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Study of Coronal Rotation using X-ray images observed by Hinode

Published online by Cambridge University Press:  27 November 2018

Satish Chandra ,
Vivek Kumar Singh  and
Sanish Thomas
Satish Chandra
Affiliation:
Dept. of Physics, P P N P G College, Kanpur, India email: satish0402@gmail.com
Vivek Kumar Singh
Affiliation:
Dept. of Physics, SHUATS, Allahabad, India
Sanish Thomas
Affiliation:
Dept. of Physics, SHUATS, Allahabad, India
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Abstract

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Solar rotation is still one of the unresolved concern of solar physics. We performed time series analysis on the bins formed on equally separated latitude regions on the soft X-ray images. These images are observed with the X-ray telescope (XRT) on board the Hinode satellite. The flux modulation method traces the passage of X-ray feature over the solar disc and statistical analysis of the time series data of the SXR images (one per day) for the period extends from year 2015 to 2017 gives the coronal rotation period as a function of latitude. The investigation provided quite systematic information of the solar rotation and its variability.

Keywords

Sun: activitySun: coronaSun: rotationSun: X-rays
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S340: Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles , February 2018 , pp. 179 - 180
Copyright
Copyright © International Astronomical Union 2018 

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