activity
20132025
most citedThermal Diagnostics with the Atmospheric Imaging Assembly onboard the Solar Dynamics Observatory: A Validated Method for Differential Emission Measure Inversions

301 citations · 349 across the 6 of their papers we have counts for

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Showing astro-ph.SRShow all

11 papers · 1 filter

astro-ph.SR20251 cited

Active region upflows in various coronal structures and their coupling to the lower atmosphere

Yingjie Zhu, Louise Harra, Krzysztof Barczynski +13

Plasma upflows with a Doppler shift exceeding -10 km/s at active region (AR) boundaries are considered potential sources of the nascent slow solar wind. We investigate the driving…

astro-ph.SR20252 cited

Anomalous cross-field motions of solar coronal loops

Sudip Mandal, Hardi Peter, James A. Klimchuk +1

Here, we present several examples of unusual evolutionary patterns in solar coronal loops that resemble cross-field drift motions. These loops were simultaneously observed from two…

astro-ph.SR20246 cited

Stereoscopic observations reveal coherent morphology and evolution of solar coronal loops

B. Ram, L. P. Chitta, S. Mandal +2

Coronal loops generally trace magnetic lines of force in the upper solar atmosphere. Understanding the loop morphology and its temporal evolution has implications for coronal heati…

astro-ph.SR2023

Small-scale Dynamo in Cool Stars III. Changes in the photospheres of F3V to M0V stars

Tanayveer S. Bhatia, Robert H. Cameron, Hardi Peter +1

Some of the quiet solar magnetic flux could be attributed to a small-scale dynamo (SSD) operating in the convection zone. An SSD operating in cool main-sequence stars is expected t…

astro-ph.SR2020

Impulsive coronal heating during the interaction of surface magnetic fields in the lower solar atmosphere

L. P. Chitta, H. Peter, E. R. Priest +1

Coronal plasma in the cores of solar active regions is impulsively heated to more than 5 MK. The nature and location of the magnetic energy source responsible for such impulsive he…

astro-ph.SR2019

Plasmoid-mediated reconnection in solar UV bursts

H. Peter, Y. -M. Huang, L. P. Chitta +1

UV bursts are transients in the solar atmosphere with an increased impulsive emission in the extreme UV lasting for one to several tens of minutes. They often show spectral profile…