EIS Team Science Meeting Agenda#
18th MarchThis page refers to one day of a closed meeting of the EIS consortium
Table of Contents
- EIS Team Science Meeting Agenda
- Comments from attendees welcome!
- Report from Technical Splinter Meeting (previous day)
- Calibration updates
- Remote Operations
- Study-creation in the S-band Era
- What we’ve learned to date:
- How do we address observing challenging targets like flares?
- EIS Science Results
- Quiet Sun
- Active Regions
- Coronal Holes
- Flares
- Techniques
- Science with other, non-Hinode instruments
- Communicating Science
- Promoting science results to the immediate and wider science community
- Communicating EIS Science beyond the professional science community
- Analysis Software
- State of reduction package
- Useful additional software
- EISWiki
- Changes made since last year
- How to increase participation
- Keeping the contents up-to-date
- New layers of information
- Confirmed Attendees
Comments from attendees welcome!#
If you are attending this day of the meeting, please comment here if you would like to give input.Those without an EISWiki account (shame on you!) can mail their comments and intended contribution topics to David Williams.
It would be good to have a discussion about this agenda before the meeting, here on the EISWiki.
Report from Technical Splinter Meeting (previous day)#
Expect to hear reports on things like...Calibration updates#
Remote Operations#
- Remote Planning
- Procedure
- Human
- Software
- Procedure
- Interactions
Study-creation in the S-band Era#
What we’ve learned to date:#
- Prospects
- Problems
- Experiences
How do we address observing challenging targets like flares?#
This is a particularly interesting problem.
EIS Science Results#
Talks should put special emphasis on unsolved components in the context of what they talk about, and how they can be addressed using all three instruments on Hinode.Are these categories now out-dated? Should we organise talks differently?
Quiet Sun#
Active Regions#
- Cambridge Active Region Studies
Coronal Holes#
Flares#
Techniques#
- Line identifications with EIS and CHIANTI (Peter Young)
- Diagnostics with the slot (Ignacio Ugarte)
Science with other, non-Hinode instruments#
- We've had many campaigns with SUMER;
- CDS routinely follows EIS's pointing;
- TRACE will routinely follow the most active target on the Sun (as declared by Max Millennium
's CO), while Hinode often does the same;
- there have been several high-profile mutli-instrument campaigns, such as the WHI campaign in 2008
- large numbers of HOPs have had a ground-based observatory component
Communicating Science#
Promoting science results to the immediate and wider science community#
Communicating EIS Science beyond the professional science community#
Analysis Software#
State of reduction package#
- EIS_PREP, etc.
Useful additional software#
(With descriptions or demonstrations)- Gaussian fitting routines for EIS (Peter Young)
EISWiki#
The EIS Wiki is our public face for informationChanges made since last year#
How to increase participation#
Keeping the contents up-to-date#
- Good practice
New layers of information#
Confirmed Attendees#
- David Brooks (NRL)
- Paul Bryans (NRL)
- Len Culhane (MSSL)
- Ken Dere (GMU)
- George Doschek (US PI; NRL)
- Hirohisa Hara (NAOJ)
- Louise Harra (PI; MSSL)
- Shinsuke Imada (NAOJ)
- Helen Mason (DAMTP)
- Ryan Milligan (GSFC)
- Steve Myers (NRL)
- Karin Muglach (NRL)
- John Rainnie (RAL)
- Ignacio Ugarte Urra (NRL)
- Harry Warren (NRL)
- Tetsuya Watanabe (Japan PI; NAOJ)
- David Williams (MSSL)
- Peter Young (NRL)
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