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IRIS-6:  The Chromosphere
IRIS-6: The Chromosphere

20–23 Jun 2016
AlbaNova University Centre
Europe/Stockholm timezone

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Details for M. Carlsson

Author in the following contributions

  • Emergence of granular-sized magnetic bubbles through the solar atmosphere: the path to the transition region
  • Flocculent flows in the chromosphere observed with SST and IRIS
  • Observational consequences of ion-neutral effects in the low solar atmosphere
  • Penumbral micro-jet studies: automated detections and simulations
  • Insights into energy transport and heating in non-flaring active regions from IRIS observations
  • Probing the solar chromosphere with ALMA
  • 3D non-LTE formation of the He I 10830 line based on 3D simulations
  • Measuring energy flux of chromospheric waves in the magnetic elements by using IRIS
  • The OI / CI Line Ration in Solar Flares
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