15 citations · 27 across the 5 of their papers we have counts for
5 papers
A comparison of G-band brightness as a proxy-magnetometer in various magnetic configurations
Malay Shukla, Sneha Pandit, Nitin Yadav
We investigate the diagnostic potential of the G-band at 430.4 nm for probing small-scale magnetic fields in the solar photosphere. Combining three-dimensional MHD simulations from…
EMISSA: Exploring millimetre indicators of solar-stellar activity III. Comparison of Ca II indices and millimetre continua in a 3D model atmosphere
Sneha Pandit, Sven Wedemeyer, Mats Carlsson
The Ca II H & K lines are strong chromospheric diagnostics that can be used to determine the temperature stratification and magnetic structure of the solar atmosphere. The Atacama…
Comparison of chromospheric diagnostics in a 3D model atmosphere: H linewidth and mm continua
Sneha Pandit, Sven Wedemeyer, Mats Carlsson +1
The Ha line, one of the most studied chromospheric diagnostics, is a tracer for magnetic field structures, while its line core intensity provides an estimate of the mass density. T…
EMISSA -- Exploring Millimetre Indicators of Solar-Stellar Activity II. Towards a robust indicator of stellar activity
Atul Mohan, Sven Wedemeyer, Peter H. Hauschildt +2
An activity indicator, which can provide a robust quantitative mapping between the stellar activity and the physical properties of its atmosphere, is important in exploring the phy…
EMISSA -- Exploring Millimeter Indicators of Solar-Stellar Activity I. The Initial mm-cm Main Sequence Star Sample
Atul Mohan, Sven Wedemeyer, Sneha Pandit +2
Due to their wide wavelength coverage across the millimetre to centimetre (mm - cm) range and their increased sensitivity, modern interferometric arrays facilitate observations of…