Odriozola, SS (reprint author), Natl Inst Space Res INPE, Av Astronautas 1758, BR-12227010 Sjc, SP, Brazil.
; Odriozola, SS (reprint author), IGA, Dept Space Geophys, Calle 212, Havana 2906, Cuba.
CNPQ agency [870480/1997-9, 140315/2014-4]
; CNPQ agency
; CAS Fellowship for Postdoctoral and Visiting Scholars [201377GB0001]
; CNPQ [312704/2015-1]
英文摘要:
A two-stage VS-30 Orion rocket was launched from the equatorial rocket launching station in Alcantara, Brazil, on 8 December 2012 soon after sunset (19:00 LT), carrying a Langmuir probe operating alternately in swept and constant bias modes. At the time of launch, ground equipment operated at equatorial stations showed rapid rise in the base of the F layer, indicating the pre-reversal enhancement of the F region vertical drift and creating ionospheric conditions favorable for the generation of plasma bubbles. Vertical profiles of electron density estimated from Langmuir probe data showed wave patterns and small-and medium-scale plasma irregularities in the valley region (100-300 km) during the rocket upleg and downleg. These irregularities resemble those detected by the very high frequency (VHF) radar installed at Jicamarca and so-called equatorial quasiperiodic echoes. We present evidence suggesting that these observations could be the first detection of this type of irregularity made by instruments onboard a rocket.
