143 citations · 272 across the 6 of their papers we have counts for
6 papers
Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release
Amir Caspi, Daniel B. Seaton, Roberto Casini +12
The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poo…
SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network
S. Wedemeyer, T. Bastian, R. Brajsa +27
The Solar Simulations for the Atacama Large Millimeter Observatory Network (SSALMON) was initiated in 2014 in connection with two ALMA development studies. The Atacama Large Millim…
Do solar decimetric spikes originate in coronal X-ray sources?
Marina Battaglia, Arnold O. Benz
In the standard solar flare scenario, a large number of particles are accelerated in the corona. Nonthermal electrons emit both X-rays and radio waves. Thus, correlated signatures…
A nanoflare heating model for the quiet solar corona
U. Mitra-Kraev, A. O. Benz
The energy input into the lower solar corona by flare evaporation events has been modeled according to the available observations for quiet regions. The question is addressed wheth…
Spatial analysis of solar type III events associated with narrow band spikes at metric wavelengths
G. Paesold, A. O. Benz, K. -L. Klein +1
The spatial association of narrow band metric radio spikes with type III bursts is analyzed. The analysis addresses the question of a possible causal relation between the spike emi…
Solar flare radio pulsations as a signature of dynamic magnetic reconnection
B. Kliem, M. Karlicky, A. O. Benz
Decimetric radio observations of the impulsive solar flare on October 5, 1992, 09:25 UT show a long series of quasi-periodic pulsations deeply modulating a continuum in the 0.6-2 G…