Ionospheric plasma acceleration at Mars: ASPERA-3 results     

R. Lundin  D. Winningham  R.A. Frahm  M. Holmström  M. Yamauchi  J.R. Sharber  A. Fedorov  J.-J. Thocaven  H. Hayakawa  D.R. Linder  C. Curtis  B.R. Sandel  M. Carter  H. Koskinen  P. Riihelä  T. Säles  N. Krupp  M. Fränz  S. McKenna-Lawler  S. Orsini  E. Roelof  S. Livi  P. Wurz 《Icarus》2006,182(2):308-319

The Analyzer of Space Plasma and Energetic Atoms (ASPERA) on-board the Mars Express spacecraft (MEX) measured penetrating solar wind plasma and escaping/accelerated ionospheric plasma at very low altitudes (250 km) in the dayside subsolar region. This implies a direct exposure of the martian topside atmosphere to solar wind plasma forcing leading to energization of ionospheric plasma. The ion and electron energization and the ion outflow from Mars is surprisingly similar to that over the magnetized Earth. Narrow “monoenergetic” cold ion beams, ion beams with broad energy distributions, sharply peaked electron energy spectra, and bidirectional streaming electrons are particle features also observed near Mars. Energized martian ionospheric ions (O⁺, O⁺₂, CO⁺₂, etc.) flow in essentially the same direction as the external sheath flow. This suggests that the planetary ion energization couples directly to processes in the magnetosheath/solar wind. On the other hand, the beam-like distribution of the energized plasma implies more indirect energization processes like those near the Earth, i.e., energization in a magnetized environment by waves and/or parallel (to B) electric fields. The general conditions for martian plasma energization are, however, different from those in the Earth's magnetosphere. Mars has a weak intrinsic magnetic field and solar wind plasma may therefore penetrate deep into the dense ionospheric plasma. Local crustal magnetization, discovered by Acuña et al. [Acuña, M.J., Connerey, J., Ness, N., Lin, R., Mitchell, D., Carlsson, C., McFadden, J., Anderson, K., Rème, H., Mazelle, C., Vignes, D., Wasilewski, P., Cloutier, P., 1999. Science 284, 790-793], provide some dayside shielding against the solar wind. On the other hand, multiple magnetic anomalies may also lead to “hot spots” facilitating ionospheric plasma energization. We discuss the ASPERA-3 findings of martian ionospheric ion energization and present evidences for two types of plasma energization processes responsible for the low- and mid-altitude plasma energization near Mars: magnetic field-aligned acceleration by parallel electric fields and plasma energization by low frequency waves.  相似文献   

Preface     

Kazuki Koketsu  Kim B. Olsen 《Journal of Seismology》2008,12(2):131-132

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Location of the bow shock and ion composition boundaries at Venus—initial determinations from Venus Express ASPERA-4     

C. Martinecz  M. Fränz  N. Krupp  E. Dubinin  S. Barabash  M. Holmström  M. Yamauchi  Y. Futaana  H. Gunell  J.D. Winningham  J. Scherrer  D.R. Linder  E. Kallio  W. Schmidt  H.E.J. Koskinen  J. Luhmann  E.C. Roelof  C.C. Curtis  B.R. Sandel  J.-A. Sauvaud  J.-J. Thocaven  S. McKenna-Lawler  R. Cerulli-Irelli  A. Mura  P. Wurz  P. Bochsler  K. Szego  T.L. Zhang 《Planetary and Space Science》2008,56(6):780-784

For the first time since 1992 when the Pioneer Venus Orbiter (PVO) ceased to operate, there is again a plasma instrument in orbit around Venus, namely the ASPERA-4 flown on Venus Express (inserted into an elliptical polar orbit about the planet on April 11, 2006). In this paper we report on measurements made by the ion and electron sensors of ASPERA-4 during their first five months of operation and, thereby, determine the locations of both the Venus bow shock (BS) and the ion composition boundary (ICB) under solar minimum conditions. In contrast to previous studies based on PVO data, we employ a 3-parameter fit to achieve a realistic shape for the BS. We use a different technique to fit the ICB because this latter boundary cannot be represented by a conic section. Additionally we investigate the dependence of the location of the BS on solar wind ram pressure (based on ASPERA-4 solar wind data) and solar EUV flux (using a proxy from Earth).  相似文献   

