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- W165763167 abstract "Prominence cavities appear as circularly shaped voids in coronal emission over polarity inversion lines where a prominence channel is straddling the solar limb. The presence of chromospheric material suspended at coronal altitudes is a common but not necessary feature within these cavities. These voids are observed to change shape as a prominence feature rotates around the limb. We use a morphological model projected in cross-sections to fit the cavity emission in Hinode/XRT passbands, and then apply temperature diagnostics to XRT and SDO/AIA data to investigate the thermal structure. We find significant evidence that the prominence cavity is hotter than the corona immediately outside the cavity boundary. This investigation follows upon Thermal Properties of A Solar Coronal Cavity Observed with the X-ray Telescope on Hinode by Reeves et al., 2012, ApJ, in press." @default.
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- W165763167 date "2012-05-31" @default.
- W165763167 modified "2023-10-16" @default.
- W165763167 title "Morphology Of A Hot Prominence Cavity Observed with Hinode/XRT and SDO/AIA" @default.
- W165763167 hasPublicationYear "2012" @default.
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