The lunar exosphere is an ensemble of multiple overlapping, noninteracting neutral
distributions that reflect the primary physical processes acting on the lunar surface. While …

The solar inner corona is a region that plays a critical role in energizing the solar wind and
propelling it to supersonic and supra-Alfvénic velocities. Despite its importance, this region …

In the radio occultation (RO) experiments, the difference between observed and predicted
Doppler, called frequency residuals, form basic input data to retrieve the vertical profiles of …

Radio occultation (RO) measurement is an established technique for profiling planetary
atmosphere/ionosphere. The accuracy of the derived physical parameters (atmospheric …

We present observations of the Moon's plasma interaction in Earth's magnetotail lobes by
the ARTEMIS mission, and compare these to hybrid model results to constrain the global …

Abstract The Space Physics Laboratory (SPL) of Vikram Sarabhai Space Centre (VSSC) has
launched a science program called the Indian network for Space Weather Impact Monitoring …

Explore the development and state-of-the-art in deep space exploration using radio science
techniques In Radio Science Techniques for Deep Space Exploration, accomplished …

The image captured by SDO/AIA (Solar Dynamics Observatory) in the 193 Å ultraviolet
channel from 2022 October 25–27, unveiled a remarkable trio of dark coronal holes near the …

Abstract The Moon of our Earth has a tenuous atmosphere, known as an exosphere. The
ionization of this exosphere is speculated to possibly form a weak ionosphere. Some radio …

We present 'first of its kind'measurements of the enhanced integrated electron density
profiles (iEDPs) at the lunar wake and trans-terminator regions using radio occultation (RO) …