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• W2889630620 abstract "Jets of all sizes are frequent magnetically channeled narrow eruptions. They occur in various solar environments: quiet regions, coronal holes and active regions. All coronal jets observed in UV, EUV and X-ray images show a bright spire with a base brightening, also known as jet bright point (JBP). Recent studies show that coronal jets are driven by small-scale filament eruptions. We found in on disk quiet regions and coronal holes that coronal jets originate at a neutral line between dominant-polarity flux and a patch of canceling minority-polarity flux." @default.
• W2889630620 created "2018-09-27" @default.
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• W2889630620 date "2018-06-25" @default.
• W2889630620 modified "2023-09-22" @default.
• W2889630620 title "IRIS and SDO Observations of Solar Jetlets Resulting from Flux Cancelation" @default.
• W2889630620 hasPublicationYear "2018" @default.
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