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11.
The synodic recurrence of the Mt. Wilson plage index (MPSI) and the Calgary cosmic ray (CR) intensity is investigated, using
the wavelet power spectra in the range of 18–38 days, during the last three solar cycles. The unique temporal coincidence
between the quasi–synodic MPSI and the CR periods is detected in 1978–1982 (the 21st solar cycle). In the 22nd cycle there
is a very strong MPSI synodic recurrence, from 1989.5 to 1990.5, but it is absent in the CR data. In 1992.5–1993.5 the MPSI
and CR recurrence phenomenon is in good accordance with the solar wind speed and cosmic ray modulation as measured during
the first Ulysses passage around the Sun. The Gnevyshev gap is present in the 27-day recurrence of CR, in agreement with Kudela
et al. (1999).
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
12.
H. Mészárosová H.S. Sawant J.R. Cecatto J. Rybák M. Karlický F.C.R. Fernandes M.C. de Andrade K. Jiřička 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The 22 min long decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare simultaneously by the Brazilian Solar Spectroscope (BSS) and the Ond?ejov radiospectrograph in frequency range 1200–4500 MHz has been analyzed. We have found that the characteristic periods of about 60 s belong to the long-period spectral component of the fast wave trains with a tadpole pattern in their wavelet power spectra. We have detected these trains in the whole frequency range 1200–4500 MHz. The behavior of individual wave trains at lower frequencies is different from that at higher frequencies. These individual wave trains have some common as well as different properties. In this paper, we focus on two examples of wave trains in a loop segment and the main statistical parameters in their wavelet power and global spectra are studied and discussed. 相似文献
13.
Luboš Perek 《Acta Astronautica》1985,12(1):67-69
Measures for the safety of space activities have to be elaborated by the scientific community. They should include principles for collision avoidance, possibly in the form of traffic separation schemes. A reduction of collision probabilities could be achieved by systematic removal of inactive satellites, by establishing disposal orbital belts and by reduction of space debris. Safety of space activities would be enhanced by the adoption of standards for the quality of technical equipment and for the competence of personnel. Also timely information on satellite movement should be made available. 相似文献
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Meteor Phenomena and Bodies 总被引:12,自引:0,他引:12
Zdeněk Ceplecha JiřÍ Borovička W. Graham Elford Douglas O. ReVelle Robert L. Hawkes VladimÍr Porubčan Miloš Šimek 《Space Science Reviews》1998,84(3-4):327-471
Meteoroids can be observed at collision with the Earth's atmosphere as meteors. Different methods of observing meteors are
presented: besides the traditional counts of individual events, exact methods yield also data on the geometry of the atmospheric
trajectory; on the dynamics and ablation of the body in the atmosphere; on radiation; on the spectral distribution of radiation;
on ionization; on accompanying sounds; and also data on orbits. Theoretical models of meteoroid interaction with the atmosphere
are given and applied to observational data. Attention is paid to radar observations; to spectroscopic observations; to experiments
with artificial meteors and to different types of meteor sounds. The proposed composition and structure of meteoroids as well
as their orbits link them to meteorites, asteroids and comets. Meteor streams can be observed as meteor showers and storms.
The rate of influx of meteoroids of different sizes onto Earth is presented and potential hazards discussed.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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