Study 000250:

ACRONYM: STA_loop_slot_v2

Objective:
----------
to investigate the morphology of coronal loops which support longitudinal
intensity perturbations, the nature of the (quasi-) periodic driver and
the evolution of the perturbation as they travel through the different
temperature regions of the solar atmosphere.

Conditions Necessary to Run & Pointing:
---------------------------------------
Occurrence of a relatively quiescent (non-flaring) coronal loop system
either on the disk or limb. Involvement of, at a minimum, Hinode/EIS,
SOHO/CDS and TRACE. Additional support from Hinode/XRT and Hinode/SOT/FPP

Study summary
-------------------
Slit/slot: 40" slot
No of pointing positions: 0
Total spatial width: 40"
Pixels in solar-y: 248
Exposure time: 20 seconds
No. of exposures: 100
Cadence: 38 minutes 39 seconds
Data rate:  3.9 kbits/s

Compression: JPG75

WARNING:

None