Figure 9 from Quantifying the Propagation of Fast Coronal Mass Ejections from the Sun to Interplanetary Space by Combining Remote Sensing and Multi-point In Situ Observations

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Quantifying the Propagation of Fast Coronal Mass Ejections from the Sun to Interplanetary Space by Combining Remote Sensing and Multi-point In Situ Observations

Authors: Xiaowei Zhao, Ying D. Liu, Huidong Hu, and Rui Wang

2019 The Astrophysical Journal 882 122.

Provider: AAS Journals

Caption: Figure 9.

Similar to Figure 4, but for the dynamic spectrum associated with the 2000 June 6 CME. The white arrows indicate the observed type II radio bands. The pink quadrilateral shows a special region, covering frequencies from about 40 to 130 kHz and times from about 13:26 UT on June 7 to 04:25 UT on June 8.

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