The Interface Region Imaging Spectrograph (IRIS) provides simultaneous imaging and spectral data of the chromosphere and transition region (TR) with great spatial, spectral and temporal resolution. A Solar coronal hole (CH) spectral observation by IRIS is studied for non-Gaussian Si IV profiles that fit the characteristics of UV burst events. Machine learning techniques such as k-means clustering and principal component analysis were applied on the data-set for classifying observed profiles into distinct groups. The least frequent representative profiles (RP), in terms of cluster size, managed to identify profiles that is characteristic for UV bursts events, i.e. complex, non-Gaussian shaped Si IV 1394 Å and Si 1403 Å profiles. It was found...
High-resolution spectral observations of the lower solar atmosphere (chromosphere and transition reg...
Transition-region explosive events (EEs) are characterized by non-Gaussian line profiles with enhanc...
Context. Surges are cool and dense ejections typically observed in chromospheric lines and closely r...
UV Bursts are small scale brightenings identified by dramatic intensification and broadening of emis...
Small reconnection events in the lower solar atmosphere can lead to its heating, but whether such he...
UV bursts are compact brightenings in active regions that appear in UV images. They are identified t...
Ultraviolet bursts (UVBs) are small-scale transient events indicative of magnetic reconnection in th...
We present a study of O IV density diagnostics in the far ultraviolet (FUV) spectra of UV bursts. UV...
The detection and mapping of Coronal Holes (CH) in solar Extreme Ultraviolet (EUV) images is useful ...
Spatially-resolved observations from the IRIS, SDO/AIA, and other space mission and ground-based tel...
Small-scale brightenings in solar atmospheric observations are a manifestation of heating and/or ene...
Abstract The Interface Region Imaging Spectrograph (IRIS) has been obtaining near- and far-ultraviol...
We compare abundance-sensitive and abundance-insensitive electron density diagnostics for a large sa...
Solar ultraviolet (UV) bursts are small-scale compact brightenings in transition region images. The ...
Context. Surges are cool and dense ejections typically observed in chromospheric lines and closely r...
High-resolution spectral observations of the lower solar atmosphere (chromosphere and transition reg...
Transition-region explosive events (EEs) are characterized by non-Gaussian line profiles with enhanc...
Context. Surges are cool and dense ejections typically observed in chromospheric lines and closely r...
UV Bursts are small scale brightenings identified by dramatic intensification and broadening of emis...
Small reconnection events in the lower solar atmosphere can lead to its heating, but whether such he...
UV bursts are compact brightenings in active regions that appear in UV images. They are identified t...
Ultraviolet bursts (UVBs) are small-scale transient events indicative of magnetic reconnection in th...
We present a study of O IV density diagnostics in the far ultraviolet (FUV) spectra of UV bursts. UV...
The detection and mapping of Coronal Holes (CH) in solar Extreme Ultraviolet (EUV) images is useful ...
Spatially-resolved observations from the IRIS, SDO/AIA, and other space mission and ground-based tel...
Small-scale brightenings in solar atmospheric observations are a manifestation of heating and/or ene...
Abstract The Interface Region Imaging Spectrograph (IRIS) has been obtaining near- and far-ultraviol...
We compare abundance-sensitive and abundance-insensitive electron density diagnostics for a large sa...
Solar ultraviolet (UV) bursts are small-scale compact brightenings in transition region images. The ...
Context. Surges are cool and dense ejections typically observed in chromospheric lines and closely r...
High-resolution spectral observations of the lower solar atmosphere (chromosphere and transition reg...
Transition-region explosive events (EEs) are characterized by non-Gaussian line profiles with enhanc...
Context. Surges are cool and dense ejections typically observed in chromospheric lines and closely r...