Response spectral attenuation relationships for Sumatran-subduction earthquakes and the seismic hazard implications to Singapore and Kuala Lumpur   总被引：1，自引：0，他引：1  

Kusnowidjaja Megawati  Tso-Chien Pan  Kazuki Koketsu 《Soil Dynamics and Earthquake Engineering》2005,25(1):11-25

Singapore and Kuala Lumpur, the capital of Malaysia, may well represent the classic examples of area with low seismic hazard but with high consequence. Both cities are located in a low-seismicity region of Southeast Asia, where active seismic sources are located more than 300 km away. Seismic designs have not been implemented in this seemingly low-hazard region though distant earthquakes in Sumatra had frequently shaken high-rise structures in the two cities. Several studies have been conducted to systematically assess the seismic hazards of Singapore and the Malay Peninsula. The present research particularly addresses issues in deriving a new set of attenuation relationships of peak ground acceleration (PGA), peak ground velocity (PGV) and response spectral acceleration (RSA) for the Sumatran-subduction earthquakes. To be relevant for the seismic hazard assessment of the remote metropolises, the derived attenuation relationships cover a long distance range from 150 to 1500 km. The attenuation relationships are derived using synthetic seismograms that account for source and path effects. The uncertainties in rupture parameters, such as stress drop, strike, dip and rake angles, have been defined according to the regional geological and tectonic settings as well as the ruptures of previous earthquakes. The seismic potential of the Sumatran subduction zone are high in the region from 2°N to 5°S as there has been no recurrence of great thrust events since 1861. A large event with M_w greater than 7.8 in this particular subduction zone may be capable of generating destructive ground motions in Singapore and Kuala Lumpur, even at a distance of 700 km.  相似文献   

Radial and 2D colour properties of E+A galaxies   总被引：1，自引：0，他引：1  

Chisato Yamauchi  Tomotsugu Goto 《Monthly notices of the Royal Astronomical Society》2005,359(4):1557-1574

We investigated the radial colour gradient and two-dimensional (2D) colour properties of 22 E+A galaxies with  5.5 < Hδ equivalent width(EW) < 8.5 Å  and 49 normal early-type galaxies as a control sample at a redshift of <0.2 in the Second Data Release of the Sloan Digital Sky Survey. We found that a substantial number of E+A galaxies exhibit positive slopes of radial colour gradient (bluer gradients toward the centre) which are seldom seen in normal early-type galaxies. We found irregular 'colour morphologies'– asymmetrical and clumpy patterns – at the centre of g − r and r − i 2D colour maps of E+A galaxies with positive slopes of colour gradient. Kolomogorov–Smirnov two-sample tests show that g − r and r − i colour gradient distributions of E+A galaxies differ from those of early-type galaxies with a more than 99.99 per cent significance level. We also found a tight correlation between radial colour gradients and colours, and between radial colour gradients and the 4000-Å break in the E+A sample; E+A galaxies which exhibit bluer colour or weaker D ₄₀₀₀ tend to have positive slopes of radial colour gradient. We compared the GISSEL model and E+A observational quantities,  Hδ EW, D ₄₀₀₀  and u − g colour, and found that almost all our E+A galaxies are situated along a single evolutionary track. Therefore, these results are interpreted as E+A galaxies evolving from  Hδ EW ∼ 8 Å  to  Hδ EW ∼ 5 Å  , with colour gradients changing from positive to negative, and with the irregular 2D colour map becoming smoother, during a time-scale of ∼300 Myr. Our results favour the hypothesis that E+A galaxies are post-starburst galaxies caused by merger/interaction, having undergone a centralized violent starburst.  相似文献   

Parametrized shooting of seismic rays in a spherical earth with discontinuities     

Shutaro Sekine  Kazuki Koketsu 《Geophysical Journal International》2001,146(2):497-503

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Miocene rhyolitic welded tuff infilling a funnel-shaped eruption conduit Shiotani, southeast of Matsue, SW Japan     

