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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 7.

Quasiperiodic pulsations and magnetoseismology during the high-confidence portion of Window 3 selected by I > 5 × 103 sfu and V/I < −0.8 (Section 2.3). (a), (c), (e) Stokes I residuals ﹩{I}_{{\rm{res}}}(t)﹩ after subtracting a 256 minutes running-median trend; the red curve is a smoothed envelope highlighting the oscillations. (b), (d), (f) Lomb–Scargle periodograms of ﹩{I}_{{\rm{res}}}(t)﹩ computed from the residual time series shown in panels (a), (c), (e) show dominant periods P of 57.1, 50.3, and 44.8 minutes at 975, 1475, and 1925 kHz (vertical dashed lines). Dashed horizontal lines indicate the 95% false-alarm level. Periodograms are evaluated over periods of 5–60 minutes (the plotted range). (g) Panel (g) explicitly shows how the measured period P maps, through the adopted vA(r) model, to the lower bound ﹩{W}_{{\rm{A}},{\rm{\min }}}﹩ and hence to the minimum half-width ﹩{a}_{{\rm{\min }}}\equiv {W}_{{\rm{A}},{\rm{\min }}}/2﹩.

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