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G. A. Kovaltsov I. G. Usoskin L. G. Kocharov H. Kananen P. J. Tanskanen 《Solar physics》1995,158(2):395-398
Response of Alma-Ata neutron monitor for solar neutrons from the 15 June 1991 was studied. We considered this response as a test for various scenarios of proton acceleration during the flare. The analysis of neutron monitor is an evidence in favour of the assumption of two acts of proton acceleration at impulsive and post-impulsive phases of the flare. 相似文献
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G. Kremser J. Woch K. Mursula P. Tanskanen B. Wilken R. Lundin 《Annales Geophysicae》1995,13(6):595-607
The magnetospheric ion composition spectrometer MICS on the Swedish Viking satellite provided measurements of the ion composition in the energy range 10.1 keV/e\leqE/Q\leq326.0 keV/e. Data obtained during orbit 842 were used to investigate the ion distribution in the northern polar cusp and its vicinity. The satellite traversed the outer ring current, boundary region, cusp proper and plasma mantle during its poleward movement. H+ and He++ ions were encountered in all of these regions. He+ ions were present only in the ring current. The number of O+ and O++ ions was very small. Heavy high-charge state ions typical for the solar wind were observed for the first time, most of them in the poleward part of the boundary region and in the cusp proper. The H+ ions exhibited two periods with high intensities. One of them, called the BR/CP event, appeared at energies up to 50 keV. It started at the equatorward limit of the boundary region and continued into the cusp proper. Energy spectra indicate a ring current origin for the BR/CP event. Pitch angle distributions show downward streaming of H+ ions at its equatorward limit and upward streaming on the poleward side. This event is interpreted as the result of pitch angle scattering of ring current ions by fluctuations in the magnetopause current layer in combination with poleward convection. The other of the two periods with high H+ ion intensities, called the accelerated ion event, was superimposed on the BR/CP event. It was restricted to energies \leq15 keV and occurred in the poleward part of the boundary region. This event is regarded as the high-energy tail of magnetosheath ions that were accelerated while penetrating into the magnetosphere. The cusp region thus contains ions of magnetospheric as well as of magnetosheath origin. The appearance of the ions depends, in addition to the ion source, on the magnetic field configuration and dynamic processes inside and close to the cusp. 相似文献
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The aurora and other phenomena in near Earth space are becoming a considerable part of the science curriculum in upper secondary school (high school) in Norway. Introducing scientific methods to the young students is an important objective of the education, but experimental experience is mainly restricted to simple laboratory exercises under controlled conditions; observations of uncontrollable natural phenomena are generally left to academic scientists and researchers. The Space Physics Group and The Science Education and Outreach Group at The Department of Physics and Technology, University of Bergen, are constructing a Space Science Suitcase with a set of simple versions of instruments for monitoring solar and geophysical activity in near Earth space. The instruments will be lent to physics classes in upper secondary schools. 相似文献
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The present paper is a state-of-the-art report on an attempt to create a suitable legend for a small-scale map for land-use planning and to test this legend by compiling a map of this type for part of Scandinavia. 相似文献
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During 1984 and 1985, the Geological Survey of Finland carried out regional geochemical mapping of till, at a scale of 1:2,000,000, as part of a programme to produce data for the first Geochemical Atlas of Finland. The Atlas is designed to give comprehensive background information on the distribution of elements in rocks, soils, and the surficial environment. 相似文献
6.
Usoskin I. G. Kovaltsov G. A. Kananen H. Mursula K. Tanskanen P. J. 《Solar physics》1997,170(2):447-452
Cycles of phase evolution of solar activity and cosmic-ray variations are reconstructed by means of the delay component method, which allows us to study the temporal behaviour of time lag between solar activity and cosmic-ray cycle phases. It is shown that the period of the late 20th cycle was very unusual. We have found a delay in the phase of the solar activity cycle with respect to that of cosmic rays and discuss the heliospheric conditions responsible for this delay. 相似文献
7.
