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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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