Results 71 to 80 of about 1,264 (196)
Near infrared observations of solar chromosphere
, 2015 Includes bibliographical references (leaves 30-31)The solar chromosphere is an excellent medium to explore the intricate interplay between plasma and magnetic fields in a regime where both are relevant and alternately dominant.
Tejomoortula, Usha Sree
core
Structure of sunspot light bridges in the chromosphere and transition region
, 2018 Context. Light bridges (LBs) are elongated structures with enhanced intensity embedded in sunspot umbra and pores. Aims. We studied the properties of a sample of 60 LBs observed with the Interface Region Imaging Spectrograph (IRIS ...
R. Rezaei
core +1 more source
Semiempirical Models of the Solar Atmosphere. II. The Quiet‐Sun Low Chromosphere at Moderate Resolution [PDF]
, 2007 J. M. Fontenla +2 more
openalex +1 more source
Propagation and damping of MHD waves in the solar atmosphere
, 2015 Quasi-periodic disturbances have been observed in the outer solar atmosphere for many years. Although first interpreted as upflows (Schrijver et al.
Kiddie, Greg
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Calcium Bright Knots and the Formation of Chromospheric Anemone Jets on the Sun
The Astrophysical Journal LettersAbstract Space-based observations show that the solar atmosphere from the solar chromosphere to the solar corona is filled with small-scale jets and is linked with small-scale explosions. These jets may be produced by mechanisms similar to those of large-scale flares and such jets may be related to the heating of the corona and ...
Kunwar Alkendra Pratap Singh +2 more
openaire +3 more sources
, 2012 Popis základních fyzikálních jevů na Slunci.Metody pozorování fotosféry a chromosféry Slunce. Společné jevy v chromosféře a fotosféře Slunce.Návod na pozorovací protokoly. Zpracování dat z pozorování.
Toman, Jakub
core
Near infrared observations of solar chromosphere
, 2009 The solar chromosphere is an excellent medium to explore the intricate interplay between plasma and magnetic fields in a regime where both are relevant and alternately dominant.
Tejomoortula, Usha Sree
core
On the Origin of the Magnetic Energy in the Quiet Solar Chromosphere
, 2019 The presence of magnetic field is crucial in the transport of energy through the solar atmosphere. Recent ground-based and space-borne observations of the quiet Sun have revealed that magnetic field accumulates at photospheric heights, via a local dynamo
Martinez-Sykora, Juan +5 more
core +1 more source
Dynamics of magnetized vortex tubes in the solar chromosphere [PDF]
, 2012 We use three-dimensional radiative MHD simulations to investigate the formation and dynamics of small-scale (less than 0.5 Mm in diameter) vortex tubes spontaneously generated by turbulent convection in quiet-Sun regions with an initially weak (10 G ...
Kitiashvili I. +3 more
core
An In-depth Analysis of Quiet-Sun IRIS Brightenings [PDF]
Small-scale brightenings are ubiquitous, dynamic, and energetic phenomena found in the chromosphere. An advanced filter-detection algorithm applied to high-resolution observations from the Interface Region Imaging Spectrograph enables the detection of ...
Kuridze, David +5 more
core +1 more source