Airglow observations over the equatorial ionization anomaly zone in Taiwan
نویسندگان
چکیده
Airglow imaging at mid-latitude stations often show intensity modulations associated with medium scale travelling ionospheric disturbances (MSTID), while those carried out near the equatorial regions reveal depletions caused by equatorial plasma bubbles (EPB). Two all sky cameras are used to observe plasma depletions in the 630.0 nm emission over the equatorial ionization anomaly (EIA) region, Taiwan (23 N, 121 E; 13.5 N Magnetic) during 1998–2002 and 2006–2007. The results show EPB and MSTID depletions in different solar activity conditions. Several new features of the EPB depletions such as bifurcation, secondary structure on the walls, westward tilt, etc., are discussed in this paper. Evidence of tilted depletions with secondary structures developing on the eastern wall that later evolve to appear as bifurcations, are presented for the first time. Moreover, detail investigations are carried out using International Reference Ionosphere (IRI) model as well as the electron density from Ionosonde and Global Positioning System (GPS) Occultation Experiment (GOX) onboard FORMOSAT-3/COSMIC satellite, to understand the conditions that favor the propagation of MSTID to the latitude of Taiwan.
منابع مشابه
Latitude dependence of zonal plasma drifts obtained from dual-site airglow observations
[1] All-sky imagers located at Tucumán, Argentina (26.9 S, 65 W, 14.2 S dip latitude), and Arequipa, Perú (16.5 S, 71.5 W, 2.7 S dip latitude), are used to track 630 nm airglow depletion motions in the first use of multisite airglow imagers for studies of low-latitude plasma dynamics. A new image analysis technique yields a consistent determination of nighttime zonal plasma drifts from all-sky ...
متن کاملIonospheric total electron content (TEC) studies with GPS in the equatorial region
This paper essentially deals with the effects of equatorial ionization anomaly gradient on space-based navigation systems like GPS. The equatorial region of the ionosphere, which extends about ±30dip about the magnetic equator, is characterized by a steep latitudinal gradient, not only in the maximum ionization but also in the total electron content (TEC), through a major part of the day. This ...
متن کاملVariability of ionospheric scintillation near the equatorial anomaly crest of the Indian zone
Multistation observations of ionosphere scintillation at VHF (250 MHz) and GNSS L1 frequency from three locations – (i) Bokkhali (BOK) (geographic 21.6 N, 88.2 E, dip 31.48), (ii) Raja Peary Mohan College Centre (RPMC) (geographic 22.66 N, 88.4 E, dip 33.5) and (iii) Krishnath College Centre (KNC), Berhampore (geographic 24.1 N, 88.3 E, dip 35.9) – at∼ 1 latitudinal separations near the norther...
متن کاملMulti-technique Studies of Ionospheric Plasma Structuring
The day-to-day variability in ionospheric irregularity generation giving rise to equatorial scintillation has remained an unresolved issue over many decades (Basu and Basu, 1985). We take a fresh look at the problem utilizing the global imagery provided by the GUVI instrument on NASA’s TIMED satellite. GUVI has been acquiring images of 135.6-nm emission in the Earth’s ionosphere/thermosphere sy...
متن کاملEffect of equatorial ionization anomaly on the occurrence of spread-F
The unique geometry of the geomagnetic field lines over the equatorial ionosphere coupled with the E– W electric field causes the equatorial ionization anomaly (EIA) and equatorial spread-F (ESF). Ionosonde data obtained at a chain of four stations covering equator to anomaly crest region (0.3 to 33 °N dip) in the Indian sector are used to study the role of EIA and the associated processes on t...
متن کامل