofer Institut Nr. 82. 相似文献
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Earth, Moon, and Planets - 相似文献
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Earth, Moon, and Planets - 相似文献
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Oldoinyo Lengai in the Tanzanian rift valley is the only active carbonatite volcano in the world and its natrocarbonatitic lavas are unique in composition. The characteristics of effusive natrocarbonatite activity in June 1988 were studied and fresh samples were directly collected from active carbonatitic lava lakes and flows. Analyses of these samples provide the first information on natrocarbonatites since these unusual volcanic rock type was first described from the 1960–1961 eruptions. The analytical results constrain the original chemistry of fresh natrocarbonatite. Temperatures in lava lakes and of carbonatite lava flows range 491–544°C. The natrocarbonatite lava is extremely fluid at these temperatures and reaches incandescence. The most common variety of natrocarbonatite is porphyritic with abundant phenocrysts of nyerereite (Na0.82K0.19)2(Ca, Sr, Ba)0.975(CO3)2 and gregoryite Na1.74K0.1(Ca, Sr, Ba)0.16CO3, with complex substitution of (CO3)2- by (SO4)2-, (PO4)3-, F-, and Cl-. A phenocryst-poor to aphyric natrocarbonatite variety reflects residual liquids separating from the crystal-rich porphyritic flows. Sylvite, fluorite, and Fe-alabandite (Mn0.7Fe0.3S) have been identified as additional primary magmatic phases. Rare phases in the matrix are witherite (BaCO3) and sellaite (MgF2). Sylvite and gregoryite, and to a lesser extent nyerereite, are water-soluble and are responsible for the immediate decomposition and chemical alteration of natrocarbonatites under atmospheric conditions. A peralkaline combeite-bearing nephelinite lava is closely related to the natrocarbonatite activity, and is isotopically indistinguishable. It is likely that these two magma compositions are related by liquid immiscibility. The unusual hyperalkaline composition of both magma types makes Oldoinyo Lengai an exotic volcano, and its carbonatites have extreme compositions, and are not representative of carbonatites in general. 相似文献
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B. Lundin C. Krafft G. Matthieussent F. Jiricek J. Shmilauer P. Triska 《Annales Geophysicae》1996,14(1):27-32
A numerical solution of the dispersion equation for electromagnetic waves in a hot magnetized collisionless plasma has shown that, in a current-free ionospheric plasma, the distortion of the electron distribution function reproducing the downward flow of a thermal electron component and the compensating upward flow of the suprathermal electrons, which are responsible for the resulting heat flux, can destabilize quasi-electrostatic ion sound waves. The numerical analysis, performed with ion densities and electron temperature taken from the data recorded by the Interkosmos-24 (IK-24, Aktivny) satellite, is compared with a VLF spectrum registered at the same time on board. This spectrum shows a wide frequency band emission below the local ion plasma frequency. The direction of the electron heat flux inherent to the assumed model of VLF emission generation is discussed. 相似文献
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Ehrenfreund Pascale Krafft Catherine Kochan Hermann Pirronello Valerio 《Earth, Moon, and Planets》1998,80(1-3):1-1
Earth, Moon, and Planets - 相似文献
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Leif Nøttestad Lise D. Sivle Bjørn A. Krafft Lise Langård Valantine Anthonypillai Matteo Bernasconi Herdis Langøy Bjørn E. Axelsen 《Marine Ecology》2014,35(2):221-232
The Norwegian Sea is a migration and feeding ground for fin whales (Balaenoptera physalus) and humpback whales (Megaptera novaeangliae) in summer. During the last decade, significant structural changes in the prey community, including northerly expansion and movement in the distribution of pelagic fish species, have been reported from this ecosystem. However, little information on whale feeding ecology exists in the Norwegian Sea and surrounding waters. A total of 59 fin whales and 48 humpback whales were sighted during 864 h of observation over an observation distance of about 8200 nmi (15,200 km) in the Norwegian Sea from 15 July to 6 August 2006 and 2007. The fin whale group size, as mean (±SD), varied between one and five individuals (2.1 ± 1.2 ind.) and humpback whale group size varied between one and six individuals (2.5 ± 1.7 ind.). Fin‐ and humpback whales were observed mainly in the northern part of the study area, and were only found correlated with the presence of macro‐zooplankton in cold Arctic water. Humpback whales were not correlated with the occurrence of adult Norwegian spring‐spawning herring (Clupea harengus) except for the northernmost areas. Despite changes in the whale prey communities in the Norwegian Sea, no apparent changes in fin‐ or humpback whale distribution pattern could be found in our study compared to their observed summer distribution 10–15 years ago. 相似文献
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