2. DOK-2 Results Page
... Fig.2 and Fig.3 show series of successive spectra for electron telescopes which exhibit space-energy dispersion of electrons ... Fig.1 . Fig.2 . Fig.3 . Fig.4 . Fig.6 . ...
4. ENERGETIC PARTICLE EXPERIMENT DOK-2
... Fig. 1 and 2. give examples of DOK-2 responce by a passage of some magnetic structures in the geotail where magnetic field ... In Fig. 2. the amplitude of the spin modulation is different for different energies. ...
5. http://www.gao.spb.ru/english/as/j2014/presentations/lipovka.pdf
... 6 Fig 7 1 2 3 RA m 01 -03 -02 8 s 09.3 22.2 32.4 DEC 9 Name 10 HD2438 HD2154 zet Cyg Fig 11 1a 2a 3a Fig 2 Fig 2 -27 25.0 +21 47.0 +38 39.4 Conclusions: Developed method of matching radio sky with optical objects, showed that the bright radio sources are ...
6. http://www.issp.ac.ru/lek/murzin/art36E.pdf
... 1) The experimental data are compared with Eq. (2) in Fig. 1 where we plotted the ... The regular arrangement of the points in Fig. 2 calls for a new explanation of the ... REFERENCES m Fig. 2. xx(1/2)n2 versus the spacer thickness d. The gles are the ...
7. http://lav01.sinp.msu.ru/~vlk/pbarp_mypreprint.ps
... ъ \Upsilon + ъ 0 (1) can be described in Regge pole model [2] by diagram in Fig. 1. ... p + ъ \Gamma (2) is descibed by the diagram in Fig.2. ... ъ + + ъ \Gamma (3) 1 D 0 ,N 0 p ґ p p p ґ Fig.2. ...
8. Space monitoring data center
... On the Fig. 2 the Oxygen fluences and the corresponding energy spectra for the SEP event from 8 Nov. 2000 are demonstrated. ... Fig.2. Measured by SIS ACE oxygen fluences for Nov. ...
9. http://hit-conf.imec.msu.ru/2006/Template.doc
... first, second and third modes (m = 1,2 and 3), respectively. [pic] Figure 2 Instability boundary in spectral space We can see from fig.1 and fig.2 that suggested We can see from fig.1 and fig.2 that suggested We can We can see from fig.1 and fig.2 that ...
10. Single
... Such materials have been identified (see Fig.2 ). a) . b) . Fig. 2 . ... the sensor material Au +100 ppm Fe (see Fig.2, a) was used, which is not as good as ... Fig.2, a and b ), though it could produce D E FWHM ~ 20 eV at 0.3K. Our best results ...