22 citations · 86 across the 8 of their papers we have counts for
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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…
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…
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…