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h1>Travel support</h1> <p>Same as for past INTEGRAL workshops, the organizers will make best efforts to provide some financial support to help participants, e.g. young (under 35 years old) scientists, attending the workshop. Travel support relies solely upon very limited funds which we hope will become available through sponsors. The total amount available is yet unknown, as is the number of requests for financial support. ...

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System of astrometric databases of Pulkovo observatory. ... The purpose of these observations is the determination of precise coordinates of Solar system bodies, which is necessary for development and improvement of motion theories, and for studying the evolution of the Solar system. ... Accuracy of photographical observations is about 0.2-0.3 arcsec for equatorial coordinates and 0.1-0.3 for relative coordinates of planetary satellites, depending on object and observational conditions. ...

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... Local Organizing Committee: . ... 196140, St. Petersburg . ... e-mail: journees2014@gao.spb.ru . ... fax: +7-(812)-723-1922 ("For Journ es 2014 organizing committee") . You can also use the following contacts for specific requests. All requests related to the Conference organization: . ... Tel: +7-(812)-363-7442 . e-mail: malkin@gao.spb.ru . ... e-mail: n.capitaine@obspm.fr (Subject: Journees 2014) . ... e-mail: km@gao.spb.ru . ...

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Photos and Imagery . ... If the photo is a NASA numbered photo and . you are a non-NASA employee or contractor or you are a member of the media, contact the JSC Media Resource Center at 281-483-4231. If you are requesting the photo on behalf of a NASA/JSC partner organization, such as Space Center Houston, contact the Media Resource Center at 281-483-4231, which will submit a form 246 for you. If you are a NASA employee or contractor, contact the NASA/JSC Photo Department at 281.483.2313 . ...

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... ACCORDING TO THE CENTRE IN BOULDER 17-19.03 ONE LONG MAGNETIC STORM WAS OBSERVED (G4, Ams = 83, dur. = 60 h.), AFTER WHICH IN 6 HOURS (19 - 20.03) MINOR MAGNETIC STORM FOLLOWED (G1, Ams= 33, dur.= 12 h.) AND AT THE END OF THE DAY 20 AND 21.03 ONE MORE MINOR MAGNETIC STORM (G1, Ams= 25, dur.= 12 h.), AND 22.03 IT IS NOTED SUBSTORM OF G1 INTENSITY, dur. 9 h. ALL THESE ADDITIONAL GEOMAGNETIC DISTURBANCES WERE FED WITH FLARES IN AR12297 AND SOLAR FILAMENT EJECTIONS 17-18.03. ...

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RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope 's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases Publication SSRT - Siberian Solar Radio Telescope . ...

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... Precisely one month ago, on 11 July 2009, the last active area of the new solar cycle disappeared from the surface of the Sun. Over the 30 days following this, neither observers on Earth nor devices in space have been able to detect the emergence of any sunspots. ... Therefore, it seems that our star has once again returned to a state of deep solar "winter", following several sparks of activity in May-June 2009. ... To date, this period has lasted 30 days. ...

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... Other Planned Activities Include Solar Observing Astrophotography Presentations and CCD Demo's Field Trip to AAAP Observatory at Jenny Jump Workshop: Learning to Use Your New Telescope Plus Swimming (life guards provided), Fishing, Volleyball, Basketball, Hiking, Game room Kayaking/canoeing (bring your own) on two lakes and nearby Pequest and Paulins Kill Rivers Registration Fees Camping and RV -- $35.00 per person ($45 after June 9) Bunkhouse -- $45.00 per ...

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The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

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... Phys. (U.S.S.R. ) 42, 1416-1418 (May, 1962) A series of size effects , which are determined by the relationships between the size of electron orbits and the size of a metallic sample, can be observed when a sample having a long fre e path is placed in a constant magnetic field. ... When the field is increased the radius of the electron orbit decreases, and the numbe r of return s of the electron throug h the skin layer durin g the fre e path time increases. ... The sample had a thickness of 0.54 mm ...

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