Abstract

Optical observations of transient luminous events and remote-sensing of the lower ionosphere with low-frequency radio waves have demonstrated that thunderstorms and lightning can have substantial impacts in the nighttime ionospheric D region. However, it remains a challenge to quantify such effects in the daytime lower ionosphere. The wealth of electron density data acquired over the years by the Arecibo Observatory incoherent scatter radar (ISR) with high vertical spatial resolution (300-m in the present study), combined with its tropical location in a region of high lightning activity, indicate a potentially transformative pathway to address this issue. Through a systematic survey, we show that daytime sudden electron density changes registered by Arecibo’s ISR during thunderstorm times are on average different than the ones happening during fair weather conditions (driven by other external factors). These changes typically correspond to electron density depletions in the D and E region. The survey also shows that these disturbances are different than the ones associated with solar flares, which tend to have longer duration and most often correspond to an increase in the local electron density content.

Highlights

  • Sudden electron density changes coincident with solar flares most often produce ionization, while the ones coincident with lightning most often cause electron density depletions. Both types of sudden electron density changes have longer duration than the underlying fluctuations present in the data, but only in the case of electron density changes coincident with solar flares, the longer duration is significant

  • The cable failures started in the second semester of 2020, after years of wear and tear, and after having survived the damage from thunderstorms ­systems[26] like the ones studied in this paper

  • GLD360 did not discriminate between intracloud (IC) and CG lightning strikes

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Summary

Results

Within the 18,606 electron density profiles analyzed, we catalogued 212,045 sudden electron density changes, or spikes, amounting to an average of 1,030 per radar scan altitude level between 80 and 150 km in the daytime ionosphere We surprisingly find that the most significant difference in median relative magnitude between type II and III spikes happens in the E region

Summary and outlook
Spikes that are not coincident with either lightning or solar flares
Methods
Full Text
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