The solar wind disappearance event of 11 May 1999: source region evolution
P. Janardhan, D. Tripathi, and H.E. Mason

TL;DR
This study investigates the evolution of a coronal hole and active region complex before a solar wind disappearance event on 11 May 1999, revealing dynamic boundary changes and flux emergence linked to space weather effects.
Contribution
It provides the first detailed analysis of the source region evolution leading to a solar wind disappearance event without associated CMEs, highlighting the role of boundary dynamics and flux emergence.
Findings
Dynamic evolution of CH-AR boundary observed.
Reduction in coronal hole area prior to event.
Emerging flux regions correlated with new loop formation.
Abstract
Context. A recent, detailed study of the well-known solar wind disappearance event of 11 May 1999 traced its origin to a coronal hole (CH) lying adjacent to a large active region (AR), AR8525 in Carrington rotation 1949. The AR was located at central meridian on 05 May 1999 when the flows responsible for this event began. We examine the evolution of the AR-CH complex during 5-6 May 1999 to study the changes that apparently played a key role in causing this disappearance event. Aims. To study the evolution of the solar source region of the disappearance event of 11 May 1999. Methods. Using images from the Soft X-ray Telescope (SXT), the Extreme-ultraviolet Imaging Telescope (EIT) and the Michelson Doppler Imager (MDI) to examine the evolution of the CH and AR complex at the source region of the disappearance event. Results. We find a dynamic evolution taking place in the CH-AR boundary…
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