Search
Now showing items 401-500 of 1306
(Master thesis / Masteroppgave, 2019)
Due to the accelerated expansion of the visible Universe, the Symmetron has been proposed as a modification of the standard Einstein field equations. I investigate the feasibility of the Symmetron in light of radial ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
We present the first spatially resolved analysis of rest-frame optical and UV imaging and spectroscopy for a lensed galaxy at z = 2.39 hosting a Seyfert active galactic nucleus (AGN). Proximity to a natural guide star has ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Line-intensity mapping is an emerging field of observational work, with strong potential to fit into a larger effort to probe large-scale structure and small-scale astrophysical phenomena using multiple complementary ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Active region moss—the upper transition region of hot loops—was observed exhibiting rapid intensity variability on timescales of order 15 s by Testa et al. in a short time series (~150 s) data set from Hi-C (High-resolution ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
We investigate the diagnostic potential of the spectral lines at 850 nm for understanding the magnetism of the lower atmosphere. For that purpose, we use a newly developed 3D simulation of a chromospheric jet to check the ...
(Journal article / Tidsskriftartikkel / AcceptedVersion; Peer reviewed, 2018)
A simple magnetized plasma torus is modeled by using a 'top-hat' density variation. The benefit of this simplification is an exactly solvable model, allowing for a few additions, such as an externally maintained parabolic ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
The intergalactic medium (IGM) plays an important role in the formation and evolution of galaxies. Recent developments in upcoming radio telescopes are starting to open up the possibility of making a first direct detection ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Analytical models for the statistical distribution of the gut content of fish larvae in a turbulent ocean environment are compared to data obtained in a field experiment. The proposed model allows the nutrition state and ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
We infer the properties of massive star populations using the far-ultraviolet stellar continua of 61 star-forming galaxies: 42 at low redshift observed with the Hubble Space Telescope and 19 at z ~ 2 from the MegaSaura ...
(Master thesis / Masteroppgave, 2019)
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 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 ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Magnetic bright points (MBPs) are small-scale magnetic elements ubiquitous across the solar disc, with the prevailing theory suggesting that they form due to the process of convective collapse. Employing a unique full ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Context: The solar chromosphere and the lower transition region are believed to play a crucial role in the heating of the solar corona. Models that describe the chromosphere (and the lower transition region), accounting ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Ellerman bombs are transient brightenings in the wings of Hα 6563 Å that pinpoint photospheric sites of magnetic reconnection in solar active regions. Their partial visibility in the 1600 Å and 1700 Å continua registered ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Manganese (Mn) is a key Fe-group element, commonly employed in stellar population and nucleosynthesis studies to explore the role of SN Ia. We have developed a new non-local thermodynamic equilibrium (NLTE) model of Mn, ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
© 2017 American Physical Society
(Master thesis / Masteroppgave, 2006)
Two galaxy clusters, Abell 1351 and Abell 1995, are examined using weak gravitational lensing
techniques. Mass maps are created, and the clusters' density and shear profiles are compared to
theoretical predictions.
Gravitational ...
(Master thesis / Masteroppgave, 2011)
The existence of dark matter is a well established fact both due to galaxy rotation curves and also due to the CMB temperature anisotropies and the matter power spectra. According to the $\Lambda$CDM model, the so called ...
(Master thesis / Masteroppgave, 2010)
In this thesis the correlation between star formation and dynamical state of a statistical well defined selection of galaxy clusters have
been studied. From simulations and theory it is expected strong
correlations between ...
(Master thesis / Masteroppgave, 2007)
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
The European Space Agency’s Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
We describe the all-sky Planck catalogue of clusters and cluster candidates derived from Sunyaev-Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite observations. The catalogue contains 1227 ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
The dust-Hi correlation is used to characterize the emission properties of dust in the diffuse interstellar medium (ISM) from far infrared wavelengths to microwave frequencies. The field of this investigation encompasses ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
Anomalous microwave emission (AME) is believed to be due to electric dipole radiation from small spinning dust grains. The aim of this paper is a statistical study of the basic properties of AME regions and the environment ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
Using Planck data combined with the Meta Catalogue of X-ray detected Clusters of galaxies (MCXC), we address the study of peculiar motions by searching for evidence of the kinetic Sunyaev-Zeldovich effect (kSZ). By ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Minuit). This allows a refinement of the ΛCDM best-fit solution with respect to previously-released results, and the ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
Our velocity relative to the rest frame of the cosmic microwave background (CMB) generates a dipole temperature anisotropy on the sky which has been well measured for more than 30 years, and has an accepted amplitude of ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
We describe the processing of the 531 billion raw data samples from the High Frequency Instrument (HFI), which we performed to produce six temperature maps from the first 473 days of Planck-HFI survey data. These maps ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
We discuss the methods employed to photometrically calibrate the data acquired by the Low Frequency Instrument on Planck. Our calibration is based on a combination of the orbital dipole plus the solar dipole, caused ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
The Planck High Frequency Instrument (HFI) spectral response was determined through a series of ground based tests conducted with the HFI focal plane in a cryogenic environment prior to launch. The main goal of the spectral ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological results. We give an overview of the main ...
