August 4, 2003
K.-I.Oyama, and T.
Maruyama
1.Scientific
satellites
NOZOMI approached the
earth on the 19th June and the earth swing by was successfully
conducted. The problem on the power supply will be repeatedly tried to be solved
until the end of November.
Hayabusa
,sample return mission,was
successfully launced on
Hayabusa is now under
routine operation. The distant between Hayabusa and the earth is about 0.1 AU in
June. Three ion engines (one out of four engines is backup) are being
used.
ASTRO-F was
postponed its launch after January 2004 because of the mechanical problem on
Telescope. Lunar –A is now scheduled in
summer 2004. ASTRO-EII will be January /February
2005.
2. Sounding
rockets
Wave 2004 rocket
experiment which is a follow on mission of WAVE2000 is scheduled its launch in
January 2004 in order to study the striation mechanism of atmospheric glow. The
ground supports will be reinforced ,by including sodium Lidar. The launch window
will be widened to have long time ground based ovservation. The NTV –3
experiment is planned in January 2005 in Andoya Rocket Range the experiment is
to study energetics and dynamics of the auroral atmosphere. EISCAT,MFradar
,Fabry Perot Interferrometer and other ground based optical facilities will be
coordinated internationally.
3.Individual
activities
Studies of the
ionosphere by using GPS data are being conducted in Kyoto University,Nagoya
University, and ISAS under the close communications. Total electron density map
over Japan was constructed by the group. During the data evaluation phase,
enhanced TEC was found at night,which was finally concluded as resulted from
erroneous data processing . The data was reprocessed and distributed to the
users by Kyoto University.
Validation of MF radar
located at Yamagawa observatory of CRL will be conducted in January 2004. Electron density profiles obtained with
VLF receiver onboard the rocket S-310-33 and obtained with MF radar will be
first compared.
MU radar is routinely
under operation. During the wave 2004 campaign, the radar will be operated to
measure nutral wind.
4. IRI NEWS June has
been issued. The NEWS has been published since 1993 and distribted more than 300
scientists in the world.
5.Workshop
and Symposium Announcements
5-1.
IRI session in General National URSI meeting.
COSPAR/URSI
Working Group of the International Reference Ionosphere (IRI) is organizing a
one day session at the upcoming German National URSI meeting in “Kleinheubach”
near Frankfurt/Main to honor Professor Karl Rawer on the occasion of his
90th birthday. Professor Rawer, who in the 1950’s wrote the first
book called “Die Ionosphäre” (later translated into English), started the
development of the IRI model more than thirty years ago under the auspices of
COSPAR and eventually COSPAR/URSI. During the URSI General Assembly in
Maastricht last year, the Working Group members voted to hold a special session
at the so-called Kleinheubach URSI Meeting in honor of Professor Rawer.
G.2 Three
Decades of the International Reference Ionosphere - a special session in honor
of Professor Karl Rawer's 90th Birthday"
Conveners: B. Reinisch and D.
Bilitza
This
session will be entirely conducted in English. If you are interested in
presenting a paper or poster on the topic of Karl Rawer’s life: the ionosphere,
please submit your abstract by August 8, 2003. Details of the meeting and its venues
can be found on
http://www.copernicus.org/URSI/kh_tagung/kleinh.htm
Bodo W. Reinisch
5-2.
International Reference Ionosphere Workshop 2003, 6-10 October
2003
IRI 2003
workshop will be held in Grahamstown, South Africa from the 6 to 10 October
2003. The overall theme of the workshop is ionospheric variability but all
papers relating to the IRI model are welcome. The following sessions have been
designed to accommodate the 43 abstracts accepted. The number of papers that
will be presented in each session is also shown.
The following countries
will be represented at this workshop: China, Brazil, USA, Argentina, South
Africa, Austria, Russia, Australia, UK, Japan, Cuba, India, Czech Republic,
Mexico, Ivory Coast and Nigeria.
Session
title |
No. of
papers |
A: Ionospheric
Variability |
12 |
B: Topside
Ionosphere |
7 |
C: Total Electron
Content |
4 |
D: IRI
Applications and Latest Results |
5 |
E: Equatorial
Ionosphere |
5 |
F: Lower and
Bottomside Ionosphere |
8 |
G:Other IRI
parameters |
2 |
A
registration fee of 55 US Dollars will be charged. This fee will include
lunches, coffee breaks, all workshop material and the workshop dinner. An
excursion is being organized for the Wednesday of the workshop week.
Accommodation has been pre arranged for delegates in a number of bed and
breakfast establishments located close to the workshop venue. Details can be
found on the workshop website.
Day tours have been
organized for accompanying persons. Seven possible day trips into the area
around and within Grahamstown (for e.g. visits to Bathurst, Port Alfred) are
available to choose from for that period. A 3-day tour option is being put
together for delegates for after the workshop. This option will include visits
to the beautiful eastern cape coast, the Addo elephant national park and the
scenic mountain village of Hogsback. Details of these tours will be available on
the workshop website by the end of June.
The workshop also has an appointed travel
agent that can assist delegates with putting together their own itineries for
visiting beautiful South Africa before or after the
workshop.
IRI 2003 is
sponsored by the International Union of Radio Science (URSI), Committee on Space
Research (COSPAR), Rhodes University and GrinTek Ewation (a division of MRCM
group).