We present an overview of fine-scale features in the Suns atmosphere, with a focus on spicules and jets. We consider older and newer observations and theories for chromospheric spicules and coronal jets. We also consider the connection between these features and some other solar atmospheric phenomena. We then discuss the possibility that there is a continuum of jet-like features ranging from spicules to large-scale CME-producing eruptions, all driven by similar magnetic processes operating on differing corresponding size scales. Future observational and theoretical studies will help clarify further the nature of these solar events, and elucidate possible connections between them
Observations of jet- like phenomena near the solar limb are reported for a long time, firs...
We observe an erupting jet feature in a solar polar coronal hole, using data from Hinode/SOT, EIS, a...
Abstract. The solar chromosphere is occupied with a wealth of fine structures referred to by diverse...
In this thesis we present a study of chromospheric features and their role in coupling the different...
Understanding the fine structures and transient phenomena associated with the origins of the fast so...
The atmosphere of the Sun is envisioned as composed of inherently complex, non-homogeneous, and dyna...
Coronal jets represent important manifestations of ubiquitous solar transients, which may be the sou...
Here, we explore the nature of small-scale jet-like structures and their possible relation to explos...
Spicules are plasma jets that are observed in the dynamic interface region between the visible solar...
The solar chromosphere has previously been thought to be a homogenic layer of the solar atmosphere, ...
Here, we explore the nature of small-scale jet-like structures and their possible relation to explos...
Coronal jets represent important manifestations of ubiquitous solar transients, which may be the sou...
Coronal jets represent important manifestations of ubiquitous solar transients, which may be the sou...
Spicules are the most ubuiquitous type of jets in the solar atmosphere. The advent of high-resolutio...
Observations of jet- like phenomena near the solar limb are reported for a long time, firs...
We observe an erupting jet feature in a solar polar coronal hole, using data from Hinode/SOT, EIS, a...
Abstract. The solar chromosphere is occupied with a wealth of fine structures referred to by diverse...
In this thesis we present a study of chromospheric features and their role in coupling the different...
Understanding the fine structures and transient phenomena associated with the origins of the fast so...
The atmosphere of the Sun is envisioned as composed of inherently complex, non-homogeneous, and dyna...
Coronal jets represent important manifestations of ubiquitous solar transients, which may be the sou...
Here, we explore the nature of small-scale jet-like structures and their possible relation to explos...
Spicules are plasma jets that are observed in the dynamic interface region between the visible solar...
The solar chromosphere has previously been thought to be a homogenic layer of the solar atmosphere, ...
Here, we explore the nature of small-scale jet-like structures and their possible relation to explos...
Coronal jets represent important manifestations of ubiquitous solar transients, which may be the sou...
Coronal jets represent important manifestations of ubiquitous solar transients, which may be the sou...
Spicules are the most ubuiquitous type of jets in the solar atmosphere. The advent of high-resolutio...
Observations of jet- like phenomena near the solar limb are reported for a long time, firs...
We observe an erupting jet feature in a solar polar coronal hole, using data from Hinode/SOT, EIS, a...
Abstract. The solar chromosphere is occupied with a wealth of fine structures referred to by diverse...