A model of the solar magnetic cycle with a meridian stream closed inside the convective zone A. G. Tlatov OriginalPaper Pages: 794 - 798
The influence of convection theories on the solar envelope structure and five-minute oscillation spectrum of the sun I. V. Mironova OriginalPaper Pages: 799 - 802
Solar models with a helioseismic sound speed profile S. V. AyukovV. A. Baturin OriginalPaper Pages: 803 - 806
From solar seismology to restrictions on the standard cosmology V. A. KotovS. V. Kotov OriginalPaper Pages: 807 - 810
The scattering effect ofp andg modes due to magnetic structure of solar spots and flares in the chromosphere V. V. KasinskyR. T. Sotnikova OriginalPaper Pages: 815 - 816
Solar radiant flux: Modern data and related problems E. A. MakarovaA. P. Sarychev OriginalPaper Pages: 820 - 824
Observed intensity of the solar continuum over the range 0.33–2.45 μm E. A. MakarovaE. M. RoshchinaA. P. Sarychev OriginalPaper Pages: 825 - 827
The color indices of the Sun in the infrared region A. V. KharitonovL. N. Knyazeva OriginalPaper Pages: 828 - 829
Hysteresis of a solar EUV flux and the relation of its characteristics to the solar cycle amplitude A. A. Nusinov OriginalPaper Pages: 830 - 832
A new data set for the absolute solar energy distribution in the 310–1070 nm wavelength region K. A. Burlov-Vasil'evI. E. Vasil'evaYu. B. Matveev OriginalPaper Pages: 833 - 837
IonosphericE region andE — F1 valley as indicators of solar radiant fluxes in the 10–30 nm wavelength region A. A. NusinovL. A. AntonovaV. V. Katyushina OriginalPaper Pages: 838 - 840
Stochastic resonance and detecting the 25-day periodicity in solar data M. M. Alibegov OriginalPaper Pages: 841 - 842
3D Modeling of the solar corona in different stages of the solar magnetic cycle over the period 1870 to 1991 V. I. MakarovA. G. TlatovM. P. Fatianov OriginalPaper Pages: 849 - 853
Coronal holes with a saddle structure as deduced from Yohkoh observations V. P. FilippovN. S. Shilova OriginalPaper Pages: 854 - 856
Magnetic field and doppler velocity correlation in quiescent solar prominences V. Yu. Klepikov OriginalPaper Pages: 857 - 861
Using color photometry to search for the solar corona “reddening” effect I. S. KimN. L. KroussanovaE. Picazzio OriginalPaper Pages: 862 - 864
Reducing the 3D equation to modulate galactic cosmic rays M. S. KalininM. B. Krainev OriginalPaper Pages: 865 - 868
The coronograph-polarimeter: An algorithm for creation of solar corona polarization images I. S. KimO. I. BougaenkoE. Picazzio OriginalPaper Pages: 869 - 873
Zero-level problem of solar magnetographs and observations of large-scale magnetic fields M. L. Demidov OriginalPaper Pages: 874 - 879
A bichromatic imaging method in solar studies V. M. GrigoryevN. I. Kobanov OriginalPaper Pages: 880 - 886
A Big Horizontal Solar Telescope of the Main Astronomical Observatory of the Ukrainian National Academy of Sciences in the caucasus K. A. Burlov-Vasil'evI. E. Vasil'evaYu. B. Matveev OriginalPaper Pages: 887 - 892
Display of helio-geomagnetic activity in circular transformations in the troposphere R. V. SmirnovE. V. Kononovich OriginalPaper Pages: 893 - 896
Some aspects of the solar cyclicity display in the lower atmosphere of the Earth R. V. SmirnovE. V. Kononovich OriginalPaper Pages: 897 - 900