Browsing by Author "Mason, Helen E."

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    Active Region Moss: Doppler Shifts from Hinode/EIS
    (2012-05-05) Tripathi, Durgesh; Mason, Helen E.; Klimchuk, James A.
    Studying the Doppler shifts and the temperature dependence of Doppler shifts in moss regions can help us understand the heating processes in the core of the ac- tive regions. In this paper we have used an active region observation recorded by the Extreme-ultraviolet Imaging Spectrometer (EIS) onboard Hinode on 12-Dec- 2007 to measure the Doppler shifts in the moss regions. We have distinguished the moss regions from the rest of the active region by de ning a low density cut-o as derived by Tripathi et al. (2010). We have carried out a very careful analy- sis of the EIS wavelength calibration based on the method described in Young, O'Dwyer and Mason (2012). For spectral lines having maximum sensitivity be- tween log T = 5:85 and log T = 6:25 K, we nd that the velocity distribution peaks at around 0 km s􀀀1 with an estimated error of 4􀀀5 km s􀀀1. The width of the distribution decreases with temperature. The mean of the distribution shows a blue shift which increases with increasing temperature and the distribution also shows asymmetries towards blue-shift. Comparing these results with observables predicted from di erent coronal heating models, we nd that these results are consistent with both steady and impulsive heating scenarios. However, the fact that there are a signi cant number of pixels showing velocity amplitudes that exceed the uncertainty of 5 km s􀀀1 is suggestive of impulsive heating. Clearly, further observational constraints are needed to distinguish between these two heating scenarios.
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    Active Region Moss: Doppler Shifts from Hinode/EIS Observations
    (2012-04-04) Tripathi, Durgesh; Mason, Helen E.; Kelimchuk, Jams A
    Studying the Doppler shifts and the temperature dependence of Doppler shifts in moss regions can help us understand the heating processes in the core of the ac- tive regions. In this paper we have used an active region observation recorded by the Extreme-ultraviolet Imaging Spectrometer (EIS) onboard Hinode on 12-Dec- 2007 to measure the Doppler shifts in the moss regions. We have distinguished the moss regions from the rest of the active region by de ning a low density cut-o as derived by Tripathi et al. (2010). We have carried out a very careful analy- sis of the EIS wavelength calibration based on the method described in Young, O'Dwyer and Mason (2012). For spectral lines having maximum sensitivity be- tween log T = 5:85 and log T = 6:25 K, we nd that the velocity distribution peaks at around 0 km s􀀀1 with an estimated error of 4􀀀5 km s􀀀1. The width of the distribution decreases with temperature. The mean of the distribution shows a blue shift which increases with increasing temperature and the distribution also shows asymmetries towards blue-shift. Comparing these results with observables predicted from di erent coronal heating models, we nd that these results are consistent with both steady and impulsive heating scenarios. However, the fact that there are a signi cant number of pixels showing velocity amplitudes that exceed the uncertainty of 5 km s􀀀1 is suggestive of impulsive heating. Clearly, further observational constraints are needed to distinguish between these two heating scenarios.
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    Heating and Dynamics of Solar Active Regions: Observations
    (2014-12-11) Mason, Helen E.; Del Zanna, Giulio; Klimchuk, Jim; Tripathi, Durgesh; Subramanian, Srividya; Gupta, Girjesh