Articles | Volume 10, issue 2
https://doi.org/10.5194/hgss-10-245-2019
https://doi.org/10.5194/hgss-10-245-2019
Review article
 | 
02 Oct 2019
Review article |  | 02 Oct 2019

The early history of the Jicamarca Radio Observatory and the incoherent scatter technique

Ronald F. Woodman, Donald T. Farley, Ben B. Balsley, and Marco A. Milla

Related authors

Simultaneous ground-based and in situ Swarm observations of equatorial F-region irregularities over Jicamarca
Sharon Aol, Stephan Buchert, Edward Jurua, and Marco Milla
Ann. Geophys., 38, 1063–1080, https://doi.org/10.5194/angeo-38-1063-2020,https://doi.org/10.5194/angeo-38-1063-2020, 2020
Short summary
Simultaneous 6300 Å airglow and radar observations of ionospheric irregularities and dynamics at the geomagnetic equator
Dustin A. Hickey, Carlos R. Martinis, Michael Mendillo, Jeffrey Baumgardner, Joei Wroten, and Marco Milla
Ann. Geophys., 36, 473–487, https://doi.org/10.5194/angeo-36-473-2018,https://doi.org/10.5194/angeo-36-473-2018, 2018
Short summary
Simultaneous observations of structure function parameter of refractive index using a high-resolution radar and the DataHawk small airborne measurement system
Danny E. Scipión, Dale A. Lawrence, Marco A. Milla, Ronald F. Woodman, Diego A. Lume, and Ben B. Balsley
Ann. Geophys., 34, 767–780, https://doi.org/10.5194/angeo-34-767-2016,https://doi.org/10.5194/angeo-34-767-2016, 2016
Short summary
Equatorial 150 km echoes and daytime F region vertical plasma drifts in the Brazilian longitude sector
F. S. Rodrigues, E. B. Shume, E. R. de Paula, and M. Milla
Ann. Geophys., 31, 1867–1876, https://doi.org/10.5194/angeo-31-1867-2013,https://doi.org/10.5194/angeo-31-1867-2013, 2013
Download
Short summary
The Jicamarca Radio Observatory is a research facility of the Geophysical Institute of Peru, located near the city of Lima, that has been conducting observations and studies of the equatorial ionosphere for more than 50 years. In these notes we focus to the period of its construction and roughly the first decade of its operation (1960–1974). We emphasize observational and instrumental developments that shaped the capabilities of one of the most powerful incoherent scatter radars in the world.