Newsletter - GEM FG9 - Space Radiation Climatology - Volume 2, Number 1, Jan 2008

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Paul O'Brien

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Jan 4, 2008, 8:58:44 AM1/4/08
to gem-2007-space-radia...@googlegroups.com

   **********************************************
   * GEM FG9 - Space Radiation Climatology      *
   * Newsletter - Volume 2, Number 1, Jan 2008  *
   * Paul O'Brien (paul.obrien-at-aero.org)     *
   * Geoff Reeves (reeves-at-lanl.gov)          *
   **********************************************

Contents:
1. Summary of 2007 GEM Mini-Workshop at Fall AGU
2. Collecting reanalyses, climatologies, etc on-line


************************************************************
1. Summary of 2007 GEM Mini-Workshop at Fall AGU

At the 2007 Mini-Workshop at Fall AGU we discussed our plans for the
remainder of the FG9 years.

Paul O'Brien lead the discussion with a set of suggested "products" we
could provide to GEM. Paul's list was sorted roughly by ease of
completion, but Terry Onsager and others suggested we also ought to
prioritize by scientific impact.

Geoff Reeves stated that our primary scientific objective ought to be
to "Discover the climatology of the inner magnetosphere." This idea
went over well.

We also discussed how to organize the summer 2008 GEM workshop FG9
sessions. Some invited talks were suggested:

- A student tutorial on reanalysis and climatology (to give students
  thesis ideas)

- What we already know about inner magnetosphere climatology.

- How do we characterize long-term climatology?

- Intro to data assimilation, principal component analysis, etc. (Yuri
  Shprits)

More information will be posted at:
http://virbo.org/wiki/index.php/GEM2007mini
This is your Wiki - you can edit it!


************************************************************
2. Collecting reanalyses, climatologies, etc on-line

As a group we decided it was important to collect at least a list of
reanalyses, climatologies, and similar data sets. Bob Weigel has
tentatively agreed to host these data on ViRBO - assuming disk space
does not become an issue. Mike Wiltberger stated that we could
probably work something out with NCAR and/or NGDC for our really huge
data sets.

We know of the following reanalysis-like data sets:

- ONERA Salammbo electrons and protons: 11+ years, Sebastien Bourdarie.
  Sebastien has stated that for the time being this data cannot be
  widely released due to ONERA policy. Individual collaborations may
  be possible. Sebastien.Bourdarie-at-onecert.fr

- LANL DREAM Outer Zone Reanalysis: full solar cycle should be done by
  Summer GEM, Geoff Reeves.

- UCLA CRRES Outer Zone Reanalysis: entire CRRES mission, Yuri
  Shprits.

- U. Mich. Ring Current: numerous 4-day runs, Mike Liemohn.

- Aerospace statistical electron reanalysis: 11 years, Paul O'Brien.
  This data set will be released to ViRBO when version 2 is complete
  (early-mid 2008).

- Aerospace Selesnick proton model: multiple solar cycles, Richard
  Selesnick.

- SymH, AsymH, global current systems, Natalia Ganushkina.

- B-field perturbations at GEO, Howard Singer.

************************************************************

For more detailed and more frequent updates, consult the ViRBO wiki at
http://virbo.org/wiki/index.php/GEM2007.

---------------------------------------------
To view the FG9 email archive, go to
http://groups.google.com/group/gem-2007-space-radiation-climatology-fg9



---------
T. Paul O'Brien, PhD
Space Science Department/Chantilly
The Aerospace Corporation
15049 Conference Center Drive, CH3/210
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Michelle Thomsen

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Jan 4, 2008, 12:55:35 PM1/4/08
to gem-2007-space-radia...@googlegroups.com
Paul,

Over the holidays I reread your paper (O'Brien and Lemon, Space
Weather, p. S03007, 2007), and I would like to explore with you the
possibility of implementing your results for future analyses here
behind the fence. However, I first need to understand better what
you actually did. I think my confusion centers on your Figure 4 (c
and d). From the text, I would have expected that for nhp at 0530
LT, you would have found one set of three models (e.g., Kp, nhp at
5.5+/-2 h) that gave the best correlation with your in-sample data
(paragraph 12). But Figure 4 shows that each of your models was
"used" thousands of times. What am I missing? If this would be
easier to explain over the phone, I'd be happy to call you or you
could call me at your convenience. I'll be here today until ~3:30
Mountain Time.

Best,
Michelle
--
Michelle F. Thomsen
Director, Center for Space Science and Exploration
MS D466
Los Alamos National Laboratory
Los Alamos, New Mexico 87545
(For overnight add:
SM-30, Bikini Atoll Road)
Phone: (505) 667-1624 (CSSE)
(505) 667-1210 (ISR-1)
FAX: (505) 665-7395
email: mtho...@lanl.gov
CORRESPONDENCE/Technical Data or Software Publicly Available

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