11 citations · 13 across the 2 of their papers we have counts for
11 papers
Characteristic Length of Energy-Containing Structures at the Base of a Coronal Hole
V. I. Abramenko, G. P. Zank, A. Dosch +4
An essential parameter for models of coronal heating and fast solar wind acceleration that rely on the dissipation of MHD turbulence is the characteristic energy-containing length…
Dynamics of Chromospheric Upflows and Underlying Magnetic Fields
Vasyl Yurchyshyn, Valentyna Abramenko, Phil Goode
We used \ha-0.1 nm and magnetic field (at 1.56) data obtained with the New Solar Telescope to study the origin of the disk counterparts to type II spicules, so-called rapid blue…
Detection of Small-Scale Granular Structures in the Quiet Sun with the New Solar Telescope
Valentyna Abramenko, Vasyl Yurchyshyn, Philip Goode +2
Results of a statistical analysis of solar granulation are presented. A data set of 36 images of a quiet Sun area on the solar disk center was used. The data were obtained with the…
Turbulent Kinetic Energy Spectra of Solar Convection from NST Observations and Realistic MHD Simulations
I. N. Kitiashvili, V. I. Abramenko, P. R. Goode +5
Turbulent properties of the quiet Sun represent the basic state of surface conditions, and a background for various processes of solar activity. Therefore understanding of properti…
Turbulent Diffusion in the Photosphere as Derived from Photospheric Bright Point Motion
V. I. Abramenko, V. Carbone, V. Yurchyshyn +5
On the basis of observations of solar granulation obtained with the New Solar Telescope (NST) of Big Bear Solar Observatory, we explored proper motion of bright points (BPs) in a q…
Maximum Coronal Mass Ejection Speed as an Indicator of Solar and Geomagnetic Activities
A. Kilcik, V. B. Yurchyshyn, V. Abramenko +4
We investigate the relationship between the monthly averaged maximal speeds of coronal mass ejections (CMEs), international sunspot number (ISSN), and the geomagnetic Dst and Ap in…