Results 101 to 110 of about 961,519 (212)
The Gondola for the Sunrise iii Balloon-Borne Solar Observatory
Publisher Copyright: © The Author(s) 2025.Sunrise iii is a balloon-borne solar observatory dedicated to investigating the physics governing the magnetism and dynamics in the lower solar atmosphere.
Korpi-Lagg, Andreas +24 more
core +1 more source
Variations in Dominant Wave Period in the Solar Atmosphere
Waves are an integral part of the solar atmosphere, and their characteristics (e.g., dominant period, range of periods, power, and phase angle) change on a diverse spatiotemporal scale.
Pradeep Kayshap +3 more
doaj +1 more source
Heat Transfer Analysis and Modeling for a Coaxial Solar Collector in a Domestic Cogeneration System
The need for an efficient energy system in domestic houses push the research toward innovative cogeneration system, which can meets the needs for electricity, heating and cooling power.
Alberto Bertaso +5 more
core +1 more source
Magnetic Flux Emergence and Solar Eruptions in Partially Ionized Plasmas
We have performed 3D MHD simulations to study the effect of partial ionization in the process of magnetic flux emergence in the Sun. In fact, we continue previous work, and we now focus (1) on the emergence of the magnetic fields above the solar ...
Georgios Chouliaras, V. Archontis
doaj +1 more source
MHD simulations of the solar photosphere
We briefly review the observations of the solar photosphere and pinpoint some open questions related to the magnetohydrodynamics of this layer of the Sun. We then discuss the current modelling efforts, addressing among other problems,
T. Roudier, M. Rieutord, F. Rincon
core +1 more source
Magnetic flux ropes are fundamental magnetic structures in solar eruptions, whose formation is generally attributed to: (1) the emergence of subsurface flux tubes; or (2) flux cancellation driven by photospheric horizontal flows and magnetic reconnection.
Can Wang +5 more
doaj +1 more source
Spatial stratification of acoustic oscillations in the solar photosphere
Space-time variations of solar atmosphere parameters are derived by solving non-equilibrium radiation transfer problem. Acoustic oscillations were extracted using k − ω filtration of variations.
Stodilka, M.I.
core
Magnetic Fields in the Solar Convection Zone
Active regions on the solar surface are generally thought to originate from a strong toroidal magnetic field generated by a deep seated solar dynamo mechanism operating at the base of the solar convection zone.
Yuhong Fan
doaj
Chromospheric differential rotation is a key component in comprehending the atmospheric coupling between the chromosphere and the photosphere at different phases of the solar cycle. In this study, we therefore utilize the newly calibrated multidecadal Ca
Dibya Kirti Mishra +7 more
doaj +1 more source
Structure of the solar photosphere studied from the radiation hydrodynamics code ANTARES. [PDF]
Leitner P +6 more
europepmc +1 more source

