activity
20142026
most citedSolar Meridional Flow in the Shallow Interior during the Rising Phase of Cycle 24

51 citations · 85 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

Origin of Coronal Extreme Ultraviolet Shockwaves without a Coronal Mass Ejection Event

Robert Bush, John Stefan, Alexander Kosovichev

A leading theory of sunquake generation involves flare-accelerated particles depositing energy into the photosphere. Simulations of sunquake excitation suggest co-excitation with w…

astro-ph.SR2025

An Acoustic Model for Sunquakes Unifying the Solar Interior and Atmosphere

John Stefan, Alexander Kosovichev

One of the leading hypotheses for sunquake generation suggests that flare-accelerated particles originating from the reconnection site in the corona travel down to the chromosphere…

astro-ph.SR2025

Operational and Exploration Requirements and Research Capabilities for SEP Environment Monitoring and Forecasting

Viacheslav Sadykov, Petrus Martens, Dustin Kempton +15

Mitigating risks posed by solar energetic particles (SEPs) to operations and exploration in space and Earth's atmosphere motivates the development of advanced, synergistic approach…

astro-ph.SR2025

Structure and Dynamics of the Sun's Interior Revealed by Helioseismic and Magnetic Imager

Alexander Kosovichev, Sarbani Basu, Yuto Bekki +43

High-resolution helioseismology observations with the Helioseismic and Magnetic Imager (HMI) onboard Solar Dynamics Observatory (SDO) provide a unique three-dimensional view of the…

astro-ph.SR2014★ 51 cited

Solar Meridional Flow in the Shallow Interior during the Rising Phase of Cycle 24

Junwei Zhao, A. G. Kosovichev, R. S. Bogart

Solar subsurface zonal and meridional-flow profiles during the rising phase of solar cycle 24 are studied using time-distance helioseismology technique. The faster zonal bands in t…

astro-ph.SR2014★ 34 cited

High Resolution Observations of Chromospheric Jets in Sunspot Umbra

V. Yurchyshyn, V. Abramenko, S. Kosovichev +1

Recent observations of sunspot's umbra suggested that it may be finely structured at a sub-arcsecond scale representing a mix of hot and cool plasma elements. In this study we repo…