Irmgard Jernej

TL;DR: To achieve mission objectives, the calibration determined on the ground will be refined in space to ensure all eight magnetometers are precisely inter-calibrated, and the information flow that provides the data on the rapid time scale needed for mission success is described.

TL;DR: The temperature and density profiles, as determined by the Huygens Atmospheric Structure Instrument (HASI), from an altitude of 1,400 km down to the surface were higher than expected and the extent of atmospheric electricity was also hitherto unknown.

TL;DR: The permittivity, waves and altimetry (PWA) instrument was designed for the investigation of the electric properties and other related physical characteristics of the atmosphere of Titan, from an altitude around 140 km down to the surface.

TL;DR: In this article, a detailed analysis of both data sets is required, in order to correct for environmental effects and compare the two independent estimates of the electrical conductivity, and the existence of a prominent ionized layer, and enhancements in the conductivity and electron density profiles at 63 km, are discussed in the light of previous theoretical predictions.

TL;DR: In this paper, the authors presented the altitude distribution of the concentration of positive ions and electrons obtained from the RP and MI sensors, which were made from 140 to 40 km and show a maximum of charge densities ≈2 × 109 m−3 positive ions, and ≈450 × 106 m− 3 electrons at around 65 km.