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Interface region imaging spectrograph (IRIS) observations of the fractal dimension in the solar atmosphere
Published 2022-11-01“…We focus here on impulsive phenomena and Quiet-Sun features in the solar transition region, observed with the Interface Region Imaging Spectrograph (IRIS) at 1,400 Å (at formation temperatures of Te ≈ 104–106 K). …”
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2
Rapid variations of Si IV spectra in a flare observed by interface region imaging spectrograph at a sub-second cadence
Published 2022-11-01“…We report on observations of highly-varying Si IV 1402.77 Å line profiles observed with the Interface Region Imaging Spectrograph (IRIS) during the M-class flare from 18 January 2022 at an unprecedented 0.8 s cadence. …”
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3
The Plasma β in Quiet Sun Regions: Multi-instrument View
Published 2024-01-01“…A joint campaign of several spaceborne and ground-based observatories, such as the GREGOR solar telescope, the Extreme-ultraviolet Imaging Spectrometer (EIS), and the Interface Region Imaging Spectrograph (Hinode Observing Plan 381, 2019 October 11–22) was conducted to investigate the plasma β in quiet Sun regions. …”
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4
High-Frequency Dynamics of Active Region Moss as Observed by IRIS
Published 2019-05-01“…The high temporal, spatial and spectral resolution of Interface Region Imaging Spectrograph (IRIS) has provided new insights into the understanding of different small-scale processes occurring at the chromospheric and transition region (TR) heights. …”
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5
The universality of power law slopes in the solar photosphere and transition region observed with HMI and IRIS
Published 2023-03-01“…We compare the size distributions of self-organized criticality (SOC) systems in the solar photosphere and the transition region, using magnetogram data from Helioseismic and Magnetic Imager (HMI) and Interface Region Imaging Spectrograph (IRIS) data. For each dataset we fit a combination of a Gaussian and a power law size distribution function, which yields information on four different physical processes: (i) Gaussian random noise in IRIS data; (ii) spicular events in the plages of the transition region (described by power law size distribution in IRIS data); (iii) salt-and-pepper small-scale magnetic structures (described by the random noise in HMI magnetograms); and (iv) magnetic reconnection processes in flares and nanoflares (described by power law size distributions in HMI data). …”
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Interrogating solar flare loop models with IRIS observations 2: Plasma properties, energy transport, and future directions
Published 2023-01-01“…Over the last decade, data from the Interface Region Imaging Spectrograph (IRIS) have provided the crucial observations with which we can critically interrogate the predictions of those flare loop models. …”
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Multi-wavelength observations and modeling of a microflare: constraining non-thermal particle acceleration
Published 2023-09-01“…In this work we analyze a small B-class flare that occurred on 29 April 2021 and was observed simultaneously by the Interface Region Imaging Spectrograph (IRIS) and the Nuclear Spectroscopic Telescope Array (NuSTAR) X-ray instrument. …”
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8
Multivariate Time Series Information Bottleneck
Published 2023-05-01“…An evaluation of our multiple time series–information bottleneck (MTS-IB) model proves its efficiency in electricity production, road traffic, and astronomical data representing solar activity, as recorded by NASA’s interface region imaging spectrograph (IRIS) satellite.…”
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Evidence for a Magnetic Flux Rope in Observations of a Solar Prominence-Cavity System
Published 2016-03-01“…We describe observations of a coronal cavity situated above a solar prominence observed on the western limb as part of an Interface Region Imaging Spectrograph (IRIS) and Hinode coordinated Observation Program (IHOP 264). …”
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Transverse MHD Waves as Signatures of Braiding-induced Magnetic Reconnection in Coronal Loops
Published 2024-01-01“…We present for the first time Interface Region Imaging Spectrograph and Solar Dynamics Observatory observations of transverse MHD waves in a coronal loop that directly result from braiding-induced reconnection. …”
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11
Near-ultraviolet continuum modeling of the 1985 April 12 great flare of AD Leo
Published 2022-11-01“…We use spatially resolved analyses of solar flare data from the Interface Region Imaging Spectrograph, combined with the results of previous radiative-hydrodynamic modeling of the 2014 March 29 X1 solar flare (SOL20140329T17:48), to interpret the two-component electron beam model as representing the spatial superposition of bright kernels and fainter ribbons over a larger area.…”
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Interrogating solar flare loop models with IRIS observations 1: Overview of the models, and mass flows
Published 2022-12-01“…In recent years, driven in part by the spectacular observations from the Interface Region Imaging Spectrograph (IRIS), flare loop models have revealed many interesting features of flares. …”
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Global Impact of Emerging Internetwork Fields on the Low Solar Atmosphere
Published 2024-01-01“…We use high-resolution, multiwavelength, coordinated observations obtained with the Interface Region Imaging Spectrograph, Hinode, and the Solar Dynamics Observatory to identify emerging IN magnetic fields and follow their evolution. …”
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An Optically Thin View of the Solar Chromosphere from Observations of the O i 1355 Å Spectral Line
Published 2023-01-01“…We present an analysis of a variety of observations of this line with the Interface Region Imaging Spectrograph (IRIS), and compare it with other IRIS diagnostics as well as diagnostics of the photospheric magnetic field. …”
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Non-thermal broadening of IRIS Fe XXI line caused by turbulent plasma flows in the magnetic reconnection region during solar eruptions
Published 2023-02-01“…We calculate the synthetic profiles of the Fe XXI 1354 Å line observed by the Interface Region Imaging Spectrograph (IRIS) spacecraft by using parameters of the MHD model, including plasma density, temperature, and velocity. …”
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The Transition Region of Solar Flare Loops
Published 2023-01-01“…We address this issue by analyzing high–spatial and temporal resolution EUV observations from an X1.6-class flare, taken with the Interface Region Imaging Spectrograph and the Solar Dynamic Observatory/Atmospheric Imaging Assembly (AIA). …”
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Type III Radio Bursts Observations on 20th August 2017 and 9th September 2017 with LOFAR Bałdy Telescope
Published 2021-01-01“…Additionally to LOFAR observations, the data recorded by instruments on boards of the Interface Region Imaging Spectrograph (IRIS) and Solar Dynamics Observatory (SDO) in the UV spectral range complement observations in the radio field. …”
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Spectral Evolution of an Eruptive Polar Crown Prominence With IRIS Observations
Published 2021-09-01“…In this paper we will introduce an eruptive polar crown prominence with spectral observations from the Interface Region Imaging Spectrograph (IRIS), and try to explain some phenomena that are rarely reported in previous works. …”
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Spatial and Temporal Analysis of Quiescent Coronal Rain over an Active Region
Published 2023-01-01“…We conduct a statistical study of coronal rain observed over an AR off limb with Interface Region Imaging Spectrograph and Solar Dynamics Observatory imaging data, spanning chromospheric to transition region (TR) temperatures. …”
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High-resolution Observations of the Low Atmospheric Response to Small Coronal Heating Events in an Active Region Core
Published 2023-01-01“…Here, we analyze the first coordinated observations of such events with the Interface Region Imaging Spectrograph (IRIS) and the CHROMospheric Imaging Spectrometer (CHROMIS), at the Swedish 1 m Solar Telescope (SST), which provided extremely high spatial resolution and revealed chromospheric brightenings with spatial dimensions down to ∼150 km. …”
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