activity
20052017
most citedCoexistence of Self-Organized Criticality and Intermittent Turbulence in the Solar Corona

66 citations · 91 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.SR20176 cited

Image-Optimized Coronal Magnetic Field Models

Shaela I. Jones, Joseph M. Davila, Vadim M. Uritsky

We have reported previously on a new method we are developing for using image-based information to improve global coronal magnetic field models. In that work we presented early tes…

astro-ph.SR2017

Slow-Mode Oscillations of Hot Loops Excited at Flaring Footpoints

Tongjiang Wang, Wei Liu, Leon Ofman +1

The analysis of a hot loop oscillation event using SOHO/SUMER, GOES/SXI, and RHESSI observations is presented. Damped Doppler shift oscillations were detected in the Fe XIX line by…

astro-ph.SR201719 cited

Variation of Coronal Activity from the Minimum to Maximum of Solar Cycle 24 using Three Dimensional Coronal Electron Density Reconstructions from STEREO/COR1

Tongjiang Wang, Nelson L. Reginald, Joseph M. Davila +2

Three dimensional electron density distributions in the solar corona are reconstructed for 100 Carrington Rotations (CR 20542153) during 2007/032014/08 using the spherically…

astro-ph200666 cited

Coexistence of Self-Organized Criticality and Intermittent Turbulence in the Solar Corona

Vadim M. Uritsky, Maya Paczuski, Joseph M. Davila +1

An extended data set of extreme ultraviolet images of the solar corona provided by the SOHO spacecraft are analyzed using statistical methods common to studies of self-organized cr…

astro-ph2005

Fe XI emission lines in a high resolution extreme ultraviolet spectrum obtained by SERTS

F. P. Keenan, K. M. Aggarwal, R. S. I. Ryans +5

New calculations of radiative rates and electron impact excitation cross sections for Fe XI are used to derive emission line intensity ratios involving 3s^23p^4 - 3s^23p^33d transi…