Nitrogen, Silicon and Zooplankton Controlling the Baltic Spring Bloom: An Experimental Study 总被引：1，自引：0，他引：1
H. Kuosa R. Autio P. Kuuppo O. Setälä S. Tanskanen 《Estuarine, Coastal and Shelf Science》1997,45(6):813-821
The importance of nitrogen, silicon and grazing for the development of the planktonic spring bloom of the transition area between the Baltic Proper and the Gulf of Finland was studied in a laboratory experiment. Water for this experiment was collected prior to the onset of the spring bloom in early April 1991. At this time, inorganic nutrient concentrations were still at their annual maxim. In the experiment, conducted in plastic tanks, the nitrate level was doubled and silicate level tripled by single and combined additions. One tank was filtered with a 100 μm net to exclude large grazers of phytoplankton. Two unmanipulated controls were used. The tanks were maintained at +2 °C for a 3 week period in 12 h of daylight (60 μE m−2s−1), during which time their nutrient and phytoplankton dynamics were followed. All added inorganic nitrogen was swiftly taken up inducing rapid phytoplankton growth; consequently, available phosphorus must have met the needs of growth. The results showed the limiting nature of nitrogen on the maximum primary productivity and chlorophyll aconcentration. Silicate additions affected the structure of the phytoplankton assemblage by promoting specifically the growth of the diatomChaetoceros holsaticusSchütt, which produced resting spores at later stages of the bloom, whileChaetoceros wighamiiBrightwell was the dominant diatom species in other tanks. The absence of large grazers had no effect on phytoplankton dynamics. 相似文献
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G. Kremser R. Rasinkangas P. Tanskanen B. Wilken G. Gloeckler 《Annales Geophysicae》1994,12(2-3):152-168
Measurements with the ion charge-energy-mass spectrometer CHEM on the AMPTE/CCE spacecraft were used to investigate the origin of energetic He+ and He++ ions observed in the equatorial plane at 3\leqL\leq9. Special emphasis was laid on the dependence of long-term average distributions on magnetic local time (MLT) and the geomagnetic activity index Kp. The observations are described in terms of the phase space densities f1 (for He+) and f2 (for He++). They confirm preliminary results from a previous study: f1 is independent of MLT, whereas f2 is much larger on the nightside than on the dayside. They show, furthermore, that f1 increases slightly with Kp on intermediate drift shells, but decreases on high drift shells (L\geq7). f2 increases with Kp on all drift shells outside the premidnight sector. Within this sector a decrease is observed on high drift shells. A simple ion tracing code was developed to determine how and from where the ions move into the region of observations. It provides ion trajectories as a function of the ion charge, the magnetic moment and Kp. The ion tracing enables a distinction between regions of closed drift orbits (ring current) and open convection trajectories (plasma sheet). It also indicates how the outer part of the observation region is connected to different parts of the more distant plasma sheet. Observations and tracing show that He++ ions are effectively transported from the plasma sheet on convection trajectories. Their distribution in the observation region corresponds to the distribution of solar wind ions in the plasma sheet. Thus, energetic He++ ions most likely originate in the solar wind. On the other hand, the plasma sheet is not an important source of energetic He+ ions. Convection trajectories more likely constitute a sink for He+ ions, which may diffuse onto them from closed drift orbits and then get lost through the magnetopause. An ionospheric origin of energetic He+ ions is unlikely as well, since the source mechanism should be almost independent of Kp. There is considerable doubt, however, that a plausible mechanism also exists during quiet periods that can accelerate ions to ring current energies, while extracting them from the ionosphere. It is concluded, therefore, that energetic He+ ions are mainly produced by charge exchange processes from He++ ions. This means that most of the energetic He+ ions constituting the average distributions also very likely originate in the solar wind. Additional ionospheric contributions are possible during disturbed periods. 相似文献
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The use of the World Neutron Monitor Network to detect high-energy solar neutrons is discussed in detail. It is shown that the existing network can be used for the routine detection of intense sporadic solar-neutron events whenever they occur. A technique is suggested involving the weighted summation of responses of separate monitors to solar neutrons. It is demonstrated that the use of this method improves the significance of solar-neutron event detection. Different results of the simulation of the neutron-monitor sensitivity to solar neutrons have been tested with respect to their application for practical use. It is shown that the total number of neutrons with energy above 300 MeV injected from the Sun during a solar flare can be estimated directly from the time-integrated neutronmonitor response to solar neutrons without any model assumptions. The estimation technique has been developed. 相似文献
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