IZMIRAN, MOSCOW, RUSSIA VOSTOK, ANTARCTICA (VSTK), 6NM64 NEUTRON MONITOR, CORRECTED FOR PRESSURE Altitude 3488 M Mean= 0.0 February 1972 Geographic Coordinates -78.47 106.87 Rc( 1965 )= 0.0 GV; SF= 100 Pressure Coefficient=- 0.787 %/mb Corrected to 620 mb Standard Pressure Comment: 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 72 02 1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 72 02 2 0 0 0 0 ...

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Wednesday, February 15th, 2012 . ... Monday, February 13th, 2012 . ... Сделать это можно использую Map Tools проекта SOPAC (http://sopac NULL .ucsd NULL .edu/maps/) . ... Wednesday, February 8th, 2012 . ... You are currently browsing the Лаборатория лазерной интерферометрии blog archives for February, 2012. ... Наши публикации . ... Публикации за 2010 . Публикации за 2011 . Публикации за 2012 . ... February 2012 . ... Лаборатория лазерной интерферометрии is proudly powered by WordPress . ...

... All events are assumed to occur in the centre of their pixel. ... Each event is tagged with a time stamp (FTCOARSE+FTFINE) corresponding to the specific FMTS integration within each tracking frame integration, in which each event occurred. ... The drift-corrected OM FAST mode event list contains 4 additional columns: the corrected X and Y pixel coordinates and OBT time for each event and a flag denoting whether the shift-corrected event falls within the defined science window. ...

Astronotes Armagh Planetarium's Stellar Blog! ... Space Flight . ... Monthly Sky Notes . ... February . ... Posted on February 2, 2016 | No Comments Goodbye January blues, hello February fun! ... Continue Reading.. ... 1 Comment If you look towards the west just after sunset this February you will see a very bright star in the darkening sky. ... 2 Comments The long dark nights continue through February, but this does give us a chance to see some interesting objects in our night sky. ...

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February 10, 2003 (Monday) Igor Tyukhov, Oregon Solar Radiation Monitoring Laboratory . February 17, 2003 (Monday) Osamu Yasuda, Tokyo Metropolitan University . February 20, 2003 (Thursday) Linear Collider Seminar . ... Fall 2002 . Fall 2001 . ... Fall 2000 . ... 3:00 pm, 472 Willamette Hall . ... The American Linear Collider Physics Group (ALCPG) has initiated a series of monthly seminars intended for a broad audience. ... This is the inaugural seminar. 1:00 pm, 472 Willamette Hall . ...

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... 2011 February 7 . Sun 360: STEREO Captures Views of the Entire Sun . Credit: STEREO Project , NASA . ... This has become possible because the two STEREO satellites orbiting and monitoring the Sun are now on opposite sides of the Sun. ... Even though the STEREO satellites will continue to drift apart at about 44 degrees per year, Sun-staring instruments on or near the Earth will augment them to provide a full view of the Sun for the next several years. ... About APOD | ...

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These cables may or may not be correctly constructed. ... 9 PIN D-SUB ?? to the Monitor. 23 PIN D-SUB FEMALE to the Amiga. 9 Pin . ... Via 2 Hex Inverters, i.e 74LS04) . ... 9 PIN D-SUB MALE to the C128. ...

... gradients dependencies on solar wind parameters and IMF; . ... fate of thermal plasma at the dayside magnetopause. velocity-dispersed injections of the thermal and superthermal ions from LLBL at cusp and cleft (lowest energy VDIS-2 events); . ... outer cusp processes, role of outer cusp indentation, plasma entry (laminar reconnection, turbulent diffusion, others), role of turbulent boundary layer; . how is the magnetosheath plasma heated near magnetopause and cusp? . ... cusp/cleft wave emissions. ...

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... The source exhibits a mas-scale structure which, according to the USNO multi-epoch monitoring at 2.3 and 8.4 GHz over the period from 1994 July through 1998 April, undergoes considerable changes in the brightness distribution and positions of the major structural features. Our image is qualitatively consistent with the structural pattern of the source. ... We note a difference of ~90 in position angles of secondary components in our image and the 5 GHz VLBI image by Shen et al. 1998). ...

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