activity
20062019
most citedMagnetic Properties of Solar Active Regions that Govern Large Solar Flares and Eruptions

191 citations · 522 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2019★ 10 cited

An improved multi-ridge fitting method for ring-diagram helioseismic analysis

Kaori Nagashima, Aaron C. Birch, Jesper Schou +2

Context: There is a wide discrepancy in current estimates of the strength of convection flows in the solar interior obtained using different helioseismic methods applied to observa…

astro-ph.SR2018★ 5 cited

Probing sunspots with two-skip time-distance helioseismology

T. L. Duvall, P. S. Cally, D. Przybylski +2

Previous helioseismology of sunspots has been sensitive to both the structural and magnetic aspects of sunspot structure. We aim to develop a technique that is insensitive to the m…

astro-ph.SR2016★ 5 cited

The amplitude of the cross-covariance function of solar oscillations as a diagnostic tool for wave attenuation and geometrical spreading

Kaori Nagashima, Damien Fournier, Aaron C. Birch +1

Context. In time-distance helioseismology, wave travel times are measured from the two-point cross-covariance function of solar oscillations and are used to image the solar convect…

astro-ph.SR2016★ 191 cited

Magnetic Properties of Solar Active Regions that Govern Large Solar Flares and Eruptions

Shin Toriumi, Carolus J. Schrijver, Louise K. Harra +2

Solar flares and coronal mass ejections (CMEs), especially the larger ones, emanate from active regions (ARs). With the aim to understand the magnetic properties that govern such f…

astro-ph.SR2016

Statistics of the two-point cross-covariance function of solar oscillations

Kaori Nagashima, Takashi Sekii, Laurent Gizon +1

Context: The cross-covariance of solar oscillations observed at pairs of points on the solar surface is a fundamental ingredient in time-distance helioseismology. Wave travel times…

astro-ph.SR2014★ 30 cited

Interpreting the Helioseismic and Magnetic Imager (HMI) Multi-Height Velocity Measurements

Kaori Nagashima, Björn Löptien, Laurent Gizon +6

The Solar Dynamics Observatory/Helioseismic and Magnetic Imager (SDO/HMI) filtergrams, taken at six wavelengths around the Fe I 6173.3 Å line, contain information about the line-of…