Results 101 to 110 of about 1,455,996 (195)
The Astrophysical JournalThis paper offers a fresh perspective on solar chromosphere heating and plasma outflows, focusing on the contribution of waves generated by solar granulation.
M. Kumar +5 more
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On the Response of the Transition Region and the Corona to Rapid Excursions in the Chromosphere
The Astrophysical JournalSpicules are the thin hair/grass-like structures that are prominently observed at the chromospheric solar limb. It is believed that fibrils and rapid blueshifted and redshifted excursions (RBEs and RREs; collectively referred to as REs) correspond to on ...
Ravi Chaurasiya +4 more
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Chromospheric Response to Nanoflares from IRIS2+ Inversion
The Astrophysical JournalNanoflares are considered one of the key mechanisms for heating the solar corona. Because they are difficult to observe directly, measurements at footpoints of coronal loops in the lower atmosphere can provide insight into their properties.
Kyuhyoun Cho +4 more
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The Astrophysical Journal LettersMagnetic tornadoes, characterized as impulsive Alfvén waves initiated by photospheric vortices in intergranular lanes, are considered efficient energy channels to the corona.
Hidetaka Kuniyoshi +2 more
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Performance of coloured solar collectors [PDF]
, 2009 The use of solar collectors with coloured absorbers for water heating is an area of particular interest when considering their integration with buildings.
Carson, James K. +2 more
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The Astrophysical JournalWe apply the HanleRT Tenerife Inversion Code to the spectropolarimetric observations obtained by the Chromospheric Layer Spectropolarimeter. This suborbital space experiment measured the variation with wavelength of the four Stokes parameters in the near-
Hao Li +12 more
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The Astrophysical JournalWe report on a flare-driven coronal rain event observed along postflare loops during the decay phase of an X1.6-class solar flare. Although high-resolution studies of flare-driven coronal rain have been conducted, imaging spectroscopic studies are rare ...
Donguk Song +8 more
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Spicules and their on-disk counterparts, the main driver for solar chromospheric heating?
, 2016 The question how the outer solar atmosphere is heated from solar photospheric temperatures of about 5800K up to solar chromospheric and coronal temperatures of about 20.000K and millions of degrees respectively, remained without any satisfying answer for centuries. On 4 May 2005, I recorded several time series of Halpha line scans with the GREGOR Fabry-
openaire +2 more sources
Passive solar space and water heating systems
, 1990 The performance of three types of passive solar feature has been studied; fifteen Roof-Space Collectors on an estate of low energy houses at the Milton Keynes Energy Park, 101m2 of Thermosyphoning Air Panels at a county primary school in Nazeing ...
Lo, S. N. G.
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Transition Region Brightening in a Moss Region and Their Relation with Lower Atmospheric Dynamics
The Astrophysical JournalSmall-scale brightenings (SBs) are commonly observed in the transition region (TR) that separates the solar chromosphere from the corona. These brightenings, omnipresent in active region patches known as “moss” regions, could potentially contribute to ...
Bhinva Ram +7 more
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