- Don't forget to VOTE, VOTE, VOTE !(Actually, only vote once!)After voting, why don't you head to Mallard Lodge tonight and meet other Star Gazers that voted...!7PM ESTPj
Tim Milligan...please email the combination for the lock to me...my version is not current...just in case you find a pretty lady in distress and re-prioritize your priorities.
my email address is
Paul Riley <dmsg_pjr@...>
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11/04/2008 07:00 AMPlease respond to
firstname.lastname@example.orgSubject [delmarvastargazers] Meeting tonight
Don't forget to VOTE, VOTE, VOTE !
(Actually, only vote once!)
After voting, why don't you head to Mallard Lodge tonight and meet other Star Gazers that voted...!
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- For whom do you want us to vote?
Just kidding!On Tue, Nov 4, 2008 at 7:00 AM, Paul Riley <dmsg_pjr@...> wrote:Don't forget to VOTE, VOTE, VOTE !(Actually, only vote once!)After voting, why don't you head to Mallard Lodge tonight and meet other Star Gazers that voted...!7PM ESTPj
"By deepening our understanding of the true nature of physical reality, we profoundly reconfigure our sense of ourselves and our experience of the universe."
- physicist Brian Greene
"Sometimes the way a message unfolds its meaning is the most important meaning it offers."
- Brooks Landon
"Why should a sequence of words be anything but a pleasure?"
- saying attributed to Gertrude Stein
- The first detected GRB event ever detected on the sun was picked up by
the Fermi Gamma-Ray Space Telescope (formerly known as the Gamma-ray
Large Area Space Telescope (GLAST)) today.
Here's the announcement message:
DATE: 08/11/04 16:34:49 GMT
FROM: Chryssa Kouveliotou at MSFC
C. Kouveliotou (NASA/MSFC) and M.S. Briggs (UAHuntsville) report on
behalf of the Fermi GBM Team:
At 20:14:42.77 UT on 02 November 2008, the Fermi GBM triggered and
located a very soft and bright event (trigger 247349683 / 081102844).
The event location was RA = 217.6 deg, dec = -15.7 deg (+/- 1.1 deg), in
excellent agreement with the Sun location. The time of the event
coincides with the solar activity reported in the GOES solar reports
(event 9790: onset at 2012 UT, max at 2015 UT, end at 2017, B5.7 flare).
This is the first GBM detection of a solar flare; future detections will
not be reported in a GCN Circular, unless they exhibit special
The GBM light curve shows a multiple peak event lasting approximately
177 s (8-30 keV). The time-averaged spectrum from T0-13.824 s to
T0+163.33 s is best fit by a single power law model with index -6.55 +/-
0.03 (chi squared 255 for 120 d.o.f.). The event fluence (8-30 keV) in
this time interval is (1.54 +/- 0.03) E-4 erg/cm^2.
The spectral analysis results presented above are preliminary.