Study 000278:

Acronym: sta_loop_context_lo

Context raster to be used in conjunction with sta_loop_slot_lo

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.

Study summary:
Slit/slot: 2" slit
No of pointing positions: 59
Total spatial width: 120"
Pixels in solar-y: 248
Exposure time: 30 seconds
Cadence: 33 minutes 50 seconds
Compression: DPCM
Data rate: 11.7755 kbits/s
Data volume: 23644.07 kbits

Condition necessary to run and POINTING:

Occurence of a relatively quiescent
(non-flaring) coronal loop system either of the disk or limb. Involvement of,
at a minimum, Hindoe/EIS, SOHO/CDS and TRACE. Additional support from
Hinode/XRT and Hinode/SOT/FPP would be nice.

WARNING:

None