Temporal Variability of Active Region Outflows
arXiv:1008.4730 · doi:10.1088/0004-637X/730/1/37
Abstract
Recent observations from the Extreme-ultraviolet Imaging Spectrometer (EIS) on board Hinode have shown that low density areas on the periphery of active regions are characterized by strong blue-shifts at 1 MK. These Doppler shifts have been associated with outward propagating disturbances observed with Extreme-ultraviolet and soft X-ray imagers. Since these instruments can have broad temperature responses we investigate these intensity fluctuations using the monochromatic imaging capabilities of EIS and confirm their 1 MK nature. We also find that the Fe XII 195.119 A blue shifted spectral profiles at their footpoints exhibit transient blue wing enhancements on timescales as short as the 5 minute cadence. We have also looked at the fan peripheral loops observed at 0.6 MK in Si VII 275.368 A in those regions and find no sign of the recurrent outward propagating disturbances with velocities of 40 - 130 km/s seen in Fe XII. We do observe downward trends (15 - 20 km/s) consistent with the characteristic red-shifts measured at their footpoints. We, therefore, find no evidence that the structures at these two temperatures and the intensity fluctuations they exhibit are related to one another.
Movies are available at http://tcrb.nrl.navy.mil/~iuu/out/papers/2010_flows/. To be submitted to ApJ
References in corpus (4)
- High precision density measurements in the solar corona: I. Analysis methods and results for Fe XII and Fe XIII
- Flows and Non-thermal Velocities in Solar Active Regions Observed with the Extreme-ultraviolet Imaging Spectrometer on Hinode: A Tracer of Active Region Sources of Heliospheric Magnetic Fields?
- The Temperature Dependence of Solar Active Region Outflows
- Flows and Motions in Moss in the Core of a Flaring Active Region: Evidence for Steady Heating
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