Inverted-Y shaped jets near the solar limb show sustained red-blue H-alpha line asymmetries indicating bi-directional flows, supporting their origin in photospheric magnetic reconnection.
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Spatially resolved signatures of bi-directional flows observed in inverted-Y shaped jets
Inverted-Y shaped jets near the solar limb show sustained red-blue H-alpha line asymmetries indicating bi-directional flows, supporting their origin in photospheric magnetic reconnection.