Issue 121, 13 December, 2002

Table of Contents
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1. Yosemite Conference Abstract Deadline Approaching
2. Call for Papers for 2003 EGS-AGU-EUG Joint Assembly Session PS5.03 on
“Outer planets plasma physics”
3. Call for Abstracts for the Joint 2003 IEEE/URSI North American Radio
Science Meeting Session “Ionospheric Sounding with GPS”
4. Job Announcement – Postdoctoral Research Associate in Computational
Solar Physics at Catholic University of America
5. Job Announcement – Research Scientist-National Virtual Observatory at
the Universities Space Research Association (USRA)
6. Student Opportunity – Summer Student Research Opportunities (SSRO) in
Space Science at the Universities Space Research Association (USRA)
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* ********* * SPA SECTION NEWSLETTER . ..
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* * *********** * * Volume IX, Issue 121 . o .
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* ********* * 13 December, 2002 . ..
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* * * Editor: Guan Le .
* * * Email: editor@igpp.ucla.edu . . . . . . .
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1. Yosemite Conference Abstract Deadline Approaching
—————————————————-
From: Patricia Reiff

The Yosemite Conference on the Cusp and Dayside Magnetosphere is fast
approaching! We have a stellar lineup of invited speakers, and
quite a few terrific contributed abstracts as well. Some support for
student participation is available – be sure to let us know by the
abstract deadline.

The abstract deadline is COB December 17, 2002. Late abstracts may
be considered, but will have a $50 late fee. Earlybird conference
registration ends December 23.

The full information, including housing and abstracts, is online at
http://yosemite2003.space.swri.edu

————————————————————————
2. Call for Papers for 2003 EGS-AGU-EUG Joint Assembly Session PS5.03 on
“Outer planets plasma physics”
————————————————————————
From: “Krupp Dr., Norbert”

EGS-AGU-EUG Joint Assembly, 6-11 April 2003, Nice, France
Web: http://www.copernicus.org/egsagueug/

Session PS5.03: “Outer planets plasma physics”

Session scope:

The scope of this session covers new experimental findings of in-situ and
remote diagnostics
of the outer planets and their satellites, as well as theoretical results
from the modeling of planetary systems. Comprehensive interpretation of
results from the Galileo mission to Jupiter,
studies in preparation of the Cassini mission as well as results from ground
based – or Earth orbit based observations are encouraged, especially new
results in understanding the aurorae on Jupiter and Saturn.

Convener:
Krupp, Norbert
Max-Planck-Institut fur Aeronomie
Max-Planck-Str. 2
37191 Katlenburg-Lindau
Germany

Co-Convener(s):
Prange, Renee
Observatoire de Paris
5, place Jules Janssen
92195 Meudon Principal Cedex
France

Important deadlines:
1. Deadline for “Early Bird” Registration: 31 December 2002
2. Deadline for Receipt of Abstracts: 15 January 2003
3. Deadline for Pre-Registration: 07 March 2003

All further details: http://www.copernicus.org/egsagueug/
Thank you for considering contributing to the success of this session with
your presentation. Please inform also all your colleagues about the session.

Please send a copy of your contribution to us. We look forward to seeing you
in Nice next year!

N. Krupp (krupp@linmpi.mpg.de)
R. Prange (renee.prange@obspm.fr)

———————————————————————–
3. Call for Abstracts for the Joint 2003 IEEE/URSI North American Radio
Science Meeting Session “Ionospheric Sounding with GPS”
———————————————————————–
From: Attila Komjathy

Dear Colleagues:

We would like to draw your attention to the “Ionospheric Sounding with GPS”
session at the upcoming joint 2003 URSI North American Radio Science
Meeting and IEEE International Symposium on Antennas and Propagation to be
held in Columbus, Ohio, 22-27 June 2003 .
We hereby invite the submission of one-page abstracts by you and your
colleagues. The abstracts are due 8 January 2002 (hard copy) and 15
January 2003 for Web submissions. We note that the Call for Papers on the
Web site above indicate a paper submission requirement by the January
deadline. As a clarification they only mean a one-page paper, i.e., a
regular URSI abstract submission.

