Die regionale Geologie im Hochschulunterricht     

Otto Wilckens 《International Journal of Earth Sciences》1913,4(3):207-209

Ohne Zusammenfassung  相似文献   

400 Jahre Mathematik und Astronomie an der Universität Würzburg: Alma Julia Herbipolensis 1582–1982     

Otto Volk 《Celestial Mechanics and Dynamical Astronomy》1982,28(1-2):243-250

Ohne Zusammenfassung

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400 years mathematics and astronomy at the Wurzburg University: Alma Julia herbipolensis 1582–1982

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s. O. Volk, Mathematik, Astronomie und Physik in der Vergangenheit der Universität Würzburg, Festschrift 1982.

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Paper presented at the 1981 Oberwolfach Conference on Mathematical Methods in Celestial Mechanics.  相似文献   

A hydrodynamic pulsation model under subharmonic resonance     

Toshiki Aikawa  Otto Bruegman 《Astrophysics and Space Science》1987,137(1):115-127

We found a hydrodynamic pulsation model of yellow supergiants under subharmonic resonance. It is confirmed that the feature of pulsation by the resonance is long-lived in the model by performing the hydrodynamical simulation for a long time.  相似文献   

Einiges zur Geometrie der Lagekugelbesetzung     

Otto Mellis 《Mineralogy and Petrology》1954,4(1-4):138-144

Ohne ZusammenfassungMit 3 Textabbildungen.  相似文献   

Gibt es auch im Diluvium orogene Phasen?     

Otto Wittmann 《International Journal of Earth Sciences》1941,32(3):337-367

Ohne Zusammenfassung  相似文献   

Structure of the Shear-Wave Low-Velocity Channel in the Western United States     

Tuncay Yasar  Otto W. Nuttli 《Geophysical Journal International》1974,37(3):353-364

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A source for hyperbolic cosmic dust particles     

Herbert A. Zook  Otto E. Berg 《Planetary and Space Science》1975,23(1):183-203

Earlier analyses of the Pioneer 8 and 9 experimental meteoroid data have shown that the detectors on these two spacecraft are intercepting meteoroids with hyperbolic orbital parameters. It is shown in this paper that these results are entirely consistent with and, indeed, to be expected from other observations of the interplanetary meteoroid complex. Collisional breakup of meteoroids and post-collision radiation pressure modification of their orbits is found to be a sufficient cause for the observed results. Details of the calculations as well as of the results are presented.  相似文献   

Flux–Profile Relationships Over a Fetch Limited Beech Forest     

Ebba Dellwik  Niels Otto Jensen 《Boundary-Layer Meteorology》2005,115(2):179-204

The influence of an internal boundary layer and a roughness sublayer on flux–profile relationships for momentum and sensible heat have been investigated for a closed beech forest canopy with limited fetch conditions. The influence was quantified by derivation of local scaling functions for sensible heat flux and momentum (_h and _m) and analysed as a function of atmospheric stability and fetch. For heat, the influences of the roughness sublayer and the internal boundary layer were in agreement with previous studies. For momentum, the strong vertical gradient of the flow just above the canopy top for some wind sectors led to an increase in _m, a feature that has not previously been observed. For a fetch of 500 m over the beech forest during neutral atmospheric conditions, there is no height range at the site where profiles can be expected to be logarithmic with respect to the local surface. The different influence of the roughness sublayer on _h and _m is reflected in the aerodynamic resistance for the site. The aerodynamic resistance for sensible heat is considerably smaller than the corresponding value for momentum.  相似文献   

Spatial and time variations of the interplanetary microparticle flux analysed from deep space probes pioneers 8 and 9     

J.A.M. Mcdonnell  Otto E. Berg  F.F. Richardson 《Planetary and Space Science》1975,23(1):205-214

The first results of a comprehensive computer analysis of over 300 front film and grid coincidence events is presented using statistical tests on the observed data. The short term time dependence of the observed flux is entirely commensurate with a random Poisson distribution and any possible contributions from discrete “cometary showers” must certainly be of relatively minor significance compared to the sporadic background for mass > 10^?13 g. Periodic seasonal variations of ～ 20 per cent of the average rate are observed common to Pioneers 8 and 9. These variations could reflect on the cometary nature of the source or alternatively indicate the presence of an interstellar component. The mass spectrum of the flux in the range 10^?11?10^?13 g indicates an increasing flux of particles to the lowest limits of mass detected, with a derived flux of Φ = 1·4 × 10^?12m^?0·68 (g) m^?2 sec^?1(2π ster.)^?1.  相似文献   

The Jiddat al Harasis 073 strewn field,Sultanate of Oman     

Edwin GNOS  Silvio LORENZETTI  Otto EUGSTER  A. J. Timothy JULL  Beda A. HOFMANN  Ali Al‐KATHIRI  Manuel EGGIMANN 《Meteoritics & planetary science》2009,44(3):375-387

Abstract— The recently discovered Jiddat al Harasis (JaH) 073 strewn field is the largest found so far in the Sultanate of Oman, covering an area of 19 × 6 km. The 3463 single stones collected range in weight from 52.2 kg down to <1 g (total weight 600.8 kg) and show a pronounced mass sorting. The strewn field shape can be approximated by a NW‐SE‐oriented ellipsoid, indicating an atmospheric entry from SE at a low angle relative to the surface. The meteorite belongs to the L6 ordinary chondrite group and shows S4 average shock grade. Smaller stones generally show a higher weathering grade resulting in a spread from W2 and W4. Enhanced weathering of the stones causing fragmentation after the fall is observed in sandy depressions. Five ¹⁴C measurements on stones of variable size and weathering grade yielded ¹⁴C from 3.8 to 49.9 dpm/kg. Three samples give a ¹⁴C/ ¹⁰Be age consistent with about 14.4 ka. For two samples the cosmogenic, trapped, and radiogenic noble gases were measured. The ratio of the ⁴He and ⁴⁰Ar gas retention ages of 0.29 ± 0.10 and that of the ³He and ²¹Ne cosmic ray exposure ages of 0.36 ± 0.08 Ma indicate that JaH 073 experienced a complex exposure history and lost ⁴He and ⁴⁰Ar due to a major collision. Fragmentation statistics indicate a single major atmospheric disruption and an originally relatively spherical shape of the object. Assuming the material collected represents the majority of fallen mass, and 90–99% of the original weight was lost by ablation, the pre‐atmospheric minimum radius of the meteoroid with density 3.4 g cm^?3would have been at least 75 cm.  相似文献