# Search results

New Astronomy > 1998 > 3 > 5 > 335-346

_{α}flares (including remarks on proton event association), and on solar radio...

New Astronomy > 1998 > 3 > 5 > 321-334

Chinese Astronomy and Astrophysics > 2013 > 37 > 2 > 149-162

Advances in Space Research > 2015 > 55 > 3 > 886-890

Advances in Space Research > 2013 > 52 > 12 > 2122-2131

_{α}filaments and the long-lived magnetic features of negative and positive polarities. Analysis of the data showed that: (a) there is N–S asymmetry in the equatorial rotation of the H

_{α}filaments and the long-lived magnetic features; (b) for both solar cycles the long-lived...

Chinese Astronomy and Astrophysics > 2012 > 36 > 1 > 49-62

Chinese Astronomy and Astrophysics > 2004 > 28 > 3 > 323-330

Chinese Science Bulletin > 1998 > 43 > 23 > 1969-1973

_{α}surge event. To our knowledge, no H

_{α}surge event coincident with the large scale coronal brightening observed...

Risk Analysis > 40 > 5 > 1020 - 1039

Astronomy Letters > 2019 > 45 > 9 > 627-634

Astrophysics and Space Science > 2019 > 364 > 11 > 1-13

*eruptive latitude*”. The eruptive...

Solar Physics > 2019 > 294 > 9 > 1-14

*Large-Angle Spectrometric Coronagraph*(LASCO) field of view (FOV). To detect the first moment of the shock onset, we found a CME on 17 July 2012 that formed at a relatively high altitude and moved with slow acceleration. We examined the possible mechanisms of shock generation. It was shown that bow-shock and piston-shock mechanisms can participate...

Astronomy Letters > 2019 > 45 > 6 > 396-401

Journal of Biological Engineering > 2019 > 13 > 1 > 1-12

Astrophysics and Space Science > 2019 > 364 > 7 > 1-7

Kinematics and Physics of Celestial Bodies > 2019 > 35 > 3 > 105-123

Space Science Reviews > 2019 > 215 > 5 > 1-129

Journal of Fixed Point Theory and Applications > 2019 > 21 > 3 > 1-11

*M*. A set

*M*is called a local $$\max $$ max -sun at a point $$x_0$$ x0 if there is a farthest point $$\widehat{y}\in {\mathrm {F}}_Mx_0$$ y^∈FMx0 and a number $$\delta >0$$ δ>0 such that $$ \widehat{y} \in {\mathrm {F}}_Mx$$ y^∈FMx for any point $$x\in \bigl [x_0, x_0+\delta...

Astronomy Letters > 2019 > 45 > 4 > 237-247

Astrophysical Bulletin > 2019 > 74 > 2 > 221-233