Please find a short summary of our session appended below. We are
encouraging you to submit the abstracts on-line
with an email
notification to the co-chairs Dr. Attila Komjathy
of the NASA Jet Propulsion Laboratory
and Dr. Richard Langley of the University of New
Brunswick, Canada.

Please note that there is a Student Paper Contest sponsored by
USNC/CNC/URSI this year. The student paper submission due date is set
for 3 January 2003. There are four prizes ($125, 250, 500 and 1000) in
addition to covering travel and subsistence expenses for the four
student finalists. For more information please refer to
.

Because this message is distributed through several mailing lists, we
apologize if you receive more than one copy of this announcement.
Please forward this information to colleagues that may not have
obtained this email.

Hope to hear from you soon.

Best regards,

Attila Komjathy and Richard Langley
Co-chairs

Ionospheric Sounding with GPS

There is an old adage in science and engineering: One person’s signal
is another person’s noise. Most Global Positioning System (GPS)
users consider the delay or advance of signals by the ionosphere to
be noise, as their presence reduces positioning accuracy. On the
other hand, one can take advantage of these errors to characterize
the ionosphere. The session will review (1) the latest modeling
techniques, methods, applications and results for ionospheric total
electron content (TEC) modeling using ground-based GPS networks
including e.g., the International GPS Service (IGS), Continuously
Operating Reference Stations (CORS) and the Wide Area Augmentation
System’s Reference Stations; (2) the current spaceborne missions such
as CHAMP, SAC-C, IOX, GPS/MET, GRACE, etc., which observe electron
density profiles using occultation techniques; (3) future GPS
occultation satellite missions such as COSMIC, ICESAT, FEDSAT and
e-POP. We particularly welcome contributions related to NASA’s Living
with a Star research program. The growing networks of ground-based
continuously operating GPS receivers and new constellations of GPS
occultation satellites represent a major new data source for space
weather analysis and prediction. We encourage contributions related
to the impact of these new techniques in the areas of space weather
analysis and prediction.

———————————————————————-
4. Job Announcement – Postdoctoral Research Associate in Computational
Solar Physics at Catholic University of America
———————————————————————-
From: “Leon Ofman”

Postdoctoral Research Associate
Computational Solar Physics
Department of Physics
Catholic University of America
200 Hannan Hall
620 Michigan Ave NE
Washington, DC 20064
USA

Tel: 301 286 9913
Fax: 301 286 1617

Email Inquiries: Leon.Ofman@gsfc.nasa.gov

A postdoctoral position is available immediately to work with Prof. Leon
Ofman on computational problems in solar coronal physics in support of space
based observations by the SOHO and TRACE satellites, and the future NASA
STEREO mission. The work involves numerical modeling (MHD, multifluid, or
kinetic) of coronal mass ejections (CME’s), and the solar wind. The work is
in close
collaboration with scientist
at NASA Goddard Space Flight Center in Greenbelt, Maryland.

The initial appointment will be for a period of one year, starting
immediately,
with a possible renewal for an additional year. Selection will be made
as soon
as a suitable candidate is found. Interested applicants should send by
email a
resume, a brief statement of research interests, a list of publications,
and
the names of at least three references to the above address. CUA is an
Affirmative Action/Equal Opportunity Employer.

————————————————————————
5. Job Announcement – Research Scientist-National Virtual Observatory at
the Universities Space Research Association (USRA)
————————————————————————
From: Ginny Peles

The Universities Space Research Association (USRA), in conjunction with the
NASA/Goddard Space Flight Center’s Laboratory for High Energy Astrophysics
(LHEA), is seeking a research scientist to work on-site at GSFC, with
NASA’s developing National Virtual Observatory (NVO) project.

The successful candidate will be responsible for the development of
interfaces to astronomical archives at the HEASARC in coordination with the
NVO collaboration. This position requires the application of new
information technologies, especially in the data grid area, to science
research activities in high-energy astronomy.

