Abstract
A distinct (or ‘gorgeous’) coronal hole was observed from October to December, 2000, at around 180° in Carrington longitude. Its formation, evolution, and rotation rates are discussed based on an analysis of Yohkoh Soft X-ray Telescope (SXT) images and synoptic maps of the Kitt Peak magnetic field.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
