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21. Accomodation - Cosmic Polarization Rotation Workshop, September 7-8, 2015
... The map available here shows the location of the workshop, of the Arcetri Observatory, and of some Hotels nearby. The hotels shown on the map have offered special rates to the participants of the Workshop on Cosmic Polarization Rotation (CPR WS). ... Hotel Villa Agape (see here ) offers single and double rooms at 72 and 135 euro per night, respectively, including taxes, continental breakfast, and private parking for one car. ... Please reserve before August 1st, 2015. ... cpr@arcetri.astro.it . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/cpr/accommodation.html -- 5.6 Кб -- 11.10.2015
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22. ASP: Cosmic Collisions
... Carefully measure the diameter of the craters formed by the impact without disturbing the sand. ... Crater diameter increases with increasing mass. ... Without disturbing the sand, carefully measure the crater diameter. ... Did you measure any difference in the diameters of the craters? Yes, as velocity increases, so does crater diameter. ... Impact cratering. ... Impact craters can be demonstrated with younger or less advanced students using mud instead of sand and ball bearings. ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/edu/publications/tnl/23/crater2.html -- 15.3 Кб -- 02.10.2012
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23. Stealth 64 VRAM Data Sheet
VRAM-based Windows and CAD Accelerator . ... 5 Year Warranty Diamond's Stealth 64 VRAM is the latest addition to the award winning Stealth family of graphics accelerators for compute-intensive Windows and DOS applications. Designed for PC/ and VESA local bus architectures,. the VRAM based Stealth 64 sets a new standard in 64-bit graphics performance. With 4MB of VRAM, the Stealth 64 displays 24-bit true color up to 1152x864 resolution and provides 65,536 colors at 1280x1024 resolution. ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/ftproot/pub/misc/doc/stealth64vram.html -- 6.4 Кб -- 11.08.1995
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24. Generation from In-Orbit Data
Next: PSF1DRB Up: PIXTOPIXSENS Previous: Generation from Ground Calibration Contents . Ideally the in-orbit PixToPixSens file will be generated from internal calibration measurements using the fullframe high resolution engineering mode. However due to their large data volume the fullframe high resolution data won't be available frequently enough to base the in-flight generation of the PixToPixSens file on the high resolution data. ... i.e. the average counts per pixel per CCD-frame . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node946.html -- 6.8 Кб -- 20.09.2011
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Еще в разделе: (Показать все результаты (>8127) - xmm.vilspa.esa.es/ )

25. http://www.wdcb.ru/stp/data/cosmic.ray/Neutron_Monitors(minute_values)/C/2001C/2001CALG/REME5M.TXT
This directory contains Calgary Neutron Monitor Data at five minute resolution. Each file is a gzipped tar archive that contains files of uncorrected count rates and barometric pressures at five minute intervals for one year. A file named snm.calg.fmi.YYYY.tgz is an archive that holds five minute data for the year YYYY. ... So a file named cal01030.fmi contains five minute uncorrected data for year 2001 day 30 (which is Jan 30, 2001). ... A text file named note.txt is also usually present. ...
[ Сохраненная копия ]  Ссылки http://www.wdcb.ru/stp/data/cosmic.ray/Neutron_Monitors(minute_values)/C/2001C/2001CALG/REME5M.TXT -- 5.0 Кб -- 04.10.2005
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26. NICMOS and the VLT: A New Era of High Resolution Near Infrared Imaging and
... ST-ECF, ESO, STScI and the NICMOS IDT organized a workshop on near infrared imaging from space and ground was held in Pula on May 26-27, 1998. ... The meeting was held in May 1998, about one year after science observations started with NICMOS, and about half a year before the Infrared Spectrometer and Array Camera (ISAAC) starts to operate on the VLT. Currently, it is expected that NICMOS will operate until the end of 1998. ...