(Journal article / Tidsskriftartikkel / AcceptedVersion; Peer reviewed, 2014)
The Euclid mission objective is to understand why the expansion of the Universe is accelerating by mapping the geometry of the dark Universe by investigating the distance-redshift relationship and tracing the evolution of ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
We present the implications for cosmic inflation of the Planck measurements of the cosmic microwave background (CMB) anisotropies in both temperature and polarization based on the full Planck survey, which includes more ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
The Planck full mission cosmic microwave background (CMB) temperature and E-mode polarization maps are analysed to obtain constraints on primordial non-Gaussianity (NG). Using three classes of optimal bispectrum estimators ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
This paper presents a study of the integrated Sachs-Wolfe (ISW) effect from the Planck 2015 temperature and polarization data release. This secondary cosmic microwave background (CMB) anisotropy caused by the large-scale ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
We use Planck data to detect the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) effect and the infrared emission from the galaxies that make up the the cosmic infrared background (CIB). We first perform a ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
We have constructed all-sky Compton parameters maps, y-maps, of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 30 to 857 GHz frequency channel maps from ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
© 2017 American Physical Society
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
We present constraints on cosmological parameters using number counts as a function of redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The PSZ is selected through the signature of the ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
This paper presents an all-sky model of dust emission from the Planck 353, 545, and 857 GHz, and IRAS 100 μm data. Using a modified blackbody fit to the data we present all-sky maps of the dust optical depth, temperature, ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
We discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part of the spectrum is dominated by free-free and spinning dust emission, whereas ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
The new cosmic microwave background (CMB) temperature maps from Planck provide the highest-quality full-sky view of the surface of last scattering available to date. This allows us to detect possible departures from the ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
We present cluster counts and corresponding cosmological constraints from the Planck full mission data set. Our catalogue consists of 439 clusters detected via their Sunyaev-Zeldovich (SZ) signal down to a signal-to-noise ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2015)
The Planck survey provides unprecedented full-sky coverage of the submillimetre polarized emission from Galactic dust. In addition to the information on the direction of the Galactic magnetic field, this also brings new ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
We describe the detection, interpretation, and removal of the signal resulting from interactions of high energy particles with the Planck High Frequency Instrument (HFI). There are two types of interactions: heating of the ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
This paper presents the characterization of the in-flight beams, the beam window functions, and the associated uncertainties for the Planck Low Frequency Instrument (LFI). Knowledge of the beam profiles is necessary for ...
(Master thesis / Masteroppgave, 2015)
Magnetic bright points (MBPs) are small-scale (generally kG) magnetic features, ubiqui- tous in the lower solar atmosphere, and are a manifestation of solar magnetism. They represent the cross-sections of thin flux tubes ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2020)
ABSTRACT
We present high spatial resolution observations of short-lived transients, ribbons and jet-like events above a pore in Ca ii H images where fine structure, like umbral dots, light bridges and penumbral ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Context. Coronal rain consists of cool plasma condensations formed in coronal loops as a result of thermal instability. The standard models of coronal rain formation assume that the heating is quasi-steady and localised ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
The quintessence model is one of the simplest and better known alternatives to Einstein’s theory for gravity. The properties of the solutions have been studied in great detail in the background, linear and non-linear ...
(Journal article / Tidsskriftartikkel / AcceptedVersion; Peer reviewed, 2019)
While the origin and composition of dark matter and dark energy remains unknown, it is possible that they might represent two manifestations of a single entity, as occurring in unified dark sector models. On the other hand, ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Modified gravity (MG) theories aim to reproduce the observed acceleration of the Universe by reducing the dark sector while simultaneously recovering General Relativity (GR) within dense environments. Void studies appear ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
During a solar flare, it is believed that reconnection takes place in the corona followed by fast energy transport to the chromosphere. The resulting intense heating strongly disturbs the chromospheric structure and induces ...
