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1. Energy From the Wind
... How much energy is there in a 20 mph wind? . 20 mph wind =10 m/s .0006 * 10 3 = .0006 * 1000 = .6 KILO watts per square meter . ... In your back yard the average wind speed is 10 mph which yields 100 watts per square meter. ... 4 3 = 64 if a 10 mph wind gives you 100 watts per square meter then a 40 mph wind gives you 64 times more power per square meter 6400 watts per square meter . total power = 6400 watts per square meter * 2 square meters = 12800 watts = 12.8 Kilowatts this is a lot! ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/1998/ph162/l11.html -- 10.9 Кб -- 14.10.1998
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2. Magnification (Power) And Using Eyepieces - an Astronomy Net Article
Magnification (Power) And Using Eyepieces . ... To determine power in a telescope, divide the focal length of the telescope by the focal length of the eyepiece. By exchanging an eyepiece of one focal length for another, you can increase or decrease the power of the telescope. For example, a 25mm eyepiece used on a telescope with a 1000mm focal length would yield a power of 40x (1000 / 25 = 40) and a 10mm eyepiece used on the same telescope would yield a power of 100x (1000 / 10 = 100). ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/articles/26/ -- 17.6 Кб -- 09.04.2016
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3. http://www.atnf.csiro.au/management/atuc/2011oct/science_meeting/docs/Ian_S_Morrison_ATUC_presentation_24-10-11.pdf
Advances in Wideband SETI and Implications for Radio Telescope Design Dr Ian S. Morrison 24 October 2011 Resurgence in SETI New generation radio telescopes and anticipation of the SKA Emergence of ` wideband SETI ' Successes in astrobiology, in particular exo-planet discoveries 2 1235 Kepler Worlds 68 288 662 184 54 are `habitable' Copyright © Jill Tarter, SETI Institute SETI by Eavesdropping Expect civilisations to have a short timespan for high power ...
[ Текст ]  Ссылки http://www.atnf.csiro.au/management/atuc/2011oct/science_meeting/docs/Ian_S_Morrison_ATUC_presentation_24-10-11.pdf -- 2640.4 Кб -- 23.10.2011
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4. Results
... We have been using it to analyze PC images of known gravitational lenses and QSOs which are candidates for lensing (Falco 1993). ... Fig. 1 plots the higher contours of the PC image of 0142 in the upper left, and its power spectrum in the upper right. ... If we fit the envelope of the power spectrum with a binary model, we find that best fit gives a separation of the two components of 1.3 PC pixels or about 58 mas. ... The lower two curves are cuts through the 0142 power spectrum. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/nisensonp.dir/section3_3.html -- 7.5 Кб -- 16.04.1994
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5. emerg_close
... The proper procedure to set up the wind baffle and enclosure to be powered by the emergency generator in the event that both commercial and site emergency generator power is lost. ... The enclosure should be open with telescope in an un-stowed position. ... Wind baffle (WB) control power switch ; Location : ?; ... Enclosure power switch box ; Location : ?; ... Change the WB manual pendent connector in WB control box to ALT Axis Brundy, make sure the "pot" is at "000" and the palm switch is depressed...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/25Procedures/Telescope/op020501emergenclose.shtml -- 10.7 Кб -- 09.05.2002
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6. http://www.naic.edu/~astro/aotms/backends/stokes-helix.pdf
The Handedness of Stokes V for the WAPPs at C-band Robert Minchin Using helical antennae illuminating the feed through a hole in the 305m reflector, circularly polarised tones were transmitted at 4800 MHz. ... Two power levels were transmitted, firstly a higher power and then a lower power (6 dB down). ... 2 Figure 2: Stokes V response in different WAPP boards to right-hand (upper) and left-hand (lower) transmission at lower power (-6 dB). ...
[ Текст ]  Ссылки http://www.naic.edu/~astro/aotms/backends/stokes-helix.pdf -- 176.1 Кб -- 03.09.2008
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7. SAO RAS home page
... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/ -- 11.4 Кб -- 09.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/ -- 11.4 Кб -- 09.04.2016
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8. East Siberian Center of Earth Ionosphere Research. Chirp ionosonde.
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Chirp ionosonde main technical characteristics . ... Linear frequency modulated continuous signals sounding method is relatively simple and has wide application in various special-purpose systems. ... Chirp signals which are applying for ionosphere channel diagnostics usually have10KHz/s -- 1MHz/s. We must point out that under modulation speed increasing there is an increase in noise suppression and resolution power. ...
[ Сохраненная копия ]  Ссылки http://rp.iszf.irk.ru/esceir/lchmen/ionozonden.htm -- 9.3 Кб -- 02.06.2001
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9. Meade Instruments Corporation - How to Calculate Power
... Meade Instruments Corporation . ... How to Calculate Power . How to Calculate Power: The magnification, or power, at which a telescope is operating is a function of the focal length of the telescope's main (objective) lens (or primary mirror) and the focal length of the eyepiece employed. ... Example: The Meade DS-2070AT telescope has an objective lens focal length of 700mm; when this telescope is used with a 25mm eyepiece, a power of 700/25 = 28 power (written as "28x") results. ... about meade | ...
[ Сохраненная копия ]  Ссылки http://www.meade.com/support/power.html -- 9.5 Кб -- 01.02.2006
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10. http://xray.sai.msu.ru/~ivan/gmt/man/grdproject.html
... If set, it will transform a gridded data set from a rectangular coordinate system onto a geographical system by resampling the surface at the new nodes. If not set, it will project a geographical gridded data set onto a rectangular grid. ... The new node spacing may be determined in one of several ways by specifying the grid spacing, number of nodes, or resolution. ... D Set the grid spacing for the new grid. ... N Set the number of grid nodes in the new grid. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~ivan/gmt/man/grdproject.html -- 8.1 Кб -- 19.03.1999
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11. Стразы пришивные "Астра", акриловые, капля, цвет: фуксия (02), 6 мм х 10 мм, 18
... Набор страз "Астра", изготовленный из акрила, позволит вам украсить одежду и аксессуары. ... ИБП Ippon Back Power Pro 500 New. Выходная мощность - 500 ВА/300 Вт. ...
[ Сохраненная копия ]  Ссылки http://astrokuban.info/astroku2624.html -- 25.8 Кб -- 14.02.2016
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12. Phil Plait's Bad Astronomy: Misconceptions
... Bad Astronomy . ... I think I will break from