Results 31 to 40 of about 1,379,332 (142)
STOCHASTIC SEISMIC EMISSION FROM ACOUSTIC GLORIES AND THE QUIET SUN [PDF]
. Helioseismic images of multipolar active regions show enhanced seismic emission in 5-mHz oscillations in a halo surrounding the active region called the ‘acoustic glory’. The acoustic glories contain elements that sustain an average seismic emission 50
C. Lindsey +3 more
core +1 more source
The Complex Nature of Magnetic Element Transport in the Quiet Sun: The Multiscaling Character
In recent studies the dynamic properties of small-scale magnetic fields (magnetic elements [MEs]) in the quiet Sun were used to investigate peculiar features of turbulent convection and get insights on the characteristic spatial and temporal scales of ...
Giannattasio, Fabio, Consolini, Giuseppe
core +1 more source
Inferring depth-dependent plasma motions from surface observations using the DeepVel neural network
Coverage of plasma motions is limited to the line-of-sight component at the Sun’s surface. Multiple tracking and inversion methods were developed to infer the transverse motions from observational data.
Tremblay Benoit +4 more
doaj +1 more source
Estimating the longitudinal magnetic field in the chromosphere of quiet-Sun magnetic concentrations [PDF]
Context. Details of the magnetic field in the quiet-Sun chromosphere are key to our understanding of essential aspects of the solar atmosphere. However, the strength and orientation of this magnetic field have not been thoroughly studied at high spatial ...
M. J. Martínez González +10 more
core +1 more source
Incoherent Solar Radio Emission
Incoherent solar radio radiation comes from the free-free, gyroresonance, and gyrosynchrotron emission mechanisms. Free-free is primarily produced from Coulomb collisions between thermal electrons and ions.
Alexander Nindos
doaj +1 more source
Cosmogenic radionuclides reveal an extreme solar particle storm near a solar minimum 9125 years BP
Cosmogenic radionuclides from ice cores and tree rings indicate that an extreme solar proton event has hit Earth about 9200 years ago. Contrary to expectations, the event occurred during a quiet phase of the Sun within the 11 year solar cycle.
Chiara I. Paleari +12 more
doaj +1 more source
Modulation of Cosmic-Ray Antiprotons in the Heliosphere: Simulations for a Solar Cycle
The precision measurements of galactic cosmic-ray protons from the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics and the Alpha Magnetic Spectrometer are reproduced using a well-established three-dimensional numerical model for ...
O. P. M. Aslam +3 more
doaj +1 more source
Determination of field strengths in the quiet Sun
The magnetism in the quiet regions of the solar photosphere carries information on the dynamo processes and its interaction with the convection of the outer layers of the sun.
M. J. Martínez González +5 more
core +1 more source
Center-to-limb variations of solar active regions
Accurate modeling of stellar active regions (ARs) remains a major bottleneck for radial-velocity and transmission-spectroscopy studies aimed at finding Earth-like planets. While much effort has been devoted to AR modeling, their center-to-limb variations
Pietrow A. G. M. +5 more
doaj +1 more source
Photospheric Swirls in a Quiet-Sun Region
Swirl-shaped flow structures have been observed throughout the solar atmosphere, in both emission and absorption, at different altitudes and locations, and are believed to be associated with magnetic structures. However, the distribution patterns of such
Quan Xie +4 more
doaj +1 more source

