Study 000595:

ACRONYM:  TimeLag_QS

A sit-and-stare study for quiet-sun areas designed to investigate
properties of coronal heating using a systematic analysis of EUV
light curves known as the time-lag method.  Time-lag diagnostics
correlate relative maxima that occur in light curves of emission
lines formed at different temperatures to detect cooling trends
in the observed areas.

TARGET: quiet-sun areas
EXPOSURE TIME: 90s
SLIT         : 2"
RASTER: sit-and-stare
NO. OF EXPOSURES: 36
DURATION: 58m 15s
SLIT LENGTH: 184"
WINDOWS	   : 11
COMPRESSION: DPCM
DATA VOLUME: 36.5 Mbits

The wavebands are selected to observe the following lines:
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(1)  184.0-186.0:  Fe X 184.537, Fe VIII 185.213 (+Ni XVI 185.230);
(2)  187.5-189.0:  Fe XI 188.216 & 188.299, Fe IX 188.497;
(3)  194.4-195.8:  Fe VIII 194.661, Fe XII 195.119+195.179;
(4)  201.3-202.5:  Fe XIII 201.538 & 202.044
(5)  262.0-265.5:  Fe XVI 262.976, S X 264.231, Fe XIV 264.789;
(6)  268.0-270.0:  Mg VI 268.991, Fe XVII 269.420 & 269.886;
(7)  273.8-274.5:  Fe XIV 274.204;
(8)  275.0-277.0:  Si VII 275.361, Fe XVII 275.550; Mg V 276.579;
(9)  279.5-281.0:  O IV 279.631 & 279.933, Fe XVII 280.160+280.199,
                   Mg VII 280.742;
(10) 283.7-284.7:  Fe XV 284.163.

Pointing:
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The target should be quiet-sun area anywhere on the disk.

Instructions to planners:
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(1) Place the context study PRY_slot_context_v3 on the timeline first.
(2) Then append the TimeLag_QS study. Adjust the number of repeats
    to fill the available time slot, preferably with a minimum total
    duration of 3 or 4 hours.
(3) Then append the context study PRY_slot_context_v3 at the end of
    TimeLag_QS to complete the sequence.

Warning:
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None