... BEGIN = PROJECT_INFO PROJECT_CODE = v172a TITLE = Imaging the scattering size PI_NAME = Giuseppe Cimo PI_ADDRESS = School of Mathematics ... Private Bag 37 PI_PHONE = +61-03-62267256 PI_OBS_PHONE = PI_EMAIL = Giuseppe.Cimo@utas.edu.au PI_FAX = +61-03-62262410 START = 2004-106 /18:00:00 STOP = 2004-107/17:56:00 CORRELATOR = LBA END = PROJECT_INFO BEGIN = STATION_SETUP STATION = Pa RECORD_SCANS = 70 RECORD_HOURS = 23.73 FE = 20cm omit 20cm ...

Microsymposium 40, abstract 28, 2004 (A4 format) HIGH PURITY GE GAMMA-RAY SPECTROMETER ON JAPANESE LUNAR POLAR ORBITER SELENE. ... GRS consists of three parts; gamma-ray detector (GRD), compressor driver unit (CDU) and gammaray and particle electronics (GPE). ... It is retained at ~80K, by means of a mechanical cryostat. ... The asymmetric shape makes it efficient to veto gamma-rays from the SELENE vehicle and leakage photons from the Ge detector, as well as to avoid charged particles. ...

... disappearance/eruption of the filament accompanied by a number of large-scale dynamic phenomena (a coronal wave, chain, CME, arcade) Yohkoh/SXT . H-alpha and Yohkoh/SXT . ... SOHO/EIT (DelaboudiniХre et al., 1995) images and movies; . ... Preceding activity SOHO/EIT, 195 A (10-22 UT) (Figure 3) . ... SOHO/EIT, 171 A (Figure 4) MLSO/HAO H-alpha and He I 10830 A (Figure 5) MLSO/HAO, He I 10830 A . ... SOHO/EIT, 171 A (Figure 4) SOHO/EIT (171, 195, 284, 304 A) Dec 29, 1999 (Figure 10) . ...

... TAKO (``Timeline Assembler, Keyword Oriented'', or in Japanese, ``octopus'') is our in-progress suite of software that takes database input and produces mission timelines. ... The three main factors to consider are calculated quantities (i.e., unchangeable facts of the situation), derived quantities (soft constraints, ratings of good and bad events, and politics), and capacity constraints (such as time and telemetry). ... And, TAKO is modular by design, to allow for use with different missions. ...

... The VSOP Symposium proceedings, "Astrophysical Phenomena Revealed by Space VLBI" have been published and have been distributed to participants. ... Following the successful launch of the VLBI Space Observatory Programme (VSOP) satellite HALCA in February 1997 there have been many exciting results from space VLBI observations. ... Also, check the newly revised getting to ISAS page which has links to pictorial "Getting to ISAS from Fuchinobe" and "Getting to the Dai-Ichi Hotel from Fuchinobe" pages! ...

... Astro­E's Mission Independent Scheduling Suite A. Antunes and A. Saunders Hughes­STX, Goddard Space Flight Center, Greenbelt, MD 20707, Email: antunes@lheamail.gsfc.nasa.gov P. Hilton Hughes International/ISAS, 3­1­1 Yoshinodai, Sagamihara, Kanagawa 229, Japan Abstract. ... TAKO (``Timeline Assembler, Keyword Oriented'', or in Japanese, ``octopus'') is our in­progress suite of software that takes database input and produces mission timelines. ... Astro­E launches early in 2000. ...

... A trial to detect non-thermal emission from a best candidate among WDs, AE Aquarii, was performed with the hard X-ray detector (HXD) on-board the fifth Japaneses X-ray satellite, Suzaku. ... NSs data [25, 24]; WDs [39, 34, 35]) 2. ... In addition to the HXD, which covers 10­70 keV with PIN diodes and 40­ 600 keV with Gd 2 SiO5 :Ce (GSO) scintillators [33, 22], it carries onboard the X-ray Imaging Spectrometer (XIS), operating at 0.2­12 keV [26, 23]. ... X-ray spectra of AE Aqrarii with HXD PIN...

Next: Mission Operations Data Transfer . ... VLBI Tape Management . VLBI Tapes . ... When: As soon as the correlator is satisfied with the correlator output. back to top . ... What: Each correlator will maintain a data base including the status of all VLBI tapes under its control. ... The correlators will distribute tapes to mission elements based on the Observation Summary File produced by the RSOG ( Observation Summary File ) to ensure each element has enough tapes to support SVLBI observations. ...

... Printed in U.S.A. THE MOTIONS OF THE HARD X-RAY SOURCES IN SOLAR FLARES : IMAGES AND STATISTICS Sergey A. Bogachev and Boris V. Somov Astronomical Institute, Moscow State University, Universitetskij Prospekt ... the basis of the Yohkoh Hard X-Ray Telescope ( HXT ) data, we present a statistical study of different types of the hard X-ray ( HXR ) source motions during solar flares ... Type I motion of HXR sources in flares. them, the HXR sources systematically moved during flare. ...