Postmidnight equatorial plasma irregularities on the June solstice during low solar activity - A case study

Claudia M.N. Candido, Jiankui Shi, Inez S. Batista, Fabio Becker-Guedes, Emília Correia, Mangalathayil A. Abdu, Jonathan Makela, Nanan Balan, Narayan Chapagain, Chi Wang, Zhengkuan Liu

Research output: Contribution to journalArticlepeer-review

Abstract

We present a case study of unusual spread-F structures observed by ionosondes at two equatorial and low-latitude Brazilian stations - São Luís (SL: 44.2° W, 2.33° S; dip angle: -6:9°) and Fortaleza (FZ: 38.45° W, 3.9° S; dip angle: -16°). The irregularity structures observed from midnight to postmidnight hours of moderate solar activity (F10.7<97 sfu, where 1 sfu=10-22Wm-2 s-1) have characteristics different from typical post-sunset equatorial spread F. The spread-F traces first appeared at or above the Flayer peak and gradually became well-formed mixed spread F. They also appeared as plasma depletions in the 630.0 nm airglow emissions made by a wide-angle imager located at the nearby low-latitude station Cajazeiras (CZ: 38.56° W, 6.87° S; dip angle: -21:4°). The irregularities appeared first over FZ and later over SL, giving evidence of an unusual westward propagation or a horizontal plasma advection. The drift-mode operation available in one of the ionosondes (a digital portable sounder, DPS-4) has enabled us to analyze the horizontal drift velocities and directions of the irregularity movement. We also analyzed the neutral wind velocity measured by a Fabry-Pérot interferometer (FPI) installed at CZ and discuss its possible role in the development of the irregularities.

Original languageEnglish (US)
Pages (from-to)657-672
Number of pages16
JournalAnnales Geophysicae
Volume37
Issue number4
DOIs
StatePublished - Jul 30 2019

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Geology
  • Atmospheric Science
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science

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