EEEEEEEEEEE U U V V EEEEEEEEEEE
E U U V V E
E U U V V E
EEEEEEE U U V V EEEEEEE
E U U V V E
E U U V V E
EEEEEEEEEEE UUUUU V EEEEEEEEEEE
------------------------------------------------------------------
ELECTRONIC NEWSLETTER OF THE EUVE OBSERVATORY Vol 2, No. 4 7/26/92
------------------------------------------------------------------
EUVE BEGINS SKY SURVEY
----------------------
THE EUVE Observatory started the all sky survey on Friday July
24. The Checkout and Calibration phase has concluded and con-
firmed that the EUVE instruments are working flawlessly.
During checkout some 22 EUV sources were detected including at
least two new EUV sources that are not previously reported.
At least four of the EUV sources observed during the checkout
period were observed to be variable during the observation.
Detected backgrounds in all 7 detectors are nominal, with back-
ground countrates due to geocoronal and inter-planetary emission
being close to the predicted values. The observed count rates
while observing down the Earth's shadow cone are very, very low.
No ram glow effects have been detected.
Instrument sensitivities are close to the predicted values from
pre-launch calibration, indicating no significant change in cali-
bration since the calibration three years ago.
The instruments were checked for any possible UV leaks by observ-
ing bright B stars. No significant UV leaks were found.
The observed instrument point spread functions are close to the
expected values indicating that the imaging is nominal. All the
instrument boresights have been calibrated.
The only unexplained instrument anomaly at this time is the occa-
sional detection of short-duration, high-count-rate bursts of
detector events. Twenty eight bursts have been seen, with the
bursts only occurring in 3 of the 7 detectors. The bursts are not
of astronomical origin and may be due to detector outgassing
events. The bursts have no impact on science.
During the first month of operation one Single Event Upset was
detected, requiring re-setting of a section of the memory.
The EUVE spacecraft is operating smoothly. During the pointed
calibrations the spacecraft stability was better than 2 arc
seconds. This is fantastic.
THE EUVE Science Operations software and image processing pipe-
lines are operating smoothly. The pipelines are operating at ap-
proximately 45% of real time. The standard science data products
are being generated on schedule.
The first EUVE data has been released through the EUVE Public Ar-
chive.
CEA PUBLIC DATA ARCHIVE - NEW DATA POSTED
------------------------------------------
The spectrum of an anonymous source detected in the medium
wavelength spectrometer has been released in the public archive.
The spectrum shows absorption at 170 angstroms due to the absorp-
tion edge aluminum from the filter on the detector.
The table showing which ROSAT WFC brights sources have been
detected has also been updated.
At the request of an archive user, we are now also posting back
issues of the EUVE electronic newsletter on the public archive.
To access the archive ftp site, ftp to superego@cea.berkeley.edu.
Change directory to pub/archive. Files available are listed in
the file index.
To obtain information concerning the Archive mail server, send a
mail message containing the word "help" (omit quotes) on the
first line, with no preceding spaces, to
archive@cea.berkeley.edu; a file containing information on the
mail server will be returned to you automatically. Although the
mail server is designed for processing requests for information
automatically, mail messages which do not address the server pro-
gram are sent to Archive personnel for a response.
Note to all archive users: NASA is currently establishing the ex-
act data rights policy on EUVE spectra released through the EUVE
public archive. Until this policy is clarified, scientists who
obtain the EUVE spectra should confine the use of these spectra
in assisting the planning of EUVE observations and analyzing
their own GO data. The publicly released spectra are not to be
used as the basis of scientific publications at this time.
Other queries concerning the EUVE Data Archive should be ad-
dressed to Dr. Jeremy Drake via archive@cea.berkeley.edu
For information about EUVE data rights policies governing the IOC
calibration data, contact Dr. Yoji Kondo, EUVE Project Scientist.
VISITORS TO BERKELEY INVITED TO ATTEND EUVE SCIENCE TEAM MEETINGS
-----------------------------------------------------------------
The EUVE Science Team meetings are held every other Friday from
3-5 PM at the Center for EUV Astrophysics conference room. The
recent EUVE results are presented and discussed. Visiting scien-
tists are invited to attend. Send e-mail to rmalina@berkeley.edu
to find out if a meeting is scheduled.
CELEBRATION OF START OF SKY SURVEY
-----------------------------------
The EUVE Project will be celebrating the success of the EUVE Ob-
servatory on August 14, 1992. All visiting friends and colleagues
are invited to join us. There will be an EUVE Science Team meet-
ing on the afternoon of August 14 where the EUVE results to date
will be summarized, followed by a celebration at the Oakland Boat
house. If you are interested in attending, send e-mail to
pub@cea.berkeley.edu
EUVE TECHNICAL BULLETIN RELEASED
--------------------------------
A new issue of the EUVE Technical Bulletin has been released. If
you are not already receiving these bulletins, you may add your-
self to the mailing list by e-mailing your name and postal ad-
dress to pub@cea.berkeley.edu
CEA E-MAIL ADDRESSES CHANGING
----------------------------
Due to a change in the campus computer network, the e-mail ad-
dresses for EUVE staff are changing. All CEA e-mail addresses are
now username@cea.berkeley.edu
------------------------------------------------------------------
The EUVE Electronic Newsletter is issued by the Center for Ex-
treme Ultraviolet Astrophysics, University of California, Berke-
ley. The opinions expressed are those of the authors. Publish-
ers: Roger F. Malina, C. Stuart Bowyer, Managing Editor: Camille
Trentacoste. Funded by NASA Contracts NAS5-30180 and NAS5-29298
Send newsletter correspondence to: pub@cea.berkeley.edu (Internet)
----------------------------------------------------------------
The EUVE Project is managed by NASA's GSFC. The Project Manager
at GSFC is Mr. Frank Volpe, the Project Scientist is Dr. Yoji
Kondo, the Deputy Project Scientist is Dr. Ronald Oliversen. The
NASA Head- quarters EUVE Program Scientist is Dr. Robert Sta-
chnik, the Depu- ty Program Scientist is Dr. Derek Buzasi, the
Program Manager is Mr. John Lintott. Information on the EUVE
Guest Observer Program is available from: Dr. Yoji Kondo, Mail
Code 684 GSFC, Greenbelt, MD 20771 (301) 286-6247 --
euve@stars.SPAN.NASA.GOV
[HomePage]
[Email]
[Search]
[Glossary]
Page created by webmastr@cea.berkeley.edu
Last modified 10/4/97