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The universality of power law slopes in the solar photosphere and transition region observed with HMI and IRIS
Published 2023-03-01“…We compare the size distributions of self-organized criticality (SOC) systems in the solar photosphere and the transition region, using magnetogram data from Helioseismic and Magnetic Imager (HMI) and Interface Region Imaging Spectrograph (IRIS) data. …”
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42
Multiline Stokes Synthesis of Ellerman Bombs: Obtaining Seamless Information from Photosphere to Chromosphere
Published 2023-01-01“…In the case of magnetic reconnection at low altitude, both red- and blueshifted components originating from reconnection bidirectional flow are identified in the photospheric lines, Fe i 8468 Å, K i 7664 Å, and K i 7698 Å. …”
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43
Identification of photospheric activity features from SOHO/MDI data using the ASAP tool
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44
Global solar photospheric and coronal magnetic field over activity cycles 21–25
Published 2024-01-01Subjects: Get full text
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45
Over 500 Days in the Life of the Photosphere of the Type Iax Supernova SN 2014dt
Published 2023-01-01“…The unique properties of SNe Iax, especially their strong photospheric lines out to extremely late times, allow us to model their optical spectra and derive the physical parameters of the long-lasting photosphere. …”
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46
The Incompatibility of Rapid Rotation with Narrow Photospheric X-Ray Lines in Exo 0748-676
Published 2013“…X-ray observations of EXO 0748–676 during thermonuclear bursts revealed a set of narrow (Δλ/λ = 0.018) absorption lines that potentially originate from the stellar photosphere. The identification of these lines with particular atomic transitions led to the measurement of the surface gravitational redshift of the neutron star and to constraints on its mass and radius. …”
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47
Photospheric activity and rotation of the planet-hosting star CoRoT-Exo-4a
Published 2009“…It assumes that stellar active regions consist of cool spots and bright faculae, analogous to sunspots and solar photospheric faculae, whose visibility is modulated by stellar rotation. …”
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48
Simulating the Photospheric to Coronal Plasma Using Magnetohydrodynamic Characteristics. I. Data-driven Boundary Conditions
Published 2024-01-01Subjects: Get full text
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49
The Imprint of Convection on Type I X-Ray Bursts: Pauses in Photospheric Radius Expansion Lightcurves
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50
Hybrid Detection Algorithm and Study on the Quantity and Brightness Evolution Characteristics of Photospheric Bright Point Groups
Published 2023-01-01Subjects: Get full text
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51
Large Photospheric Doppler Shift in Solar Active Region 12673. I. Field-aligned Flows
Published 2023-01-01“…Delta ( δ ) sunspots sometimes host fast photospheric flows along the central magnetic polarity inversion line (PIL). …”
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52
The Role of a Neutron Component in the Photospheric Emission of Long-duration Gamma-Ray Burst Jets
Published 2024-01-01“…Here, we present results of the photospheric emission from an LGRB jet, using a combination of relativistic hydrodynamic simulations and radiative transfer postprocessing using Monte Carlo radiation transfer code. …”
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53
Photospheric activity, rotation, and radial velocity variations of the planet-hosting star CoRoT-7
Published 2010Journal article -
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Photospheric activity, rotation, and star-planet interaction of the planet-hosting star CoRoT-6
Published 2010“…The CoRoT satellite has recently discovered a hot Jupiter that transits across the disc of a F9V star called CoRoT-6 with a period of 8.886 days. We model the photospheric activity of the star and use the maps of the active regions to study stellar differential rotation and the star-planet interaction. …”
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55
ASYMMETRY IN OCCURRENCE OF THE LEADING AND FOLLOWING POLARITIES IN THE PHOTOSPHERIC MAGNETIC FIELD AT THE EARLY STAGE OF ACTIVE REGION FORMATION
Published 2020-12-01“…We study the evolution of the photospheric magnetic field at the early stage of active region development. …”
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56
Converging photospheric vortex flows close to the polarity inversion line of a fully emerged active region
Published 2019-07-01“…<p>We report on the occurrence of vortexes in flow fields obtained from the evolution of the line-of-sight component of the photospheric magnetic field in a region around the polarity inversion line (PIL) of a fully emerged active region. …”
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57
MHD simulation of rapid change of photospheric magnetic field during solar eruption caused by magnetic reconnection
Published 2023-06-01“…It has been well observed that the horizontal component of the magnetic field at photosphere changes rapidly and irreversibly after solar eruptions. …”
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58
Numerical Simulation of Photospheric Emission in Long Gamma-Ray Bursts: Prompt Correlations, Spectral Shapes, and Polarizations
Published 2024-01-01“…We explore the properties of photospheric emission in the context of long gamma-ray bursts (GRBs) using three numerical models that combine relativistic hydrodynamical simulations and Monte Carlo radiation transfer calculations in three dimensions. …”
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59
Exploring possibilities for solar irradiance prediction from solar photosphere images using recurrent neural networks
Published 2022-01-01“…This paper presents a neural network-based approach, which uses images of the solar photosphere to extract sunspot and active region information and thus generate inputs for recurrent neural networks to perform the irradiance prediction. …”
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60
Photospheric Velocity Evolution of SN 2020bvc: Signature of r-process Nucleosynthesis from a Collapsar
Published 2023-01-01“…Based on semi-analytic SN emission models with and without r -process materials, we perform a fitting to the multiband light curves and photospheric velocities of SN 2020bvc. We find that in a r -process-enriched model the mixing of r -process materials slows down the photospheric recession and therefore matches the velocity evolution better. …”
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