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891.
892.
R. M. Suleiman J.L. Kohl A. V. Panasyuk A. Ciaravella S.R. Cranmer L.D. Gardner R. Frazin R. Hauck P.L. Smith G. Noci 《Space Science Reviews》1999,87(1-2):327-330
The Ultraviolet Coronagraph Spectrometer (UVCS) on the Solar and Heliospheric Observatory (SOHO) has been used to measure
spectral line profiles for H I Lyα in the south polar coronal hole at projected heliocentric heights from 3.5 to 6.0 R⊙ during 1998 January 5–11. Observations from 1.5 to 2.5 R⊙ were made for comparison. The H I Lyα profile is the only one observable with UVCS above 3.5 R⊙ in coronal holes. Within this region the outflowing coronal plasma becomes nearly collisionless and the ionization balance
is believed to become frozen.
In this paper, the 1/e half widths of the coronal velocity distributions are provided for the observed heights. The velocity
distributions include all motions contributing to the velocities along the line of sight (LOS). The observations have been
corrected for instrumental effects and interplanetary H I Lyα. The half widths were found to increase with projected heliographic
height from 1.5 to 2.5 R⊙ and decrease with height from 3.5 to 5 R⊙.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
893.
The current university education of electrical and electronics engineers has evolved from the well-established system of the 1950's to a wishy-washy mixture operating with lots of ill-motivated or less-qualified students, a process mostly accelerated by the growth in the telecommunications industry. External projects take staff time and the curriculum continues to threaten youngsters with de-focused mathematics. The computer age has reduced the interest in experimental research, and the continuation of science in the systems level may be in danger 相似文献
894.
P.R. Gazis F.B. McDonald R.A. Burger S. Chalov R.B. Decker J. Dwyer D.S. Intriligator J.R. Jokipii A.J. Lazarus G.M. Mason V.J. Pizzo M.S. Potgieter I.G. Richardson L.J. Lanzerotti 《Space Science Reviews》1999,89(1-2):269-305
We discuss the structure and evolution of CIRs and their successors in the outer heliosphere. These structures undergo significant
evolution as they are convected to greater heliocentric distances. A progression of different types of structure are observed
at increasing distance from the Sun. Similar structures are observed at similar heliocentric distance at different portions
of the solar cycle. CIRs and their successors are associated with many important physical processes in the outer heliosphere.
We discuss the relationship between these structures and recurrent phenomena such as cosmic ray variations, and review some
of the associated theoretical models on the role of corotating structures and global merged interaction regions (GMIRs) in
global cosmic ray modulation. We also discuss some outstanding questions related to the origin of non-dispersive quasi-periodic
particle enhancements associated with CIRs and their successors in the outer heliosphere.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
895.
Thermal drill sampling system onboard high-velocity impactors for exploring the subsurface of Europa
P. Weiss K.L. Yung N. Kömle S.M. Ko E. Kaufmann G. Kargl 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The planned Europa Jupiter System Mission (EJSM) will provide a unique opportunity to place scientific instruments onto the surface of Jupiter’s moon Europa in the late 2020s. After the Galileo mission, this will be a long awaited chance to have a close glimpse into some of the mysteries of this moon. Care must be taken in the choice of in-situ science that will be undertaken on the surface. 相似文献
896.
V.P. Kim J.Y. Liu V.V. Hegai 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
This paper presents the results of modeling the ionospheric effect of the seismogenic electrostatic field (SEF) seen at the earth’s surface as a perturbation of the vertical atmospheric electrostatic field in the earthquake preparation zone. The SEF distribution at ionospheric altitudes is obtained as an analytical solution of the continuity equation for the electric current density. It is shown that at night, the horizontally large scale SEF can efficiently penetrate into the ionosphere and produce noticeable changes in the horizontal distribution of the F region electron density. The results suggest that the seismogenic electrostatic field could be a possible source for the ionospheric variations observed over Taiwan before the strong Chi Chi earthquake of September 21, 1999. 相似文献
897.
V. Ballu P. Bonnefond S. Calmant M.-N. Bouin B. Pelletier O. Laurain W.C. Crawford C. Baillard O. de Viron 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
Measuring ground deformation underwater is essential for understanding Earth processes at many scales. One important example is subduction zones, which can generate devastating earthquakes and tsunamis, and where the most important deformation signal related to plate locking is usually offshore. We present an improved method for making offshore vertical deformation measurements, that involve combining tide gauge and altimetry data. We present data from two offshore sites located on either side of the plate interface at the New Hebrides subduction zone, where the Australian plate subducts beneath the North Fiji basin. These two sites have been equipped with pressure gauges since 1999, to extend an on-land GPS network across the plate interface. The pressure series measured at both sites show that Wusi Bank, located on the over-riding plate, subsides by 11 ± 4 mm/yr with respect to Sabine Bank, which is located on the down-going plate. By combining water depths derived from the on-bottom pressure data with sea surface heights derived from altimetry data, we determine variations of seafloor heights in a global reference frame. Using altimetry data from TOPEX/Poseidon, Jason-1, Jason-2 and Envisat missions, we find that the vertical motion at Sabine Bank is close to zero and that Wusi Bank subsides by at least 3 mm/yr and probably at most 11 mm/yr. 相似文献
898.
B. Rani T.P. Krichbaum B. Lott L. Fuhrmann J.A. Zensus 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The GeV observations by Fermi-LAT give us the opportunity to characterize the high-energy emission (100 MeV–300 GeV) variability properties of the BL Lac object S5 0716+714. In this study, we performed flux and spectral analysis of more than 3 year long (August 2008 to April 2012) Fermi-LAT data of the source. During this period, the source exhibits two different modes of flux variability with characteristic timescales of ∼75 and ∼140 days, respectively. We also notice that the flux variations are characterized by a weak spectral hardening. The GeV spectrum of the source shows a clear deviation from a simple power law, and is better explained by a broken power law. Similar to other bright Fermi blazars, the break energy does not vary with the source flux during the different activity states. We discuss several possible scenarios to explain the observed spectral break. 相似文献
899.
S. Bingert P. Zacharias H. Peter B.V. Gudiksen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The structure and dynamics of a box in a stellar corona can be modeled employing a 3D MHD model for different levels of magnetic activity. Depending on the magnetic flux through the surface the nature of the resulting coronal structures can be quite different. We investigate a model of an active region for two sunspots surrounded by magnetic field patches comparable in magnetic flux to the sunspots. The model results in emission from the model corona being concentrated in loop structures. In Gudiksen and Nordlund (2005) the loops seen in EUV and X-ray emission outline the magnetic field, following the general paradigm. However, in our model, where the magnetic field is far from a force-free state, the loops seen in X-ray emission do not follow the magnetic field lines. This result is of interest especially for loops as found in areas where the magnetic field emerging from active regions interacts with the surrounding network. 相似文献
900.
A technological process of removing a complex-shaped ceramic core from the interior of GTE thin-walled blade castings is considered. We propose an aluminium oxide-based method for removing a core by leaching accompanied by process intensification with a carboxylic acid additive. 相似文献