Now showing items 276-295 of 518

  • Shimojo, M.; Bastian, T. S.; Hales, A. S.; White, S. M.; Iwai, K.; Hills, R. E.; Hirota, A.; Phillips, N. M.; Sawada, T.; Yagoubov, P.; Siringo, G.; Asayama, S.; Sugimoto, M.; Brajša, Roman; Skokic, I.; Barta, M.; Kim, S.; de Gregorio-Monsalvo, I.; Corder, S. A.; Hudson, H. S.; Wedemeyer, Sven; Gary, D. E.; De Pontieu, Bart Walter; Loukitcheva, M.; Fleishman, G. D.; Chen, B.; Kobelski, A.; Yan, Y. (Journal article / Tidsskriftartikkel / AcceptedVersion; Peer reviewed, 2017)
    This is a post-peer-review, pre-copyedit version of an article published in Solar Physics. The final authenticated version is available online at: http://dx.doi.org/10.1007/s11207-017-1095-2
  • Gjerløw, Eirik (Master thesis / Masteroppgave, 2010)
    The theory of inflation gives certain predictions for the amount of primordial gravitational waves compared to the amount of density perturbations. These predictions are, in principle, verifiable through observation of the ...
  • Leenaarts, Jorrit; Carlsson, Mats; Rouppe, Van Der Voort Luc (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2015)
    Observations of the solar chromosphere in the line core of the Hα line show dark elongated structures called fibrils that show swaying motion. We performed a three-dimensional radiation-MHD simulation of a network region ...
  • Hipólito-Ricaldi, William S.; vom Marttens, R.F.; Fabris, J.C.; Shapiro, I.L.; Casarini, Luciano (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2018)
    Reduced relativistic gas (RRG) is a useful approach to describe the warm dark matter (WDM) or the warmness of baryonic matter in the approximation when the interaction between the particles is irrelevant. The use of Maxwell ...
  • Færder, Øystein Håvard (Master thesis / Masteroppgave, 2012)
    The solar corona has a temperature of order 1 MK, which is almost 200 times the temperature of the underlying surface. This fact has puzzled solar physicists for more than six decades. As of today, most solar physicists ...
  • Andersen, Monica (Master thesis / Hovedoppgave, 2007)
    The goals of this thesis are to provide a general introduction to CMB fundamentals, give an overview of non-Gaussianity analysis, and to compare the sensitivities of a selection of tests (Minkowski functionals, skeleton ...
  • Skogsrud, Håkon; Rouppe, Van Der Voort Luc; De Pontieu, Bart Walter (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
    The Interface Region Imaging Spectrograph (IRIS) provides spectroscopy and narrow band slit-jaw (SJI) imaging of the solar chromosphere and transition region at unprecedented spatial and temporal resolutions. Combined with ...
  • Martinez-Sykora, Juan; De Pontieu, Bart Walter; Hansteen, Viggo; Rouppe van der Voort, Luc; Carlsson, Mats; Mendes Domingos Pereira, Tiago (Journal article / Tidsskriftartikkel / AcceptedVersion; Peer reviewed, 2017)
    In the lower solar atmosphere, the chromosphere is permeated by jets known as spicules, in which plasma is propelled at speeds of 50 to 150 kilometers per second into the corona. The origin of the spicules is poorly ...
  • Kanella, Charalambos (Doctoral thesis / Doktoravhandling, 2018)
    The identification of small-scale 3-D heating events in numerical simulations brought us a step closer to solve one of the biggest mysteries in astrophysics. The identification of small scale 3-D heating events in the ...
  • Skogsrud, Håkon; Rouppe, Van Der Voort Luc; De Pontieu, Bart Walter (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
    A dominant constituent in the dynamic chromosphere is spicules. Spicules at the limb appear as relatively small and dynamic jets that are observed to stick out everywhere. Many papers emphasize the important role spicules ...
  • Windhorst, Rogier A.; Timmes, F.X.; Wyithe, J. Stuart B.; Alpaslan, Mehmet; Andrews, Stephen K.; Coe, Daniel; Diego, Jose M.; Dijkstra, Mark; Driver, Simon P.; Kelly, Patrick L.; Kim, Duho (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2018)
    We summarize panchromatic Extragalactic Background Light data to place upper limits on the integrated near-infrared surface brightness (SB) that may come from Population III stars and possible accretion disks around their ...
  • Froment, Clara; Auchère, F.; Mikic, Z.; Aulanier, G.; Bocchialini, Karine; Buchlin, E.; Solomon, J.; Soubrie, E. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2018)
    Long-period EUV pulsations, recently discovered to be common in active regions, are understood to be the coronal manifestation of thermal nonequilibrium (TNE). The active regions previously studied with EIT/Solar and ...
  • Martinez-Sykora, Juan; Hansteen, Viggo; Gudiksen, Boris Vilhelm; Carlsson, Mats; De Pontieu, Bart Walter; Gošić, Milan (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 ...
  • Skogsrud, Håkon; Rouppe, Van Der Voort Luc; De Pontieu, Bart Walter; Mendes Domingos Pereira, Tiago (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2015)
    Spicules are ubiquitous, fast moving jets observed off-limb in chromospheric spectral lines. Combining the recently launched Interface Region Imaging Spectrograph with the Solar Dynamics Observatory and Hinode, we have a ...
  • Valberg, Pål (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 ...
  • Bose, Souvik; Nagaraju, K (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2018)
    The solar mean magnetic field (SMMF) is referred to as the disk-averaged line-of-sight (LOS) magnetic field that also reflects the polarity imbalance of the magnetic field on the Sun. The origin of the SMMF has been debated ...
  • Barrena, R.; Streblyanska, A.; Ferragamo, A.; Rubiño-Martín, J. A.; Aguado-Barahona, A.; Tramonte, D.; Génova-Santos, R. T.; Hempel, A.; Lietzen, H.; Aghanim, Nabila; Arnaud, M.; Böhringer, H.; Chon, G.; Démoclès, J.; Dahle, Håkon; Douspis, M.; Lasenby, A. N.; Mazzotta, P.; Melin, J. B.; Pointecouteau, E.; Pratt, G. W.; Rossetti, M.; van der Burg, R. F. J. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2018)
    We have identified new clusters and characterized previously unknown Planck Sunyaev–Zeldovich (SZ) sources from the first Planck catalogue of SZ sources (PSZ1). The results presented here correspond to an optical follow-up ...
  • Gjerløw, Eirik; Colombo, L. P. L.; Eriksen, Hans Kristian Kamfjord; Górski, Krzysztof M.; Gruppuso, A.; Jewell, J. B.; Plaszczynski, S; Wehus, Ingunn Kathrine (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2015)
    We revisit the problem of exact cosmic microwave background (CMB) likelihood and power spectrum estimation with the goal of minimizing computational costs through linear compression. This idea was originally proposed for ...
  • Mas Ribas, Lluis; Riemer-Sørensen, Signe; Hennawi, Joseph F; Miralda-Escudé, Jordi; O'Meara, John M.; Pérez-Ràfols, Ignasi; Murphy, Michael T.; Webb, John K. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2018)
    We present the first paper of the series Origin of Metals around Galaxies, which aims to explore the origin of the metals observed in the circumgalactic and intergalactic media. In this work we extract and build catalogs ...
  • Spilker, Andri Karoline Lunøe (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 ...