The effects of the host-substrate properties on maar-diatreme volcanoes: experimental evidence     

Élodie Macorps  Alison H. Graettinger  Greg A. Valentine  Pierre-Simon Ross  James D. L. White  Ingo Sonder 《Bulletin of Volcanology》2016,78(4):26

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D-Rex, a program for calculation of seismic anisotropy due to crystal lattice preferred orientation in the convective upper mantle   总被引：1，自引：0，他引：1  

Édouard Kaminski  Neil M. Ribe  Jules T. Browaeys 《Geophysical Journal International》2004,158(2):744-752

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THE DIRECTIVITY OF SOLAR KILOMETRIC TYPE III BURSTS: ULYSSES–ARTEMIS OBSERVATIONS IN AND OUT OF THE ECLIPTIC PLANE     

HOANG  S.  POQUÉRUSSE  M.  BOUGERET  J.-L. 《Solar physics》1997,172(1-2):307-316

Comparing the records of the radio spectrographs ARTEMIS (100–500 MHz) on the ground and URAP (1–1000 kHz) on the Ulysses spacecraft, we find that most type III bursts extend from the corona to the solar wind. Using the positions of the associated flares, and assuming an average intensity ratio between these two frequency ranges, we derive for the first time the average radiation pattern of interplanetary type III bursts. We find that at 800 kHz it is shifted east of the radial direction by 30° and has a half-width of about 80° at maximum/10; the shift and width increase towards lower frequencies. Ulysses high-latitude observations show that the cross-section perpendicular to the heliospheric equator is about the same. We interpret these properties by refraction effects in local density gradients.  相似文献   

Energy release by the compression of the envelope of a cooling white dwarf     

T. A. Éminzade 《Astrophysics》1974,10(3):248-250

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Explosive He4 burning: I. Kinetics of burning at constant temperature and density     

A. M. Khokhlov  É. V. Érgma 《Astrophysics》1985,23(3):724-732

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Low-mass x-ray binaries and millisecond pulsars     

É. Érgma  A. G. Masevich 《Astrophysics》1993,36(1):82-101

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An equation for the characteristic curve of a family of symmetric periodic orbits     

George Bozis  Bálint Érdi 《Celestial Mechanics and Dynamical Astronomy》1994,59(4):301-311

Szebehely's equation for the inverse problem of Dynamics is used to obtain the equation of the characteristic curve of a familyf(x,y)=c of planar periodic orbits (crossing perpendicularly thex-axis) created by a certain potentialV(x,y). Analytic expressions for the characteristic curves are found both in sideral and synodic systems. Examples are offered for both cases. It is shown also that from a given characteristic curve, associated with a given potential, one can obtain an analytic expression for the slope of the orbit at any point.  相似文献   

Model for horizontal branch of globular clusters     

A. M. Éigenson  N. N. Samus' 《Astrophysics》1975,11(2):247-248

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Products of carbon burning at constant temperature     

O. A. Bessonov  A. D. Kudryashov  É. V. Érgma 《Astrophysics》1978,14(1):91-96

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Existence of the solution of Szebehely's equation in three dimensions using a two-parametric family of orbits     

F. Váradi  B. Érdi 《Celestial Mechanics and Dynamical Astronomy》1983,30(4):395-405

The three-dimensional inverse problem is investigated. A quasi-linear system of partial differential equations is derived for the determination of the potential. The solution of this system is studied by a method of differential geometry. A necessary condition for the solution is derived and the determination of the potential is reduced to algebraic equations written in vectorial form. A few examples are also given.  相似文献