Fig. 2 Synoptic maps showing the varying properties of the corona and photosphere over a whole solar rotation. Synoptic maps showing the varying properties.

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Presentation transcript:

Fig. 2 Synoptic maps showing the varying properties of the corona and photosphere over a whole solar rotation. Synoptic maps showing the varying properties of the corona and photosphere over a whole solar rotation. Shown here are (A) mean temperature, (B) EM, and (C) radial magnetic field component for a whole solar rotation during 04 March 2011. The y axis shows latitude on the solar disk, on a sine latitude scaling. The two horizontal dotted lines indicate the latitudinal range within ±40° of the equator (areas outside are not included for further study). Areas defined as active regions are shown within unbroken contours. Areas outside the dashed contours are considered as quiet corona. See Methods for more details on the identification of regions. Huw Morgan, and Youra Taroyan Sci Adv 2017;3:e1602056 Copyright © 2017 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution License 4.0 (CC BY).