Viggo Haraldson Hansteen

Bilde av Viggo Haraldson Hansteen
English version of this page
Telefon +47 22856120
Brukernavn
Besøksadresse Sem Sælands vei 13 0371 Oslo
Postadresse Postboks 1029 0315 Oslo

Se Viggo Hansteens engelske profil for mer informasjon.

Emneord: Astronomi og astrofysikk, Solfysikk

Publikasjoner

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  • Hansteen, Viggo Haraldson & Spilde, Ingrid (2022). Norske forskere skal lage romfartøy for NASA. [Avis]. forskning.no.
  • Hansteen, Viggo Haraldson (2021). Heating the outer layers of the Sun: braiding, flux emergence, and episodic events.
  • Hansteen, Viggo Haraldson (2021). Flux emergence in the Quiet Sun and its implications for chromospheric/coronal heating.
  • Hansteen, Viggo Haraldson (2021). Numeriske Modeller av Sola . Astronomi. ISSN 0802-7587. s. 24–24.
  • Hansteen, Viggo (2020). IRIS: heating of the solar chromosphere, Ellerman Bombs and UV bursts.
  • Hansteen, Viggo (2019). EBs and UV-bursts: reconnection at different heights in the solar atmosphere .
  • Hansteen, Viggo (2019). Ellerman Bombs and UV bursts - observations.
  • Hansteen, Viggo (2019). Ellerman Bombs and UV bursts, numerical simulations and IRIS observations.
  • Hansteen, Viggo (2019). Ellerman Bombs and UV bursts, reconnection at different heights in the chromosphere?
  • Hansteen, Viggo (2019). Ellerman Bombs and UV-bursts, a result of flux emergence.
  • Hansteen, Viggo (2019). Ellerman bombs and UV bursts in the solar chromosphere.
  • Hansteen, Viggo (2019). The FIP effect in the Chromosphere, Transition Region, Corona, and Solar Wind.
  • Kohutova, Petra; Antolin, Patrick; Popovas, Andrius; Szydlarski, Mikolaj Marcin & Hansteen, Viggo (2019). 3D radiative MHD simulations of coronal rain formation and evolution.
  • Hansteen, Viggo (2018). Ellerman bombs and UV bursts: reconnection at different atmospheric layers?
  • Hansteen, Viggo (2018). Ellerman bombs and UV bursts: reconnection at different atmospheric layers?
  • Hansteen, Viggo (2018). Modeling chromospheric heating and dynamics: What do we understand?
  • Hansteen, Viggo (2018). Chromospheric Dynamics and Heating Processes Ion-Neutral Effects in the Solar Chromosphere and Type II Spicules.
  • Hansteen, Viggo (2018). Ion neutral effects in the solar chromosphere and type II spicules.
  • Hansteen, Viggo (2018). The Heating of the Solar Chromosphere and Corona, What can "realistic" 3D Numerical Models teach us?
  • Hansteen, Viggo (2018). Mass and energy flows between the solar chromosphere, transition region and corona.
  • Mendes Domingos Pereira, Tiago; Carlsson, Mats; De Pontieu, Bart Walter & Hansteen, Viggo (2015). The Mg II lines as a diagnostic for heating in the lower chromosphere.
  • Carlsson, Mats & Hansteen, Viggo (2015). Vær og uvær på sola.
  • Hansteen, Viggo (2014). Heating of the upper chromosphere, transition region and corona.
  • Hansteen, Viggo (2014). Energy transport in the transition region and lower solar corona.
  • Hansteen, Viggo (2014). IRIS observations and 'realistic' 3D models of the solar chromosphere.
  • Hansteen, Viggo (2014). IRIS Observations of transition region 'unresolved fine structure'.
  • Hansteen, Viggo (2014). 'Realistic' 3D simulations of a small flare resulting from flux emergence.
  • Hansteen, Viggo (2014). Numerical modeling of the solar chromosphere and corona; what has been done? what should be done?
  • Hansteen, Viggo (2014). Numerical modeling of the outer solar atmosphere, with some examples from IRIS observations.
  • Hansteen, Viggo (2014). Simulating the transition region and corona: magnetic heating of the outer solar atmosphere.
  • Hansteen, Viggo (2014). Numerical modeling of the chromosphere and corona; what has been done? what should be done?
  • Kato, Yoshiaki; Steiner, Oskar; Hansteen, Viggo; Carlsson, Mats & Gudiksen, Boris Vilhelm (2014). Chromospheric and Corona Wave Generation in Flux Tubes.
  • Kato, Yoshiaki; De Pontieu, Bart Walter; Martinez-Sykora, J.; Hansteen, Viggo; Pereira, Tiago Mendes Domingos & Leenaarts, Jorritt [Vis alle 7 forfattere av denne artikkelen] (2014). Measuring energy flux of magneto-acoustic wave in the magnetic elements by using IRIS.

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Publisert 3. nov. 2010 15:20 - Sist endret 19. apr. 2022 13:38