Center for Radio Astronomy and Astrophysics at Mackenzie

CRAAM

Instrumental Collection

Ionosphere

The ionosonde is radar that emits vertically signals in the 1 to 20 MHz frequency range, which are reflected in the ionosphere. The analysis of the signals of different frequencies transmitted and received by the system gives the vertical electron density profile. The ionosonde we operate at Brazilian Antarctic Station EACF is a ‘Canadian Advanced Digital Ionosonde’ (CADI). It operates simultaneously in two distinct modes, the first one transmits six frequencies (between 3 and 8 MHz) at each 200 seconds, and the second one transmits 80 frequencies at each 300 seconds (scanning from 1 to 20 MHz in a logaritmic scale) [Macdougall et al. 1995]. The CADI operation to at EACF started on 2009.

The main objectives of the continuous monitoring of the Global Atmospheric Electric Circuit (GAEC) are: (i) obtaining Carnegie curves and evolution in function of the season, the solar activity cycle, the presence of solar and geomagnetic disturbances; (ii) relationship with seismic activity on the Pacific coast of Peru.

The AFINSA network (Atmospheric Electric Field Network in South America) is composed of 8 sensors installed in Brazil, Argentina and Peru. Therefore, continuous measurements of the atmospheric electric field are recorded at various locations in South America. The already existing locations are: CAS (2 sensors named CAS and SAV at El Leoncito, San Juan, Argentina), PLO (1 sensor Punta Lobos, Lima, Peru), ICA (1 sensor Ica, Peru), HYO (1 sensor Huancayo, Peru), CGR (1 sensor Paraiba, Brazil), ROR (1 sensor Roraima, Brazil), and MACK (1 sensor São Paulo, Brazil). are shown as triangles in the figure. New stations (stars) are planned for beginning of operation in 2017.

Each sensor consists of a commercially manufactured (Boltek Corporation EFM100-1000120-050205) electric field mill (EFM). The minimum overall sensitivity range is ±20 kV/m and can be improved up to 40 kV/m. The response time of each sensor is 0.1 s. The basic principle of operation of the EFM stands on the fundamental laws of electromagnetism. When a conducting plate is exposed to an electric field, a charge is induced proportional to the electric field intensity and the area of the plate. The EFM produces alternate electrical fields by using an array of electrodes and rotor driven by motor.

The network is operated by CRAAM (Brazil) in collaboration with other institutions: CASLEO(Argentina), ICATE (Argentina), CONIDA (Peru). One of our first task will be to provide AFINSA data access in the form of monthly means of the fair-weather AEF.

Riometers are systems that detect the cosmic noise in the 20 and 30 MHz frequency range, which strongest source is the galactic center. The radiation at this frequency range could be absorbed while crossing the ionosphere when its condition is disturbed by the increase of radiation due solar explosions or by the impact of energetic particles. Thus, riometer can be used to monitor the ionospheric conditions. The riometer observations at EACF started on 2009, and at ROI on 2008.