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881.
V. A. Parkhomov G. N. Zastenker M. O. Riazantseva B. Tsegmed T. A. Popova 《Cosmic Research》2010,48(1):86-100
We present the results of studying the magnetospheres’s response to sharp changes of the solar wind flow (pressure) based
on observations of variations of the ions flux of the solar wind onboard the Inreball-1 satellite and of geomagnetic pulsations (the data of two mid-latitude observatories and one auroral observatory are used).
It is demonstrated that, when changes of flow runs into the magnetosphere, in some cases short (duration ~ < 5 min) bursts
of geomagnetic pulsations are excited in the frequency range Δf~ 0.2–5 Hz. The bursts of two types are observed: noise bursts without frequency changes and wide-band ones with changing
frequency during the burst. A comparison is made of various properties of these bursts generated by pressure changes at constant
velocity of the solar wind and by pressure changes on the fronts of interplanetary shock waves at different directions of
the vertical component of the interplanetary magnetic field. 相似文献
882.
We investigate the relative occurrence rate for various types of the solar wind and their geoeffectiveness for magnetic storms
with Dst < —50 nT. Both integrated effect for the entire time 1976–2000 and variations during this period of 2.5 cycles of solar activity
are studied As raw data for the analysis we have used the catalog of large-scale types of the solar wind for the period 1976-2000
(see ftp://ftp.iki.rssi.ru/omni/) created by us with the use of the OMNI database (http://omni.web.gsgc.nasa.gov) [1] and
described in detail in [2]. The average annual numbers of different type of events are as follows: 124 ±81 for the heliospheric
current sheet (HCS), 8 ±6 for magnetic clouds (MC), 99 ±38 for Ejecta, 46 ±19 for Sheath before Ejecta, 6 ±5 for Sheath before
MC, and 63 ±15 for CIR. The measurements that allowed one to determine a source in the solar wind were available only for
58% of moderate and strong magnetic storms (with index Dst < —50 nT) during the period 1976–2000. Magnetic clouds (MC) are shown to be the most geoeffective (~61%). The CIR events and
Ejecta with Sheath region are three times less geoeffective (~20–21 %). Variations of occurrence rate and geoeffectiveness
of various types of the solar wind in the solar cycle are discussed. 相似文献
883.
E. N. Parker 《Space Science Reviews》2009,144(1-4):15-24
We review some longstanding scientific mysteries related to solar magnetism, with final attention to the mystery of the “turbulent diffusion” essential for the theoretical α ω-dynamo that is believed to be the source of the magnetic fields of the Sun. Fundamental difficulties with the concept of turbulent diffusion of magnetic fields suggest that the solar dynamo problem needs to be reformulated. An alternative dynamo model is proposed, but it remains to be shown that the model can provide the quantitative aspects of the cyclic magnetic fields of the Sun. 相似文献
884.
N. Straumann 《Space Science Reviews》2009,148(1-4):25-36
In this written version of a pre-dinner-speech at the workshop “The Nature of Gravity” at ISSI I illustrate Pauli’s science primarily with material that has not formally been published by him, but was communicated in detailed letters to eminent colleagues and friends. 相似文献
885.
886.
The organization principles of constructing the European system of warning about dangerous situations in the outer space are
considered in the paper. 相似文献
887.
Design of a three-axial accelerometer-seismometer, constructed on the basis of two-coordinate sensors (sensitive elements)
of high and low accelerations, is considered in the paper. This instrument is applied for gravi-inertial measurements. Basic
characteristics of the instrument are described, as well as the technique and results of its standardization. 相似文献
888.
A problem of cruciform parachute deployment is considered. The process of deployment is simulated using the present-day numerical methods in the continuum mechanics, that is, the method of concentrated masses and the method of vortex frames. The calculation results are compared with the experimental data. 相似文献
889.
An analysis of the existing astrometric and radar observations of the Apophis asteroid is performed. On the basis of this
analysis, characteristics of future measurements of the asteroid orbit and limitation on their conduction are accepted. A
proposed launching of a spacecraft to the asteroid in order to obtain high-accuracy measurements of its distance and radial
velocity is also considered. Trajectories of the flight to the asteroid in 2012–2022 are studied. Estimates of the accuracy
of the Apophis position determination at various sets of both available and planned measurements at various numbers of determined
parameters are obtained. The method of estimating accuracy is similar to that used in [1] for the Vega project. 相似文献
890.