排序方式: 共有5条查询结果,搜索用时 0 毫秒
1
1.
2.
3.
P. Nenovski Y. Semkova R. Koleva S. Chapkunov N. Kanchev N. Tabov A. Kanchev O. Vaisberg V. Smirnov G. Zastenker A. Leibov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1982,2(7):27-30
An original instrument for ion energy distribution measurement in ionospheric plasma above the F-layer was designed and launched on board the ‘INTERCOSMOS-BULGARIA-1300’ satellite. The instrument performs differential energy analysis of ion species within the two energy ranges of 1 – 27 eV/q and 0.2–8keV/q. 相似文献
4.
G. N. Zastenker J. Safrankova Z. Nemecek L. Prech I. Cermak I. Vaverka A. Komarek J. Voita L. S. Chesalin B. T. Karimov Yu. N. Agafonov N. L. Borodkova E. A. Gavrilova T. I. Gagua I. T. Gagua P. A. Dalin A. V. D’yachkov I. V. Koloskova A. V. Leibov N. P. Semena V. V. Chernov Ya. I. Markov E. E. Ryazanova M. O. Ryazanrtseva N. N. Shevyrev V. V. Chrapchenkov O. M. Chugunova A. S. Yurasov 《Cosmic Research》2013,51(2):78-89
Design of the plasma spectrometer BMSW (Fast Monitor of the Solar Wind, possessing high temporal resolution) is described in the paper, as well as its characteristics and modes of operation. Some examples of measurements of various properties of the solar wind, made with this instrument installed onboard the high-apogee satellite Spektr-R, are presented. 相似文献
5.
O. L. Vaisberg A. V. Leibov V. N. Smirnov L. A. Avanov J. -J. Bertelier K. Torcar F. Leblan V. F. Babkin V. A. Grishin V. Baumjohann F. Escoubet 《Cosmic Research》2006,44(3):202-208
A numerical model of an ion mass-spectrometer is developed based on the new type of charged-particle analyzer CAMERA suggested previously [1–3]. The spectrometer provides for complete instantaneous imaging of the flux distribution of various ions in a hemisphere. Such a type of the mass-spectrometer is chosen, which allows one to analyze a conelike beam of ions at the exit of the CAMERA. The mathematical model of the CAMERA with this time-of-flight mass-analyzer ensures sufficiently high mass resolution (M/ΔM > 100) at conserved imaging capabilities of the CAMERA. Such an instrument can find a wide application both in magnetospheric studies and in studying various objects of the solar system. 相似文献
1