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Extended MHD modeling of the steady solar corona and the solar wind [PDF]
Living Reviews in Solar Physics, 2018 The history and present state of large-scale magnetohydrodynamic modeling of the solar corona and the solar wind with steady or quasi-steady coronal physics is reviewed.
Tamas I. Gombosi +3 more
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Chromospheric Jets and Their Properties [PDF]
Iranian Journal of Astronomy and Astrophysics, 2022 In this study we review solar chromospheric jets and characteristics of them. The chromosphere and transition region are the interface between the solar photosphere and the corona, which plays a key role in the formation and acceleration of the solar ...
Ehsan Tavabi, Sima Zeighami
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Polarization of white-light solar corona and sky polarization effect during total solar eclipse on March 29, 2006 [PDF]
Serbian Astronomical Journal, 2019 Ground-based total solar eclipse observations are still the key method for coronal investigations. The question about its white-light degree of polarization remains unanswered.
Merzlyakov V. L. +3 more
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Magnetic Reconnection as the Driver of the Solar Wind
The Astrophysical Journal, 2023 We present EUV solar observations showing evidence for omnipresent jetting activity driven by small-scale magnetic reconnection at the base of the solar corona.
Nour E. Raouafi +18 more
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Energy Budget in the Solar Corona
The Astrophysical Journal, 2023 This paper addresses the first direct investigation of the energy budget in the solar corona. Exploiting joint observations of the same coronal plasma by Parker Solar Probe and the Metis coronagraph aboard Solar Orbiter and the conserved equations for ...
Daniele Telloni +36 more
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Investigating Coronal Holes and CMEs as Sources of Brightness Depletion Detected in PSP/WISPR Images
The Astrophysical Journal, 2023 The Parker Solar Probe (PSP) mission provides a unique opportunity to observe the solar corona from distances below 20 R _☉ . In this work, we utilize white light images from the Wide-field Imager for Solar PRobe aboard the PSP from solar encounters 10 ...
Guillermo Stenborg +4 more
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THE ROLE OF RADIO WAVE PROPAGATION EFFECTS IN THE SOLAR CORONA TO INTERPRET THE BEHIND-LIMB BURSTS
Radio Physics and Radio Astronomy, 2016 Purpose: The radio emission propagation of solar radio bursts in the solar corona which sources are located on the far side of the Sun relative to the observer on Earth is studied.
A. A. Stanislavsky
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EUV imaging and spectroscopy for improved space weather forecasting
Journal of Space Weather and Space Climate, 2020 Accurate predictions of harmful space weather effects are mandatory for the protection of astronauts and other assets in space, whether in Earth or lunar orbit, in transit between solar system objects, or on the surface of other planetary bodies. Because
Golub Leon +8 more
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Coronal spectral diagnostics: The coronal solar magnetism observatory (COSMO)
Frontiers in Astronomy and Space Sciences, 2022 The Need: Understanding and predicting the major phenomena taking place in the solar corona, such as flares and Coronal Mass Ejections (CMEs), the heating and evolution of the solar atmosphere, and the acceleration of the solar wind, are fundamental ...
Enrico Landi +9 more
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Slow solar wind acceleration through the middle corona: Spacecraft radio studies
Frontiers in Astronomy and Space Sciences, 2022 The “Middle Corona”, defined by recent consensus as the region spanning 1.5–6 solar radii (R⊙, heliocentric), is an important zone through which several structural and dynamic changes occur in coronal streamer regions. Among these is a regime change from
David B. Wexler +3 more
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