A 2D numerical study of explosive events in the solar atmosphere     

S.-P. Jin  B. Inhester  D. Innes 《Solar physics》1996,168(2):279-295

Two-dimensional (2D) compressible magnetohydrodynamic simulations are performed to explore the idea that the asymmetric reconnection between newly emerging intranetwork magnetic field flux and pre-existing network flux causes the explosive events in the solar atmosphere. The dependence of the reconnection rate as a function of time on the density and temperature of the emerging flux are investigated. For a Lundquist number of L _u= 5000 we find that the tearing mode instability can lead to the formation and growth of small magnetic islands. Depending on the temperature and density ratio of the emerging plasma, the magnetic island can be lifted upward and convected out of the top boundary, or is suppressed downward and convected out of the top boundary, or is suppressed downward nad submerged below the bottom boundary. The motions of the magnetic islands with different direction are accompanied respectively with upward or downward high velocity flow which might be associated with the red- and blue-shifted components detected in the explosive events.  相似文献   

Radon global simulations with the multiscale chemistry and transport model MOCAGE   总被引：2，自引：0，他引：2  

B. JOSSE  P. SIMON  V.-H. PEUCH 《Tellus. Series B, Chemical and physical meteorology》2004,56(4):339-356

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Simulating colour variations in pulsating sdB stars     

B. Ramachandran  C.S. Jeffery 《Astrophysics and Space Science》2004,289(3-4):441-444

After briefly recalling basic facts about the metallicity gradients inspiral galaxies, we summarize two recent N-body gas-dynamical modelsthat implement a non-instantaneous gas recycling and point our their potential for an improved treatment of the chemical evolution ingalactic disks.  相似文献   

Optical properties of solid and liquid sulfur at visible and infrared wavelengths     

R. Sasson  R. Wright  E.T. Arakawa  B.N. Khare  Carl Sagan 《Icarus》1985,64(3):368-374

Knowledge of the optical constants of elemental sulfur has potential applications to Venus, Jupiter, Io, Amalthea, and the Earth. The real part, n, of the index of refraction of liquid sulfur (at 133°C) and of solid orthorhombic sulfur (at 25°C) for the wavelength range 0.4–2.0 μm were measured ellipsometrically. The imaginary part, k, of the refractive index of liquid sulfur was obtained by transmittance measurements at the same temperature and wavelength range. The reflectance of semi-infinite slabs of solid and liquid sulfur is calculated using the measured n and k values. We confirm that sulfur melts on Io would be classified as “black” by the Voyager imaging system.  相似文献   

Eclipsing binaries in extrasolar planet transit surveys: the case of SuperWASP     

B. Willems  U. Kolb  S. Justham 《Monthly notices of the Royal Astronomical Society》2006,367(3):1103-1112

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Progress in coronal physics     

Jack B. Zirker 《Solar physics》1985,100(1-2):281-287

This paper reviews research highlights of the past five years. Considerable progress has been made in observing and interpreting coronal mass ejections. The stability of coronal loops is much better understood and new observations of the onset of wind streams in coronal holes have been made. Observations from the Solar Maximum Mission should helpt to clarify the physics of the active corona.The mechanisms that heat the corona and accelerate the high-speed wind streams remain to be identified, however.Operated by the Association of Universities for Research in Astronomy, Inc., under contract with the National Science Foundation.  相似文献   

Relative and absolute ages of individual craters and the rate of infalls on the moon in the post-imbrium period     

Ralph B. Baldwin 《Icarus》1985,61(1):63-91

This paper contains a reasonably successful attempt to determine relative ages and then absolute ages of individual craters younger than Imbrium, and the rate of infalls onto the Moon as a function of time. After the tail of the massive premare bombardment became depleted before 3 aeons (1 aeon = 10⁹ years) ago, there was a period of minimal numbers of infalls. The rate of infalls increased rather steadily from this minimum to the present. The rate in the geologically recent past (0.3 aeon) was about two times that found for the period immediately after the last of the major lave outpourings (3.2 aeons). Absolute ages were determined for large craters (?8 km) from crater counts on the surfaces within and on the rims of the large craters. Key dates were 0 and 0.3 aeon for terrestrial meteoritic craters, 3.2, 3.5, 3.8, and 3.82 aeons for the various mare surfaces according to the determinations of D.E. Wilhelms (1980, Geologic history of the Moon, U.S. Geol. Surv. Prof. Pap.) and 3.85 aeons from the formation of Imbrium.  相似文献   

The Second International Hydrographic Technical Conference: Plymouth, 3–7 September 1984     

P.B. Beazley 《Marine Policy》1985,9(1):78-79

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The Martian hydrologic cycle: Effects of CO₂ mass flux on global water distribution     

Philip B. James 《Icarus》1985,64(2):249-264

The Martian CO₂ cycle, which includes the seasonal condensation and subsequent sublimation of up to 30% of the planet's atmosphere, produces meridional winds due to the consequent mass flux of CO₂. These winds currently display strong seasonal and hemispheric asymmetries due to the large asymmetries in the distribution of insolation on Mars. It is proposed that asymmetric meridional advection of water vapor on the planet due to these CO₂ condensation winds is capable of explaining the observed dessication of Mars' south polar region at the current time. A simple model for water vapor transport is used to verify this hypothesis and to speculate on the effects of changes in orbital parameters on the seasonal water cycle.  相似文献   

World Fisheries Conference     

B.F. Dada 《Marine Policy》1985,9(3):252-253

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