activity
20192021
most citedSolar-type Stars Observed by LAMOST and Kepler

20 citations · 56 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.SR202120 cited

Predictions of Astrometric Jitter for Sun-like Stars. II. Dependence on Inclination, Metallicity, and Active-Region Nesting

K. Sowmya, N. -E. Nèmec, A. I. Shapiro +5

Ultra-precise astrometry from the Gaia mission is expected to lead to astrometric detections of more than 20,000 exoplanets in our Galaxy. One of the factors that could hamper such…

astro-ph.SR2021

Modeling stellar Ca II H & K emission variations. I. Effect of inclination on the S-index

K. Sowmya, A. I. Shapiro, V. Witzke +5

The emission in the near ultraviolet Ca II H & K lines is modulated by stellar magnetic activity. Although this emission, quantified via the S-index, has been serving as a prime pr…

astro-ph.SR20206 cited

Importance of Angle-dependent Partial Frequency Redistribution in Hyperfine Structure Transitions Under Incomplete Paschen-Back Effect Regime

K. N. Nagendra, K. Sowmya, M. Sampoorna +2

Angle-frequency coupling in scattering of polarized light on atoms is represented by the angle-dependent (AD) partial frequency redistribution (PRD) matrices. There are several lin…

astro-ph.SR202020 cited

Solar-type Stars Observed by LAMOST and Kepler

Jinghua Zhang, Alexander I. Shapiro, Shaolan Bi +8

Obtaining measurements of chromospheric and photometric activity of stars with near-solar fundamental parameters and rotation periods is important for a better understanding of sol…

astro-ph.SR2019

Fast downflows in a chromospheric filament

K. Sowmya, A. Lagg, S. K. Solanki +1

An active region filament in the upper chromosphere is studied using spectropolarimetric data in He I 10830 A from the GREGOR telescope. A Milne-Eddingon based inversion of the Unn…

astro-ph.SR201910 cited

Polarized Line Formation in Arbitrary Strength Magnetic Fields: the case of a two-level atom with hyperfine structure splitting

M. Sampoorna, K. N. Nagendra, K. Sowmya +2

Quantum interference effects together with partial frequency redistribution (PFR) in line scattering produce subtle signatures in the so called Second Solar Spectrum (the linearly…