K. Kano  H. Matsuura  S. Yamauchi 《Bulletin of Volcanology》1997,59(2):125-135

 At Shiotani, SW Japan, rhyolitic welded tuff forms a steep-sided funnel-shaped body, confined by Paleogene granitic rocks to an elliptical area 1–1.5 km across. The Shiotani welded tuff is pervasively welded and foliated concordantly with the contact that dips inward at angles of 70–90°. In contrast, nearby contemporary volcaniclastic deposits are non-welded and gently inclined. Near the contact with the granite, the tuff is plastically deformed and shows lineations that plunge inward at angles of 40–65°. Lithic and crystal clasts in the rheomorphic outer part are rotated in a plane normal to the foliations and parallel to the lineations indicating downward flow of the welded tuff. The geometry and internal structures suggest that the Shiotani welded tuff was emplaced and welded in a funnel-shaped eruption conduit. Upon collapse of a plinian or phreatoplinian eruption column, the majority of the conduit-filling pyroclasts probably fell back en masse into the conduit. Heat and steam from underlying magma and diffusion of interstitial volatiles into the glass perhaps reduced the viscosity of juvenile pyroclasts and facilitated welding in the conduit, especially at deep levels. The hot welded pyroclasts then flowed down the conduit wall during welding compaction and retreat of the magma. These processes resulted in increased welding toward the contacts and welding foliations concordant with the steep wall. Emplacement of nearby correlative volcaniclastic mass-flow deposits in a shelf to upper bathyal environment suggests a possibility that, when active, the Shiotani conduit was under the sea. Welding compaction would occur even under the sea provided that the steam generated in the upper part of the conduit fill prevented water access. Received: 28 February 1996 / Accepted: 5 May 1997  相似文献   

Effect of estradiol-17β on pituitary-thyroidal axis of Japanese eel (Anguilla japonica)     

Qu Xiancheng  Masaki Nagae  Sinji Adachi  Kohei Yamauchi 《海洋学报(英文版)》2001,20(4):585-596

In teleost sPeCies, it is well accepted that estradiol--l75 (E2 )is generated from ovarian fOl-licles stimulated by pituitary gonadOtropins (GTH) (Nagahama, l987). FUrthermore, E2 canstimulate hepatic vitellngenesis and elevate plasrna yOlk protein precursor vite1lOgenin, totalCa and W levels in several teleosts (KorSgaard and Petersen, l976, l978; Whiteheadet al., l978; Elliott et al., l979; Pertersen et al., l983; Wallace, 1985; tapigliati etal., 1999). On the other hand, many stud…  相似文献   

1978和2005年宫城近海地震的动力学震源模拟:破裂能解释     

Takeshi Kimura  Kazuki Koketsu  Hiroe Miyake  Takashi Miyatake  袁志祥 《世界地震译丛》2010,(6)

对1978和2005年发生在同一板块边界而震级不同的日本宫城近海地震建立了自发动力破裂模型,再现了由运动学震源模型所预测的滑动和破裂速度。对这两次地震的动力学震源参数进行比较,可使我们看到同一断层上不同震源过程的破裂动力学特征。特别是,我们比较了应力降和破裂能,在这两次地震中,二者可以进行稳定的评估。在整个断层面上和两次地震破裂的凹凸体上,两个模型中应力降的最大值和平均值几乎相同。另外,1978年地震的震级比2005年的大,它的破裂能值不仅是在整个断层面上,而且在多次破裂的凹凸体上也比2005年的大。这些结果与先前用地震矩所做的破裂能标度的研究结果一致。我们还将破裂能值与以前研究中所估算的其他内陆地震的能值进行了对比,我们得到的宫城近海地震的值较小。造成这种不一致的原因可能是内陆浅源地震和俯冲带深源地震在构造背景上的差异。  相似文献   

Finite-element simulations of long-period ground motions: Japanese subduction-zone earthquakes and the 1906 San Francisco earthquake     

Yasushi Ikegami  Kazuki Koketsu  Takeshi Kimura  Hiroe Miyake 《Journal of Seismology》2008,12(2):161-172

Large earthquakes at shallow depths commonly excite long-period ground motions in distant sedimentary basins, thereby inflicting damage upon large-scale structures. For example, the 2003 Tokachi-oki earthquake, Japan, damaged oil tanks in the Yufutsu Basin, located 250 km from the epicenter. Similar long-range effects were also observed during the 2004 earthquake off Kii Peninsula, Japan. In this study, we present the results of simulations of these earthquakes undertaken using the finite element method (FEM) with a voxel mesh. In addition, to examine whether the 1906 San Francisco earthquake excited long-period ground motions in the Los Angeles-area basins, we performed long-period ground motion simulations of most of the California region. The FEM simulations confirmed the importance of path effects for the development of long-period ground motions.  相似文献