The successful candidate should possess a Ph.D., or at minimum, a Master’s
degree, in astrophysics or information sciences. Experience in using
science data archives for research, and familiarity with emerging
technologies including the data grid, web services, and metadata standards
is highly desired. Good communications skills and the ability to work in a
distributed collaborative environment are essential.

USRA is a non-profit university consortium, chartered to broaden
opportunities for collaboration between university and government space
research communities. EOE. Applications received by 17 January 2003 will
receive full consideration. Apply on-line at:
http://phoenix.seabrook.usra.edu/cpss/resume/ and/or mail letter describing
research interests, complete CV and publication list, and contacts (include
e-mail addresses) for at least three references to:

Universities Space Research Association
Attn: David V. Holdridge
Code: NVO
7501 Forbes Blvd., Suite 206
Seabrook, MD 20706-2253

————————————————————————
6. Student Opportunity – Summer Student Research Opportunities (SSRO) in
Space Science at the Universities Space Research Association (USRA)
————————————————————————
From: Ginny Peles

Summer Student Research Opportunities (SSRO)

Sponsored by Universities Space Research Association (USRA) and the
NASA Goddard Space Flight Center’s (GSFC) Space Sciences Directorate
Greenbelt, Maryland

June 9 – August 15, 2003

The Program

A limited number of paid positions are available to undergraduate and
graduate students to encourage an interest in physics, solar physics,
extraterrestrial physics, astronomy, astrophysics, and computer science/
information technology. Selected students will be teamed with a scientist
mentor having parallel scientific interests, to jointly develop and carry
out a research-related project at GSFC over the 10-week period.

In addition to the primary research project, participants will be expected
to attend scientific colloquia, participate in lunchtime brown bag
seminars, and visit other GSFC laboratories. Participants will receive a
tour of the Goddard campus conducted by a representative of the GSFC Public
Affairs Office. At the conclusion of the 10-week period, participants will
present oral and written reports on their projects to their fellow summer
students, their mentors, and other members of the Space Sciences
Directorate. On a case-by-case basis, participants may be granted
incentives to continue collaborative projects during the next academic year.

Projects

The Space Science Directorate is comprised of the Laboratories for High
Energy Astrophysics, Astronomy and Solar Physics, Extraterrestrial Physics
as well as the Space Science Data Operations Office. Scientific research
within the laboratories is directed toward both experimental and
theoretical activities in the following areas: x-ray, gamma-ray, and
cosmic-ray astrophysics; UV/optical astronomy; solar physics; infrared
astrophysics; astrochemistry; interplanetary physics; planetary systems;
planetary magnetospheres; and, electrodynamics.

A sampling of past and possible future projects includes the following:

* Cosmic rays: investigating the processes of cosmic ray propagation and
acceleration, characterizing the cosmic ray composition and sources.

* Detectors: development of high-energy resolution calorimeters for x-ray
spectroscopy (Constellation-X), and scalable, large area micro-well arrays
for all sky monitoring (ISS-Lobster).

* Galactic binaries: the study of the spectral variation of x-ray bursts.

* Gamma-ray bursts: using Bayesian analysis algorithms to characterize
pulse distributions in gamma-ray burst (GRB) temporal profiles.

* Ionospheric response: investigation of global ionization, heating, and
flow of ionospheric plasma in response to solar and magnetospheric energy
inputs, using POLAR/TIDE, FAST, and DMSP spacecraft.

* Interplanetary gas and dust: exploration using a combination of direct
and indirect observations of interstellar atoms and neutralized solar wind
ions from the IMAGE/LENA imager, and energetic “pickup” ions in the solar
wind from Wind, ACE, and Ulysses.

* Interstellar matter and molecular clouds: studying the diffuse gamma-ray
emission observed by the Energetic Gamma Ray Experiment Telescope (EGRET)
to evaluate the coupling of cosmic rays to interstellar gas in the outer
Galaxy.

