This page (revision-186) was last changed on 18-Apr-2021 19:09 by Jian Sun

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185 30-Jun-2011 16:36 45 KB Jian Sun to previous | to last
184 11-Apr-2011 10:53 45 KB JianSun to previous | to last
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Page References

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EisCoreStudy...nobody
EisCoreStudy

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Difference between version and

At line 600 changed one line
!ar091229-01 => CORE EIS Flare Study 2
!ar091229-11 => CORE EIS Flare Study 2
At line 620 changed one line
!ar100329-01 => Full CCD Scans of ARs for Increasing Spectral
!ar100329-12 => Full CCD Scans of ARs for Increasing Spectral
At line 640 added one line
!ar100417-02: Nanoflare heating of coronal loops
At line 642 added 26 lines
 Information – - Klimchuk ([james.a.klimchuk@masa.gov|mailto:james.a.klimchuk@masa.gov]), Patsourakos ([spatsurakos@gmail.com|mailto:spatsurakos@gmail.com]), Young ([pyoung@ssd5.nrl.navy.mil|mailto:pyoung@ssd5.nrl.navy.mil])\\
%%roundedCorners-yyyy-E3F0EE-808080
{{
-- test theory that coronal loops are bundles of unresolved, impulsively-heated strands by searching for spectral signatures in the wings of hot (~ 5MK) emission lines\\
-- run PRY_slot_context_v3 (4.9 Mbits, 3min 29s), nanoflare_sas_v1 (82.5 Mbits, 31min 24s)\\
-- run sequence: PRY_slot_context_v3, then nanoflare_sas_v1, finally PRY_slot_context_v3\\
-- run nanoflare_sas_v1 multiple times with raster repeats to fill available time\\
-- AR pointing for nanoflare_sas_v1 to be at lower legs of loops\\
-- select inner part of AR; not perimeter “fan” loops\\
-- choose side of AR with legs oriented along line-of-sight to maximize Doppler shift due to field-aligned flows\\
-- prefer ARs near disk center\\
-- for wavelength calibration, position hot loops towards either bottom or top of slit; ensure that the opposite side of the slit observes a quiet Sun region.\\
*NOTE *: for pointing confirmation, please send screen grab from eis_image_tool to all three study authors showing suggested pointing. See *http://tiny.cc/43rcc *for typical pointing examples\\
}}
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%%center
||Study ID||Acronym|| ||
|353|PRY_slot_context_v3|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=353]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=353]
|392|Eclipse_raster_v2|[details|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/ShowEisStudy.jsp?study=392]|[Example fits|http://msslxr.mssl.ucl.ac.uk:8080/SolarB/Studies2FitsConn.jsp?study=392]
%%
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This page (revision-186) was last changed on 18-Apr-2021 19:09 by Jian SunTop