activity
20032022
most citedThe Prelude to the Deep Minimum between Solar Cycles 23 and 24: Interplanetary Scintillation Signatures in the Inner Heliosphere

140 citations · 736 across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.SR2022★ 14 cited

Soft X-ray Spectral Diagnostics of Multi-thermal Plasma in Solar Flares with Chandrayaan-2 XSM

N. P. S. Mithun, Santosh V. Vadawale, Giulio Del Zanna +7

Spectroscopic observations in X-ray wavelengths provide excellent diagnostics of the temperature distribution in solar flare plasma. The Solar X-ray Monitor (XSM) onboard the Chand…

astro-ph.SR2022★ 13 cited

Multi-wavelength observations by XSM, Hinode and SDO of an active region. Chemical abundances and temperatures

G. Del Zanna, B. Mondal, Y. K. Rao +7

We have reviewed the first year of observations of the Solar X-ray Monitor (XSM) onboard Chandrayaan-2, and the available multi-wavelength observations to complement the XSM data,…

astro-ph.SR2021

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…

astro-ph.SR2021★ 26 cited

Observations of the Quiet Sun During the Deepest Solar Minimum of the Past Century with Chandrayaan-2 XSM -- Sub-A Class Microflares Outside Active Regions

Santosh V. Vadawale, N. P. S. Mithun, Biswajit Mondal +12

Solar flares, with energies ranging over several orders of magnitude, result from impulsive release of energy due to magnetic reconnection in the corona. Barring a handful, almost…

astro-ph.SR2021★ 20 cited

Observations of the Quiet Sun During the Deepest Solar Minimum of the Past Century with Chandrayaan-2 XSM -- Elemental Abundances in the Quiescent Corona

Santosh V. Vadawale, Biswajit Mondal, N. P. S. Mithun +12

Elements with low First Ionization Potential (FIP) are known to be three to four times more abundant in active region loops of the solar corona than in the photosphere. There have…

astro-ph.SR2020★ 40 cited

Solar X-ray Monitor On Board the Chandrayaan-2 Orbiter: In-flight Performance and Science Prospects

N. P. S. Mithun, Santosh V. Vadawale, Aveek Sarkar +14

The Solar X-ray Monitor (abbreviated as XSM) on board India's Chandrayaan-2 mission is designed to carry out broadband spectroscopy of the Sun from lunar orbit. It observes the Sun…