We present a one-dimensional coupled ion-neutral photochemical kinetics and diffusion
model to study the atmospheric composition of Titan in light of new theoretical kinetics …

Since the arrival of the Cassini spacecraft at Saturn in July 2004, newly collected plasma
and magnetic field data have greatly expanded our knowledge on the interaction between …

We examine the dynamics of energetic magnetospheric electrons exposed to the highly
perturbed and asymmetric plasma environment of Jupiter's moon Callisto. The interaction of …

Blazars are classified into high-, intermediate-and low-energy-peaked sources based on the
location of their synchrotron peak. This lies in infra-red/optical to ultra-violet bands for low …

Temperature profiles derived from Cassini Ion Neutral Mass Spectrometer data in Paper I
show that the thermal structure of Titan's upper atmosphere is extremely variable. The …

Abstract Effects of solar EUV on positive ions and heavy negative charge carriers (molecular
ions, aerosol, and/or dust) in Titan's ionosphere are studied over the course of almost 12 …

Titan's ionosphere is created when solar photons, energetic magnetospheric electrons or
ions, and cosmic rays ionize the neutral atmosphere. Electron densities generated by …

Based on a multi-instrumental Cassini dataset we make model versus observation
comparisons of plasma number densities, n P=(nen I) 1/2 (ne and n I being the electron …

Analysis of the Cassini Ion Neutral Mass Spectrometer data reveals the omnipresence of
density waves in various constituents of Titan's upper atmosphere, with quasi‐periodical …

We have studied the effects of ion-neutral collisions on Titan׳ s interaction with the
magnetospheric plasma flow and also on the Alfvén wings formed in this super-Alfvénic …