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Unprecedented 19 Day Type IV Radio Burst as a Corotating Electron Reservoir

  • Authors: Vratislav Krupar, Oksana Kruparova, Adam Szabo, Lynn B. Wilson, Lan K. Jian, David Lario, Teresa Nieves-Chinchilla, Andreas J. Weiss, Anthony Iampietro, Hamish A. S. Reid, Lucie M. Green, Eduard P. Kontar, Rui F. Pinto, Keith Goetz

Vratislav Krupar et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 8.

White-light context. Coronagraph images spanning the STEREO-A interval with wavevector-corrected direction-finding angles overplotted as angular positions (circles: blue 975 kHz, green 1475 kHz, red 1925 kHz). The corrected directions remain near the helmet streamer apex as the system rotates across the visible hemisphere; these points indicate directions on the sky and are not an independent 3D reconstruction, so their projected distance from the occulter is not a direct proxy for heliocentric source height. An animation of this figure is available. It shows the sequence from 2025 September 6 at 11:53:30 to 2025 September 9 at 11:53:30. The real-time duration is 18 s.

(An animation of this figure is available in the online article.)

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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