Anil Bhardwaj

TL;DR: The Advanced Telescope for High Energy Astrophysics (Athena+) mission as discussed by the authors provides the necessary performance (e.g., angular resolution, spectral resolution, survey grasp) to address these questions and revolutionize our understanding of the Hot and Energetic Universe.

TL;DR: High-spatial-resolution observations demonstrate that most of Jupiter's northern auroral X-rays come from a ‘hot spot’ located significantly poleward of the latitudes connected to the inner magnetosphere, invalidate the idea that jovian auroralX-ray emissions are mainly excited by steady precipitation of energetic heavy ions from the inner Magnetosphere.

TL;DR: In this paper, Chandra Advanced CCD Imaging Spectrometer (ACIS-S) observations of the Jovian auroral X-ray spectrum were carried out over 24-26 February 2003 by NASA's Advanced CCS-S instrument over 24 and 26 February 2003, and the results showed that the spectrum consists of line emission consistent with high-charge states of precipitating ions.

TL;DR: A review of the development of our current understanding of auroral emissions from Jupiter, Saturn, Uranus, and Neptune, as revealed through multispectral observations and supplemented by plasma measurements can be found in this paper.

TL;DR: In this paper, the authors present a review of the X-ray emission from the solar system bodies, excluding the Sun, and an overview of the main source mechanisms of Xray production at each object.