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Eis40June...nobody

Difference between version and

At line 1 changed 2 lines
[{ALLOW view jsun,ms2,DaveWilliams,LouiseHarra}]
[{ALLOW edit jsun,ms2,DaveWilliams,LouiseHarra}]
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
At line 63 added 3 lines
[click here to see EIS data list | https://vsolar.mssl.ucl.ac.uk/SolarB/ThumbsConn_js2.jsp?startdate=2008-01-07+00%3A52&enddate=2008-01-08+00%3A52&Instrument=Thumbnail&Instrument=Movie&Submit=Submit+entry]
At line 108 changed one line
* Due to having only two projections (order_0 & 1 images), the deconvolution is not good enough to reveal small or changed-rapidly structures. But considering 1" scanning usually takes long time to finish (in this case, 80 minutes for a small FOV), it is also not good enough to observe fast-changing features. So it looks the slot deconvolution will be useful for, at leat, synoptic review(?)
* Due to having only two projections (order_0 & 1 images), the deconvolution is not good enough to reveal small or changed-rapidly structures. But considering 1" scanning usually takes long time to finish (in this case, 80 minutes for a small FOV), it is also not good enough to observe fast-changing features. So it looks the slot deconvolution would be useful for, for example, synoptic velocity review(?)
At line 116 changed one line
- Instrument response is different, eg, PSF
- Instrument response is different, eg, response fuctions & PSF
At line 118 changed one line
- Spectral resolution is different, eg, TRACE covers wider for FeXII 195 line compared with EIS 195 line (according to drw)
- Spectral resolution is different, eg, TRACE covers wider range for FeXII 195 line compared with EIS 195 line (according to drw)
At line 120 changed one line
- images from TRACE & EIS may have different distortions and alias, which makes alignment difficult
- images from TRACE & EIS may have different distortions and alias, which makes alignment difficulties
At line 145 added 32 lines
\\
EIS study 235 – PRY_slot_context for large slot context
__Details__:
40” slot, 14 scans, spectral window width: 48pix, Y-height: 512pixs\\
exposure time: 10s, duration: 3m6s, 15 lines\\
Data obtained on 07-Jan-2008, 5 fits files\\
TRACE 195A data is used as order-0 image: tri20080107.0600
__Details__:
FeXII 195A line, 1K by 1K size, 29 frames\\
processed by standard TRACE routines\\
[{Image src='images/eis40/eis_trace_flist.png'}]
\\
TRACE movie from tri200807107.0600 (Red color-table, log scale applied)
[click here | https://vsolar.mssl.ucl.ac.uk/eiswiki/images/eis40/trace20080107.0600.mov]
\\
EIS intensity and reconstructed velocity movie (Red color-table, log scale applied)\\
5 frames, time range: 07-Jan-2008 06:16 ~ 06:28
[click here | https://vsolar.mssl.ucl.ac.uk/eiswiki/images/eis40/eis_int_vel_v0_log.mov]
\\
At line 146 changed one line
[Ignacio Ugarte-Urra: using 40" slot to do plasma diagnostics: electron density and DEM analysis|http://msslxr.mssl.ucl.ac.uk:8080/eiswiki/Wiki.jsp?page=SlotDiagnostics]
[Ignacio Ugarte-Urra: using 40" slot to do plasma diagnostics: electron density and DEM analysis|https://vsolar.mssl.ucl.ac.uk/eiswiki/Wiki.jsp?page=SlotDiagnostics]