Largest Radar In Antarctica Measures Earth’s Ionosphere For The First Time

Eddie Gonzales Jr. – MessageToEagle.com – Researchers have used radar in Antarctica to make the first measurements from the Antarctic region.

The ionosphere – about 60 to 600 miles above Earth’s surface – is blasted by solar radiation that breaks down the bonds of ions. Free electrons and heavy ions are left behind, constantly colliding.

The Program of the Antarctic Syowa Mesosphere-Stratosphere-Troposphere/Incoherent Scatter radar (PANSY radar) consisting of an active phased array of 1045 Yagi antennas. CREDIT Taishi Hashimoto (NIPR)Antarctic Syowa radar(PANSY), the first Mesosphere–Stratosphere–Troposphere/Incoherent Scatter (MST/IS) radar consisting of an active phased array of 1045 Yagi antennas. Photo: Taishi Hashimoto (NIPR)

These activities were previously measured through a method called incoherent scatter radar in the northern hemisphere, where researchers beam radio wave into the ionosphere. The electrons in the atmosphere scatter the radio wave “incoherently”. The different ways they scatter tell researchers about the particles populating the layer.

Researchers published their preliminary results on September 17, 2019, in the Journal of Atmospheric and Oceanic Technology.

“Incoherent scatter radar is currently the most powerful tool available to investigate the ionosphere because it covers a wide altitudinal range and it observes essential ionospheric parameters such as electron density, ion velocity, ion, and electron temperatures, as well as ion compositions,” Taishi Hashimoto, assistant professor at the National Institute of Polar Research in Japan, said in a press release.

While these radars are powerful, they’re also rare due to their size and power demand.

Using the Program of the Antarctic Syowa Mesosphere-Stratosphere-Troposphere/Incoherent Scatter (PANSY) radar, the largest and fine-resolution atmospheric radar in the Antarctic, researchers performed the first incoherent scatter radar observations in the southern hemisphere in 2015, the first 24-hour observation was made in 2017.

While analyzing these observations, Hashimoto and the team expected to see significant differences between the southern measurements and the northern measurements, as Earth’s lower atmosphere has a strong asymmetry between hemispheres.

According to Hashimoto, observations in the southern hemisphere are crucial to revealing global features of both the atmosphere and the ionosphere.

“Our next step will be the simultaneous observation of ionosphere incoherent scatter and field-aligned irregularities since the suppression and extraction are using the same principle from different aspects,” Hashimoto said. “We are also planning to apply the same technique to obtain other types of plasma parameters, such as the drive velocity and ion temperature, leading to a better understanding of auroras,” Hashimoto added.

Written by Eddie Gonzales Jr. – MessageToEagle.com Staff