On the Relationship Between Small-Scale Sigmoids and Coronal Jets

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Observations from SDO/AIA and Hinode/XRT are used to study the structure of bright points sources of coronal jets. Several jets are found to emanate from S-shaped bright points suggesting the presence of coronal micro-sigmoids. These structures may provide explanation for numerous characteristics of coronal jets, such as helical structures and jet types.

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