Simultaneous 6300 Å airglow and radar observations of ionospheric irregularities and dynamics at the geomagnetic equator

• Published in: Annales geophysicae (1988) Vol. 36; no. 2; pp. 473 - 487
• Main Authors: Hickey, Dustin A, Martinis, Carlos R, Mendillo, Michael, Baumgardner, Jeffrey, Wroten, Joei, Milla, Marco
• Format: Journal Article
• Language: English
• Published: Katlenburg-Lindau Copernicus GmbH 22.03.2018; Copernicus Publications
• Subjects: Airglow; Airglow observations; Altitude; Depletion; Dynamics; Echoes; Equator; Equatorial ionosphere; Evolution; Geomagnetism; High altitude; Instruments; Interferometers; Ionosphere; Ionospheric irregularities; Irregularities; Latitude; Magnetic equator; Magnetic fields; Observatories; Plasma; Plasma drift; Plasma temperature; Plumes; Radar; Radar data; Separation; Spread F; Temperature; Temperature effects; Wind; Winds; Zonal winds
• ISSN: 1432-0576; 0992-7689; 1432-0576
• DOI: 10.5194/angeo-36-473-2018

In March 2014 an all-sky imager (ASI) was installed at the Jicamarca Radio Observatory (11.95∘ S, 76.87∘ W; 0.3∘ S MLAT). We present results of equatorial spread F (ESF) characteristics observed at Jicamarca and at low latitudes. Optical 6300 and 7774 Å airglow observations from the Jicamarca ASI are compared with other collocated instruments and with ASIs at El Leoncito, Argentina (31.8∘ S, 69.3∘ W; 19.8∘ S MLAT), and Villa de Leyva, Colombia (5.6∘ N, 73.52∘ W; 16.4∘ N MLAT). We use Jicamarca radar data, in incoherent and coherent modes, to obtain plasma parameters and detect echoes from irregularities. We find that ESF depletions tend to appear in groups with a group-to-group separation around 400–500 km and within-group separation around 50–100 km. We combine data from the three ASIs to investigate the conditions at Jicamarca that could lead to the development of high-altitude, or topside, plumes. We compare zonal winds, obtained from a Fabry–Pérot interferometer, with plasma drifts inferred from the zonal motion of plasma depletions. In addition to the ESF studies we also investigate the midnight temperature maximum and its effects at higher latitudes, visible as a brightness wave at El Leoncito. The ASI at Jicamarca along with collocated and low-latitude instruments provide a clear two-dimensional view of spatial and temporal evolution of ionospheric phenomena at equatorial and low latitudes that helps to explain the dynamics and evolution of equatorial ionospheric/thermospheric processes. Keywords. Ionosphere (equatorial ionosphere; ionospheric irregularities; plasma temperature and density)