2012
DOI: 10.1007/s11214-012-9920-2
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Solar Fine-Scale Structures. I. Spicules and Other Small-Scale, Jet-Like Events at the Chromospheric Level: Observations and Physical Parameters

Abstract: Over the last two decades the uninterrupted, high resolution observations of the Sun, from the excellent range of telescopes aboard many spacecraft complemented with observations from sophisticated ground-based telescopes have opened up a new world producing significantly more complete information on the physical conditions of the solar atmosphere than before. The interface between the lower solar atmosphere where energy is generated by subsurface convection and the corona comprises the chromosphere, which is … Show more

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Cited by 168 publications
(166 citation statements)
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References 188 publications
(281 reference statements)
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“…This magnetic reconnection between newly emerging magnetic flux and the ambient field plays a major role for jets has been confirmed in numerical experiments recently by Moreno-Insertis and Galsgaard (2013). For a recent review on small-scale, jet-like events at chromospheric levels, we refer to Tsiropoula et al (2012), as well as to Sect. 6.2.4 for polar jets.…”
Section: Jetssupporting
confidence: 62%
“…This magnetic reconnection between newly emerging magnetic flux and the ambient field plays a major role for jets has been confirmed in numerical experiments recently by Moreno-Insertis and Galsgaard (2013). For a recent review on small-scale, jet-like events at chromospheric levels, we refer to Tsiropoula et al (2012), as well as to Sect. 6.2.4 for polar jets.…”
Section: Jetssupporting
confidence: 62%
“…(for a review see Tsiropoula et al 2012). The IBIS images were overlayed with the EIS contour of the blueshifted coronal emission to determine the region associated with the AR upflow.…”
Section: Ibismentioning
confidence: 99%
“…The plasma-β parameter (with β defined as the ratio of the gas pressure to the magnetic pressure) is used to distinguish between these two regimes, and the condition β = 1 defines the location of the magnetic canopy. In and above the magnetic canopy layer, flux tubes become highly inclined, and the chromosphere in Hα appears as a mesh pattern of elongated dark structures, most of them related to mottles (see Tsiropoula et al 2012, for a comprehensive review on their properties).…”
Section: Introductionmentioning
confidence: 99%