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- W1628483278 abstract "We present an analysis of time series data acquired with the SUMER spectrograph on SoHO in coronal hole regions, being particularly interested to nd the fast solar wind origins as low as possible in the solar atmosphere. We study the temporal evolution of the magnetic network as seen in dierent layers in the transition region (TR). Our results indicate that, in lines originating from low to medium TR temperatures, we nd variations of intensity with periods of 20 min or longer which are made up of short time brightenings that repeat every 5 min. In these observations, we have not observe the fast solar wind starting as a steady outow in the TR. Instead, we see bursts of short time brightenings, some of which represent bi-directional jets of dierent scales that, because of the open eld structure they meet in coronal holes, we suggest they could pump plasma into the corona." @default.
- W1628483278 created "2016-06-24" @default.
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- W1628483278 date "2004-12-01" @default.
- W1628483278 modified "2023-09-27" @default.
- W1628483278 title "TEMPORAL EVOLUTION OF THE MAGNETIC NETWORK IN POLAR CORONAL HOLES" @default.
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