<The full description> Initial helioseismology observations with BFI (quiet Sun regions on January 1 and February 28, and sunspots on January 8 and May 2) have showed uniqueness and importance of these observations for helioseismology. These observations allow us to extend the time-distance helioseismology for much shorter wave travel distances and probe the subsurface layers in much greater detail. Also, simultaneous observations in two filters provide unique information about wave interaction with the atmospheric layers and magnetic fields, allowing us to obtain more knowledge about the wave physics and improve the quality of helioseismic inference. In addition, the SOT FG observations provide unique capability of measuring flows at high latitudes and polar regions. Joint observations with SOHO/MDI are particularly valuable.
However, our analysis of the FG data shows that the solar noise level in the FG data (G-band, blue continuum and CaII H) is higher than in the corresponding Dopplergram data. Thus, it is necessary to have longer time series for the helioseismology (time-distance) measurements. Our preliminary analysis shows that the FG data require 12-hour continuous runs with 1-min cadence for helioseismology analysis.
The SOHO/MDI continuous contact schedule for this year is the following: SOHO/MDI Future Continuous Contact Periods: ================================= (Jul 18-22 2007 MDI Continuous Contact) Sep 10 - Nov 11 2007 MDI 60-day Continuous Contact (Dec 26-30 2007 MDI Continuous Contact)
We propose to schedule Hinode helioseismology observations during these periods, particularly, during the 60-day continuous run.
At the beginning or at the end of this period we propose to schedule two joint observing runs with MDI data taken in the high-resolution mode. For the first run, both SOT/FG and MDI data will be taken in the MDI high-resolution field of view (tracking a quiet Sun region or a magnetic region). The required minimal length of these observations is 12 hours. For the second run, we propose to keep MDI in the hi-res mode and point SOT to a high-latitude regions for large-distance measurements, which will allow us to reach the tachocline and estimate the sensitivity of these measurements to the deep meridional flow. These measurements require 24-hour continuous run. Such two-point observation can be also made with MDI in the full-disk mode. These joint observations will also allow us to measure the subsurface rotation at high-latitudes.
During the 60-day continuous contact, we propose to schedule observations of active regions at different positions on the disk, preferably, of the same active region, following its evolution. These will allow us to investigate the inclined field effect in the MDI measurements and improve the inferences of the subsurface structure and flows for evolving active regions. In the case of the absence of active regions, tracking a quiet Sun region will provide for investigations of evolution of supergranulation, and, in particular, the wave-like behavior of supergranulation. Observations of a plage region will allow us to investigate scattering of acoustic and surface gravity waves on small-scale magnetic elements, and develop diagnostics of these elements by helioseismology. These observations require at least 12-hour long runs.
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