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• W83895534 abstract "A blowout jet occurred within the south coronal hole on 2011 February 9 at 09:00 UT and was observed by the Atmospheric Imaging Assembly (AIA) and Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamics Observatory, and the EUV Imaging Spectrometer (EIS) and X-Ray Telescope (XRT) on board the Hinode satellite during coronal hole monitoring performed as part of Hinode Operations Program No. 177. Images from AIA show expanding, hot and cold loops from a small bright point with plasma ejected in a curtain up to 30 Mm wide. The initial intensity front of the jet has a projected velocity of 200 km/s, and line-of-sight velocities measured by EIS are between 100 and 250 km/s. The jet plasma has a density of 2.7 x 10^8 cm^-3, and a temperature of 1.4 MK. During the event a number of bright kernels are seen at the base of the bright point. The kernels have sizes of 1000 km, are variable in brightness, and have lifetimes of 1-15 mins. A XRT filter ratio yields temperatures of 1.5-3.0 MK for the kernels. The bright point existed for at least 10 hours, but disappeared within 2 hours after the jet, which lasted for 30 mins. HMI data reveal converging photospheric flows at the location of the bright point, and the mixed polarity magnetic flux cancels over a period of four hours either side of the jet." @default.
• W83895534 created "2016-06-24" @default.
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• W83895534 date "2013-09-27" @default.
• W83895534 modified "2023-09-27" @default.
• W83895534 title "SDO and Hinode observations of a blowout jet in a coronal hole" @default.
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