(Master thesis / Masteroppgave, 2019)
Investigating properties of vortices formed in the superfluid dark matter picture, along with the parameter space of the model.
(Journal article / Tidsskriftartikkel / AcceptedVersion; Peer reviewed, 2019)
During the epoch of reionization, neutral gas in the early Universe was ionized by hard ultraviolet radiation emitted by young stars in the first galaxies. To do so, ionizing ultraviolet photons must escape from the host ...
(Journal article / Tidsskriftartikkel / AcceptedVersion; Peer reviewed, 2019)
Future Cosmic Microwave Background (CMB) satellite missions aim at using the B-mode polarisation signal to measure the tensor-to-scalar ratio r with a sensitivity σ(r) of the order of ≤ 10-2. Small uncertainties in the ...
(Doctoral thesis / Doktoravhandling, 2016)
For over a hundred years Einstein’s theory of gravity has reigned supreme as the best theory for explaining how gravity functions in our Universe, however during the last 30 years the limitations of the theory have started ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
To extract the information that the Mg ii NUV spectra (observed by the Interface Region Imaging Spectrograph) carry about the chromosphere during solar flares, and to validate models of energy transport via model–data ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2020)
Context. Penumbral microjets (PMJs) are short-lived, jet-like objects found in the penumbra of sunspots. They were first discovered in chromospheric lines and have later also been shown to exhibit signals in transition ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
Reproduced with permission from Astronomy & Astrophysics, © ESO 2017
(Journal article / Tidsskriftartikkel / AcceptedVersion; Peer reviewed, 2019)
We consider a cosmological model with an interaction between dark matter and dark energy which leaves the background cosmology unaffected and only affects the evolution of the perturbations. This is achieved by introducing ...
(Journal article / Tidsskriftartikkel / AcceptedVersion; Peer reviewed, 2019)
The evolution of the virial overdensity Δvir for ΛCDM and seven dynamical dark-energy models is investigated in the extended spherical collapse model (SCM). Here the virialization process is naturally achieved by introducing ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
We provide predictions of the yield of 7 < z < 9 quasars from the Euclid wide survey, updating the calculation presented in the Euclid Red Book in several ways. We account for revisions to the Euclid near-infrared ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Context. Sunspot observations in chromospheric spectral lines have revealed short-lived linear bright transients that are commonly referred to as penumbral microjets (PMJs). Details on the origin and physical nature of ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Since there is no known symmetry in nature that prevents a nonminimal coupling between the dark energy (DE) and cold dark matter (CDM) components, such a possibility constitutes an alternative to standard cosmology, with ...
(Doctoral thesis / Doktoravhandling, 2019)
Einstein's theory of general relativity is currently our best model for how gravity works. It can be used to predict motions of planets, the speed-up of clocks on GPS satellites, and gravitational waves. General relativity ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
The GOES X1 flare SOL2014-10-25T17:08:00 was a three-ribbon solar flare observed with the Interface Region Imaging Spectrograph (IRIS) in the near-UV (NUV) and far-UV. One of the flare ribbons crossed a sunspot umbra, ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
The escape of ionizing Lyman continuum (LyC) photons requires the existence of low-NH I sightlines, which also promote escape of Lyα. We use a suite of 2500 Lyα Monte-Carlo radiative transfer simulations through models of ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2020)
A new upper limit on the 21 cm signal power spectrum at a redshift of z ≈ 9.1 is presented, based on 141 h of data obtained with the Low-Frequency Array (LOFAR). The analysis includes significant improvements in spectrally ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Hinode is Japan’s third solar mission following Hinotori (1981–1982) and Yohkoh (1991–2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries three instruments: the Solar Optical Telescope, ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2020)
NASA’s Interface Region Imaging Spectrograph (IRIS) provides high-resolution observations of the solar atmosphere through ultraviolet spectroscopy and imaging. Since the launch of IRIS in June 2013, we have conducted ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
The volume of data being collected in solar physics has exponentially increased over the past decade and with the introduction of the Daniel K. Inouye Solar Telescope (DKIST) we will be entering the age of petabyte solar ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Eruptive flares (EFs) are associated with erupting filaments and, in some models, filament eruption drives flare reconnection. Recently, however, observations of a confined flare (CF) have revealed all the hallmarks of an ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
We report on quasar outflow properties revealed by analyzing more than 60 composite outflow spectra built from ~60,000 C iv absorption troughs in the SDSS-III/BOSS DR12QBAL catalog. We assess the dependences of the equivalent ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
We characterize, for the first time, type-II spicules in Ca II K 3934 Å using the CHROMIS instrument at the Swedish 1 m Solar Telescope. We find that their line formation is dominated by opacity shifts with the K3 minimum ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
Using the Eris zoom-in cosmological simulation of assembly of a Milky Way analogue, we study the chemical enrichment of stars due to accretion of metal-enriched gas from the interstellar medium (ISM) during the Galaxy's ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
© 2017. The American Astronomical Society. All rights reserved.
