Study 000313:

ACRONYM: dot+eis:mic_fib_sit (HOP 88)

Key Note:
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Because of a concern about a possible artifacts (possible introducing of noise)
associated with using JPEGs on low count rate data
(short exposures) (e.g. 10s), the following is recommended: 

1) If more TM is available, try to switch the DC on the timeline to DPCM
(requires just over 200 Mbits)
2) else try JPEG95
3) Otherwise keep the default DC (JPEG90)

This applies to both context and SNS studies.

STUDY TITLE:
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Solar microflares and network dynamic fibrils - relevance for coronal 
heating and mass supply

TARGET/POINTING:
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QS at the disk center (or)
AR (or its remnants) near the disk center

Raster specific:
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EXPOSURE TIME: 10s
SLIT: 2"
COMPRESSION: JPEG90 (default, see key note above)

USE/INSTRUCTIONS TO PLANNERS:
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The following sequence (1 to 3) should be repeated **TWICE**

1. Run dot+eis:mic_fib_con (context raster), number of raster repeats:  3 

total time: 14m30s

2. Run dot+eis:mic_fib_sit (SNS), number of raster repeats: 11

total time: 1h50m

**** slit placed at the X-center of the context raster ****

3. Run dot+eis:mic_fib_con (context raster), number of raster repeats:  3

total time: 14m30s

**** raster positioned as in the previous context (step 1) ****

Steps 1 to 3 total time: 2h19m

*********** Total HOP time **********

2 x 2h19m (Data volume: 2 x 51.23 MBits - Using JPEG95)

There could be an interruption between the previous and following study
allowing any instrument specific upload of tables, etc. Adjust the number
of repeats so as to finish before the OBS table uplink. For example,
if it is only possible to do 3 of the 11 SNS, schedule the remaining 8
following the OBS table uplink.

SCHEDULING OF THE PROGRAM:
--------------------------

PREFERRED OBSERVING TIME SLOT (~DOT/LaPalma): ~09 - ~13 UT

Warning:
--------

As usual, avoid SAAs if possible (DC degradation)