----
EIS continues calibration operation (eg. [REGCAL071|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/studyeis/studydef/study_000027.def.txt]/[REGCAL072|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/studyeis/studydef/study_000028.def.txt]) to generate hot and warm pixels maps for [EIS_PREP|Eis_prep] routine use: e.g. to mark the hot/warm pixel positions and smooth the values on those positions. 

The hot/warm pixels maps are distributed with [SolarSoft|http://www.mssl.ucl.ac.uk/surf/surfsolarsoft.html] under [hinode/eis/data/cal|http://sohowww.nascom.nasa.gov/solarsoft/hinode/eis/data/] branch.

Before EIS launch, the CCD read-out section was assumed in the __middle 512 rows of the CCD__. That means [EIS_PREP|Eis_prep] only needs hot/warm pixels maps of middle section of CCDs.

However, in post-launch phase, the top and bottom of the CCDs were introduced to cover __whole CCDs area__ (ie. ''Y-axis: 0-1023 rows, X-axis: 0-4095 columns''). Thus hot/warm pixels maps for EIS CCDs have been generated accordingly as top and bottom maps (in detail: [REGCAL072|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/studyeis/studydef/study_000028.def.txt] study for top of CCDs and [REGCAL071|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/studyeis/studydef/study_000027.def.txt] study for bottom). The [EIS_PREP|Eis_prep] routine has also changed in order to use top and bottom hot/warm pixels maps.

%%information
The following paragraphs are a little bit deep in details. If you don't know what is talking about, that's fine, just ignore it and use EIS software as usual. But in case you are interesting in this topic, here are some technical descriptions: 
%%

The EIS camera electronics __do not__ readout CCD ''row 0'' in the y-direction (this is due to how the electronics work, row 0 is always discarded), so for the bottom of the CCDs EIS camera readout from row 1 to row 512 (inclusive), and for the top the camera readout from row 512 to row 1023 (inclusive).

So we can see there is an overlap at the 512th row, ie.:

|Bottom half: |row 1 -- %%(color:#cc0000;)row 512%%
|Top Half: |%%(color:#cc0000;)row 512%% -- row 1023


{{"The overlapping row (512) is there because the MDP requires that data to be a multiple of 8 in both the X and Y directions. Rows 1 to 511 is not a multiple of 8, hence we have to read rows 1 to 512 (inclusive). For the top half we must read 512 for 512 (i.e. rows 512 to 1023), hence the overlap in row 512."}}


-- Jian Sun (2008-10-17)

----


----

The __middle 512 rows__ of the CCDs were used at the beginning of the mission until January 2008 when the change was made to read-out the __full CCD height (1024 rows)__.
The hot and warm pixel maps are for the middle 512 rows until 18th January 2008. From the 19th January 2008 onwards the hot and warm pixel maps are for the full CCD height (split into the top 512 rows and bottom 512 rows). 

--[LouisaBradley|http://null], 13-Aug-2009