2011 FEBRUARY 15 CME IN THE INTERPLANETARY MEDIUM BY OBSERVATIONS OF RADIO SOURCE SCINTILLATIONS AT THE DECAMETER WAVELENGTHS
Abstract
The high efficiency of the interplanetary scintillation method
at the decameter wavelengths for detection of coronal mass ejections
beyond Earth’s orbit is shown. It is established that coronal
mass ejection in the interplanetary medium continues
slowing at distances from 1 to 1.7 AU from the Sun, its velocity
tending to that of the ambient solar wind, the angular size being
no less than 66°.
at the decameter wavelengths for detection of coronal mass ejections
beyond Earth’s orbit is shown. It is established that coronal
mass ejection in the interplanetary medium continues
slowing at distances from 1 to 1.7 AU from the Sun, its velocity
tending to that of the ambient solar wind, the angular size being
no less than 66°.
Full Text:
PDFReferences
Калиниченко Н. Н. Корональный выброс массы 15 февраля 2011 г. в межпланетном пространстве и его наблюдения методом мерцаний космических источников в декаметровом диапазоне радиоволн / Н. Н. Калиниченко, А. А. Коноваленко, А. И. Браженко, В. В. Соловьев // Радиофизика и радиоастрономия. — 2013. — Т. 18, № 4. — С. 301-308.
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)