%%warning The following section %%(color:#5555ff;)in blue%% was written prior to Hinode changing from X-band to S-band telemetry. Therefore, please bear this in mind.

However, the discussion of the scientific type of observation is still valid, and many new studies have been designed for the new telemetry situation. See [Study4LowDataVolume] for some more examples.
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%%(color:#5555ff;)This is a list of some studies that I've either designed or used that I think are generally useful.

__PRY_footpoints_v2__

Consists of two rasters, the first being a 40" slot context raster (600"x512" field of view). The narrow slit raster has a moderate cadence (23mins), wide range of emission lines, 100x240 arcsec^2 field of view. Uses 2" slit.

__Diag_40x180_s0_30s__

Similar to above, but more focussed on hot plasma, and uses 1" slit. Also has a 40" slot context raster. 

__AR_velocity_map_v2__

This is a large field of view (460"x384"), 1" slit raster suitable for diagnostic and velocity maps of ARs. The duration is 5hr 40mins and so fits in the inter-synoptic slots nicely.



__CAM_ARTB_RHESSI_b_2__

A high cadence (4mins) raster covering 40x120 arcsec%%sup 2%% with many diagnostic lines, and a 10s exposure time. It is a good diagnostic study for studying flaring activity in active regions. 

!! Eclipse season

During the eclipse season, it is possible to run studies with a higher data rate than normal during the day period, leaving the night periods empty on the timeline. Some studies that are suitable for running in this way are:

__HPW008_FULLCCD_RAST__

Takes full CCD spectra over a 128x128 arcsec^2 area, with 25s exposure times, and 1" slit. Duration: 1 hour. Data rate: 96 kbits/s.

__Eclipse_raster1__


Takes over 60% of the EIS spectral bands (mainly dropping low sensitivity areas), and covers 105x178 arcsec^2 area, with 40s exposures, and 1" slit. Duration: 1hr 22mins. Data rate: 50 kbits/s. Includes a slot context raster.


Peter Young, 13-Sep-2007%%