Coronal Condensations Caused by Magnetic Reconnection between Solar Coronal Loops [PDF]
AbstractEmployingSolar Dynamics Observatory/Atmospheric Imaging Assembly (AIA) multi-wavelength images, we report the coronal condensation during the magnetic reconnection (MR) between a system of open and closed coronal loops. Higher-lying magnetically open structures, observed in AIA 171 Å images above the solar limb, move downward and interact with ...
Leping Li +7 more
openaire +4 more sources
STATISTICAL EVIDENCE FOR THE EXISTENCE OF ALFVÉNIC TURBULENCE IN SOLAR CORONAL LOOPS [PDF]
10 pages, 6 figures, 1 ...
Jiajia Liu +4 more
openaire +5 more sources
3D Reconstruction of Coronal Loops by the Principal Component Analysis [PDF]
Knowing the three dimensional structure of plasma filaments in the uppermost part of the solar atmosphere, known as coronal loops, and especially their length, is an important parameter in the wave-based diagnostics of this part of the Sun.
Erwin Verwichte +2 more
doaj +2 more sources
Self-organized braiding in solar coronal loops [PDF]
AbstractIn this paper, we investigate the evolution of braided solar coronal loops. We assume that coronal loops consist of several internal strands which twist and braid about each other. Reconnection between the strands leads to small flares and heating of the loop to x-ray temperatures.
Berger, M.A. +2 more
core +4 more sources
Reduced Thermal Conduction in Solar Coronal Loops
Thermal conduction plays an important role in the energy balance of the solar coronal plasma. In this paper, we present a new method for deriving observational constraints on the density–temperature relationship for coronal loops from the differential ...
M. Asgari-Targhi, A. A. van Ballegooijen
doaj +2 more sources
Radiation-Resistant Aluminum Alloy for Space Missions in the Extreme Environment of the Solar System. [PDF]
A novel ultrafine‐grained aluminum crossover alloy exhibits unprecedented radiation resistance and mechanical stability under extreme irradiation doses up to 100 dpa. The exceptional resilience arises from thermodynamically stable T‐phase precipitates, enabling lightweight structural materials for next‐generation spacecraft and extraterrestrial ...
Willenshofer PD +9 more
europepmc +2 more sources
Acoustic response to transverse oscillations in a solar coronal loop [PDF]
Context. Magnetohydrodynamic (MHD) waves play an important role in the dynamics and heating of the solar corona. Their investigation also reveals information about the local conditions. Transverse (Alfvénic) oscillations of loops commonly occur in response to solar eruptions. It has been shown that these oscillations elicit an acoustic response through
S. J. White, E. Verwichte
openaire +2 more sources
HomoTherm: An Open-Source Approach to Modelling Heat Exchange in Humans and Other Hominins in Diverse Environments. [PDF]
We present ‘HomoTherm’, a human heat budget model for simulating humans and related species with diverse traits in diverse environments. It is part of the NicheMapR package for biophysical modelling and is a multi‐part extension of the ‘endoR’ function.
Kearney MR, Mitchell D, Maloney SK.
europepmc +2 more sources
EUV FLICKERING OF SOLAR CORONAL LOOPS: A NEW DIAGNOSTIC OF CORONAL HEATING [PDF]
ABSTRACT A previous work of ours found the best agreement between EUV light curves observed in an active region core (with evidence of super-hot plasma) and those predicted from a model with a random combination of many pulse-heated strands with a power-law energy distribution.
E. Tajfirouze +3 more
openaire +2 more sources
Observational signatures of waves and flows in the solar corona [PDF]
DM acknowledges support of a Royal Society University Research Fellowship and a KU Leuven Research Council senior research fellowship (SF/12/008). The research leading to these results has also received funding from the European Commission Seventh ...
Antolin, Patrick +3 more
core +1 more source

