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Showing 1 to 2 of 2 for “"Coronal lines"”.

  1. The variation of coronal holes with solar cycle

    Coronal holes are commonly known to be the source of the open magnetic flux and the high-speed solar wind. In EUV and X-ray emission lines, coronal holes are seen as the regions with reduced emission due to lower temperatures and electron density than the surrounding quiet sun. Observing the …

    cent-lancashire Repository record for The variation of coronal holes with solar cycle (opens in a new tab)