* Magnetospheric response: the coupling of energy and plasma from the
solar wind into magnetospheres, creating space weather, is studied using
observations from WIND, POLAR, FAST, and IMAGE missions, in comparison with
relevant theories and global simulations.

* Particle analyzers and imagers: development of innovative particle and
plasma velocity analysis and detection systems, including imaging systems
for electrons, ions, and neutral atoms.

* Solar wind acceleration and dynamics: observations from several
spacecraft are compared with theories of the solar wind to investigate the
processes that heat the corona, accelerate the wind, and influence its
properties.

* Stars: continuous monitoring of the x-ray variations from the extremely
massive star Eta Carinae using the Rossi X-ray Timing Explorer (RXTE).

* Supernovae and supernova remnants: analyzing the x-ray emission from SNR
G21.5-0.98 to better understand the x-ray emission from composite type
supernova remnants.

* Black holes: mapping the accretion history of super-massive black holes.

* Mechanical design and analysis: modifications and additions to existing
project instruments.

* Space data systems: development of autonomous flight and ground systems
for command and data handling and flow.

Compensation and Support

Selected students will be placed on USRA’s payroll as Student Assistants
and compensated at the rate of $10 per hour for undergraduates and $12 per
hour for graduate students for 40 hours per week for 10 weeks. USRA will
reimburse reasonable roundtrip domestic travel expenses for non-local
participants. A variety of local housing arrangements are available and
will be funded for program participants only (no family members).

Eligibility and Selection Criteria

The program is open to students enrolled in, or accepted to, accredited U.
S. undergraduate and graduate programs in physics, astronomy, astrophysics,
engineering, computer science, or related disciplines. Students will be
selected based on the following:
* academic record (official transcripts required)
* motivation and career interests
* preparation to contribute toward research in astronomy, astrophysics,
solar/magnetospheric physics, and space data and information sciences
* relevance of career goals and experiences to USRA and GSFC scientists
* letters of recommendation.

We encourage students at minority, tribal, and community colleges to apply
who may have limited on-campus access to specialized faculty and/or
resources in the research areas listed above. Women and minorities are
encouraged to apply.

Participants MUST commit for the full 10-week period. Due to NASA security
regulations, citizens of certain countries may not be eligible for access
to the GSFC campus. Non-U. S. citizens should contact the SSRO Program
Coordinator to confirm eligibility before applying
(lmewshaw@seabrook.usra.edu).

Application Deadline Friday, February 14, 2003 for receipt of all
application materials, transcripts, and letters of recommendation.

Application Guidelines

The application form is located at the following URL:
http://phoenix.seabrook.usra.edu/cpss/. On the left sidebar, click on
Student Opportunities. The link to the application form is at the bottom
of the SSRO program announcement.

Complete the application form and mail it to the address below with a copy
of your CV or resume that shows a complete education and employment
history. In addition, have an official copy of your transcript and two
letters of recommendation sent directly by mail to the same address for
receipt by the February 14th deadline.
SSRO Program Coordinator
Universities Space Research Association
7501 Forbes Blvd, Suite 206
Seabrook, MD 20706

A complete application contains the application form, a CV or resume, an
official transcript, and two letters of recommendation. Complete
applications will receive full consideration.

Questions regarding this program or the application process should be
directed to the SSRO Program Coordinator at 301-805-8396 or
lmewshaw@seabrook.usra.edu.

Selection Announcements

The number of positions awarded will depend upon funding availability.
Applicants selected will be contacted electronically in late March or early
April 2003.

Sources of Additional Information

Information on the USRA Cooperative Program in Space Sciences that operates
SSRO may be found at http://phoenix.seabrook.usra.edu/cpss/.

Information on USRA may be found at http://www.usra.edu.

Information on the NASA Goddard Space Flight Center may be found at
http://www.gsfc.nasa.gov.

Information on the NASA Goddard Space Sciences Directorate may be found at
http://space.gsfc.nasa.gov.

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