Coronal/interplanetary disturbances associated with disappearing solar filaments

Astronomy and Astrophysics – Astronomy

Scientific paper

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Interplanetary Medium, Magnetohydrodynamic Stability, Solar Corona, Solar Prominences, Solar Wind, Spaceborne Astronomy, H Alpha Line, Japanese Spacecraft, Solar Limb, Solar X-Rays

Scientific paper

Two examples of coronal events associated with two erupting-filament events observed from different angles are discussed. These are coronal/interplanetary disturbances associated with the disappearance of a 35-deg-long quiescent filament occurring near the solar disk center, observed on September 28, 1991, and with a 25 deg long eruptive prominence at the eastern solar limb, which took place on November 7, 1991. In both cases, bright soft X-ray arcades were observed with the Yohkoh Soft X-ray Telescope about 2-3 hr after the onset of H-alpha events. A transient coronal hole was formed in the immediate vicinity of the disappearing filament on Septemper 28, suggesting that the formation of the new coronal hole was a cause of the filament disappearance.

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