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Showing 1 to 2 of 2 for “"Solar transition region"”.

  1. Catastrophic cooling in solar coronal loops : thermal instability as a road to complex evolution

    … have revealed the highly dynamic nature of the solar corona and enabled us to study physical processes in the outer atmosphere of our mother star in great detail. This thesis deals with dynamic processes in coronal loops, i.e. magnetic structures which may be thought of as the elementary …

    freiburg-diss Repository record for Catastrophic cooling in solar coronal loops : thermal instability as a road to complex evolution (opens in a new tab)

  2. Modelling line emission in the lower solar atmosphere

    The transition region in the solar atmosphere bridges the lower temperature, higher density chromosphere at the base with the tenuous, high temperature plasma in the corona. It undergoes a change in temperature from 25000K to about 600000K. Plasma conditions mean that fundamentally different models …

    cambridge Repository record for Modelling line emission in the lower solar atmosphere (opens in a new tab)