22 citations · 86 across the 8 of their papers we have counts for
9 papers
Coronal Elemental Abundances during A-class Solar Flares Observed by Chandrayaan-2 XSM
Lakshitha Nama, Biswajit Mondal, S Narendranath +1
The abundances of low First Ionisation Potential (FIP) elements are three to four times higher (FIP bias) in the closed loop active corona than in the photosphere, known as the FIP…
Science with the Daksha High Energy Transients Mission
Varun Bhalerao, Disha Sawant, Archana Pai +72
We present the science case for the proposed Daksha high energy transients mission. Daksha will comprise of two satellites covering the entire sky from 1~keV to ~MeV. The prima…
Evolution of Elemental Abundances During B-Class Solar Flares: Soft X-ray Spectral Measurements with Chandrayaan-2 XSM
Biswajit Mondal, Aveek Sarkar, Santosh V. Vadawale +6
The Solar X-ray Spectrometer (XSM) payload onboard Chandrayaan-2 provides disk-integrated solar spectra in the 1-15 keV energy range with an energy resolution of 180 eV (at 5.9 keV…
Lunar Volatiles and Solar System Science
Parvathy Prem, Ákos Kereszturi, Ariel N. Deutsch +38
Understanding the origin and evolution of the lunar volatile system is not only compelling lunar science, but also fundamental Solar System science. This white paper (submitted to…
Coronal Elemental Abundance: New Results from Soft X-ray Spectroscopy of the Sun
S. Narendranath, P. Sreekumar, Netra S Pillai +3
Elemental abundances in the solar corona are known to be different from those observed in the solar photosphere. The ratio of coronal to photospheric abundance shows a dependence o…
Simulating charge transport to understand the spectral response of Swept Charge Devices
P. S. Athiray, P. Sreekumar, S. Narendranath +1
Swept Charge Devices (SCD) are novel X-ray detectors optimized for improved spectral performance without any demand for active cooling. The Chandrayaan-1 X-ray Spectrometer (C1XS)…