Observations of time dependent periodicity within the coronal hole boundary

Physics

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Solar Coronal Holes

Scientific paper

High time resolution (≍13 sec cadence) Solar and Heliospheric Observatory (SOHO) Coronal Diagnostic Spectrometer (CDS) Grazing Incidence Spectrometer (GIS) time series data is analysed for evidence of quasi-periodic variability in the solar corona. The observations are obtained from a GIS study of a coronal hole boundary region taken in October 1997. A wavelet analysis is applied to EUV emission lines covering a temperature range of log Te = 5.3-6.1K. Wavelet analysis allows the frequency and temporal information of any periods present within the data to be analysed. Observations are presented of a time dependent periodicity positioned over a chromospheric network position located at the boundary position of a coronal hole.

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