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
We compare 237 Lyman-α (Lyα) spectra of the MUSE-Wide survey to a suite of radiative transfer simulations consisting of a central luminous source within a concentric, moving shell of neutral gas, and dust. This six parameter ...
(Master thesis / Masteroppgave, 2018)
Analysing the state of the art, zoom-in simulation "Eris", we study the distribution, origins and kinematics of O~VI gas around star forming L* galaxies. A detailed comparison to observations from the COS-halo survey is ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
© 2017 American Institute of Physics.
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
Our ability to model the shapes and strengths of iron lines in the solar spectrum is a critical test of the accuracy of the solar iron abundance, which sets the absolute zero-point of all stellar metallicities. We use an ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
© 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
Solar “magnetic tornadoes” are produced by rotating magnetic field structures that extend from the upper convection zone and the photosphere to the corona of the Sun. Recent studies show that these kinds of rotating features ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
(Master thesis / Masteroppgave, 2018)
(Master thesis / Masteroppgave, 2018)
The nuclide 187Re beta-decays to 187Os with a half-life of approximately 41.6 Gyr. The long half-life and simple relation between 187Re and 187Os makes the ratio a good candidate for a cosmic clock. In order to "use the ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
Magnetic reconnection is thought to drive a wide variety of dynamic phenomena in the solar atmosphere. Yet, the detailed physical mechanisms driving reconnection are difficult to discern in the remote sensing observations ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
Future solar missions and ground-based telescopes aim to understand the magnetism of the solar chromosphere. We performed a supporting study in Quintero Noda et al. focused on the infrared Ca ii 8542 Å line and we concluded ...
(Master thesis / Masteroppgave, 2018)
The ''theory of dark matter superfluidity'' \cite{berezhiani2015theory} is reproduced in SI units with the inclusion of intermediate, and precise, steps in the calculations. By use of another measure of the mean interparticle ...
(Master thesis / Masteroppgave, 2018)
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
© 2017. The American Astronomical Society. All rights reserved.
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
We present rest-frame ultraviolet and optical spectroscopy of the brightest lensed galaxy yet discovered, at redshift z = 2.4. The source reveals a characteristic triple-peaked Lyman α profile that has been predicted in ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
We investigate the contribution of outer H i disks to the observable population of merging black hole binaries. Like dwarf galaxies, the outer H i disks of spirals have low star formation rates and lower metallicities than ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
Aims. Although observational data unequivocally point to the presence of chromospheres in red giant stars, no attempts have been made so far to model them using 3D hydrodynamical model atmospheres. We therefore compute an ...
(Journal article / Tidsskriftartikkel / AcceptedVersion; Peer reviewed, 2017)
line (121.6 nm). The instrument was successfully launched on 3 September 2015 and observations were conducted at the solar disc center and close to the limb during the five-minutes flight. In this article, the disc center ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
High-energy particles enter the solar atmosphere from Galactic or solar coronal sources, and produce ‘albedo’ emission from the quiet Sun that is now observable across a wide range of photon energies. The interaction of ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
The Multi-slit Solar Explorer (MUSE) is a proposed mission aimed at understanding the physical mechanisms driving the heating of the solar corona and the eruptions that are at the foundation of space weather. MUSE contains ...
(Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
Context. Thermal non-equilibrium (TNE) is a phenomenon that can occur in solar coronal loops when the heating is quasi-constant and highly-stratified. Under such heating conditions, coronal loops undergo cycles of evaporation ...