Results 111 to 120 of about 1,455,996 (195)
Understanding the mechanisms underlying the heating of the solar atmosphere is a fundamental problem in solar physics. The lower atmosphere of the Sun (i.e., photosphere and chromosphere) is composed of weakly ionized plasma.
M. S. Yalim +6 more
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Models currently fail to reproduce observations of the coldest regions in the Sun’s atmosphere, though recent work suggests the thermal Farley–Buneman instability (TFBI) may play a critical role.
Samuel Evans +3 more
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We present the analysis of high-resolution H α observations of fan-shaped jets above a penumbral light bridge (LB) subject to external disturbance through fast downflows in active region (AR) 12683 using data from the Goode Solar Telescope and the ...
Kristina Brocklebank +2 more
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How Are the Abnormally Hot Chromosphere and Corona Heated by the Solar Magnetic Fields?
Abstract The corona is a structure possessed by stars, including the Sun. The abnormal heating of the solar corona and chromosphere is one of the greatest mysteries in modern astronomy. While state-of-the-art observations have identified some candidates of magnetic activity events that could be responsible for this abnormal heating, and ...
K. J. Li +5 more
openaire +3 more sources
Context. Solar spicules are highly dynamic chromospheric jets that play an important role in the mass and energy balance of the solar atmosphere, even though their connection to the transition region and corona remains unclear. Aims.
Chaurasiya Ravi +2 more
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The nature of energy generation, transport, and effective dissipation responsible for maintaining a hot solar upper atmosphere is still elusive. The Poynting flux is a vital parameter for describing the direction and magnitude of the energy flow, which ...
Suzana S. A. Silva +5 more
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Small-scale jets, such as chromospheric and transition region (TR) network jets, are of great interest regarding coronal heating and solar wind acceleration. Spectroscopic analysis based on multiple spectral lines with different formation temperatures is
Eun-Kyung Lim +8 more
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Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]
Cang T +13 more
europepmc +2 more sources
Sequential Magnetic Reconnections in a Fishbone-like Structure Leading to Recurrent Brightenings
The fine-scale release of magnetic free energy in the solar atmosphere is a fundamental open question in solar physics. Multiwavelength observations at high spatiotemporal resolution now offer a direct window into this process.
Bo Yang +3 more
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Vortex Motions in the Solar Atmosphere: Definitions, Theory, Observations, and Modelling. [PDF]
Tziotziou K +14 more
europepmc +1 more source

