共 12 条
[2]
A manifestation of magnetic fluxes in microwave emission of the solar corona.[J].B.V. Agalakov;B.I. Lubyshev;D.V. Prosovetsky;G.V. Rudenko;G.Ya. Smolkov;A.M. Uralov.Cospar.2002,
[3]
Observations of bright coronal points at wavelengths of 5.2 and 1.76 cm
[J].
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS,
2001, 27 (03)
:181-185
[4]
Microwave signatures of solar flare buildup
[J].
SPACE WEATHER: PHYSICS AND APPLICATIONS,
2000, 26 (01)
:193-196
[8]
Stepwise Emergence and Development of Microwave Emission of Active Regions – A Fundamental Property of Active Solar Corona.[J].G. Ya. Smolkov;V. P. Nefedyev;A. M. Uralov;N. N. Kardapolova.International Astronomical Union Colloquium.1994,
[9]
Two-dimensional solar mapping at 5.2 cm with the Siberian Solar Radio Telescope.[J].C. E. Alissandrakis;B. I. Lubyshev;G. Ya. Smolkov;B. B. Krissinel;T. A. Treskov;V. G. Miller;N. N. Kardapolova.Solar Physics.1992, 2