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1. Temperature and humidity data
Next: Pressure Up: Additional information Previous: Additional information . ... Although the ESO Archive standard is to record temperatures in kelvins, this is often inconvenient. ... Therefore, if the temperatures are not in kelvins, the appropriate units should be provided in the table file (if temperatures are in a column), or as a comment. ... If filter and detector temperatures are otherwise regulated or recorded, it may still be useful to record DOMETEMP in the data file as a Real*4 column. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node642.html -- 5.6 Кб -- 23.02.1996
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2. Very Low Mass PMS Objects
... Since the reddening found for the stars in Table 13 was small, no reddening correction was attempted. ... These diamonds indicate the positions of very low mass, 3 Myr old, objects from the work of Burrows et al. ... This optical V versus R - I scheme is a very powerful method of detecting very low mass (VLM) objects. ... Because of this, young brown dwarfs are intrinsically no more difficult to observe in the optical than low mass stars at the age of Orionis. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~swolk/thesis/optical/node11.html -- 8.5 Кб -- 02.10.2012
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3. ALFA Receiver Temperature Polynomial Fit
Note: These models for T-receiver are based on measurements for all of the 14 pipelines. download Trx polynomial fit parameters . ... any additional offset to be addded as a correction not incorporated in the model (e.g. the contribution to receiver temperature from beyond the pre-amplifier stages), . ... No. of coefficient pairs, n_harm, associated with the harmonic (Cos & Sin) part of the fit (where the final fit is a simple sum of the two parts).. ... cos(j*pi*X/2) & sin(j*pi*X/2), . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/alfa/performance/spectral-scans/Trx/Trx_polyFit.shtml -- 7.2 Кб -- 05.02.2013
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4. Initial ``fixes'' to millimetre data
... The next step after loading is to apply a number of ``fixes'' that are important for 3-mm data. ... By default atfix applies the ``standard'' gain/elevation model for the antennas. ... As mentioned above, the ATCA uses the chopper wheel method to measure an above atmosphere system temperature. ... On the night of an ATCA reconfiguration, a solution for the antenna positions is derived. ... Task atfix corrects the data for an improved antenna location solution via the dantpos parameter. ... ATFIX . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/userguide/node209.html -- 9.8 Кб -- 10.04.2016
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5. ARC 3.5m | GFP
... ARC 3.5m | GFP . ... Install Appropriate Filters and Edit filters.txt file . Edit filters.txt file on aiscam@finesse in /home/aiscam/config . ... It also loads the filter info and the gfp.cfg settings including the calibration file for the appropriate course z-setting . aiscam: etalon in ;load etalon into optical path . ... aiscam: fpzero -w 4044.4 -1591.47 ;set fpzero with wavelength and central z . ... aiscam: time 40 . ... aiscam: file bias ;set filename for biases, no time needed . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/arc35m/Instruments/GFP/ -- 10.9 Кб -- 05.03.2014
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6. Saturn's Moon Titan
Titan . ... Hubble Space Telescope Images of Titan's surface . ... Later that year, it will release the European-built Huygens probe for a descent through Titan's atmosphere. ... This artist's rendering shows the European Space Agency's Huygens probe descending into the atmosphere of Saturn's moon Titan after being released by NASA's Cassini spacecraft. ... This artist's rendering shows the Huygens probe on the surface of Saturn's moon Titan after being released by NASA's Cassini spacecraft. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/solar/eng/titan.htm -- 11.2 Кб -- 15.10.1997
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/titan.htm -- 12.2 Кб -- 15.03.1998
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7. Frictional heating [Oulu]
... Electric field is a potential heat source for ionospheric particles (Rees, 1989). It is due to the fact that, under the action of an electric field, charged particles drift relative to one another and relative to neutral particles. ... This is called frictional heating. ... However, the effect of frictional/Joule heating of neutrals in the auroral electrojet region can lead to upward neutral wind in a region of high electron densities and strong electric fields (Winser et. al., ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/friction.html -- 8.2 Кб -- 21.12.2007
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8. TS33F-M Wireless remote temperature and humidity sensor
STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Remote Sensors . ... TS33F-M Wireless remote temperature and humidity sensor . ... Wireless remote temperature and humidity sensor #TS33F-M. Reads and displays both temperature and humidity at unit location on the built in LCD display. ...
[ Сохраненная копия ]  Ссылки http://www.meade.com/ts33f-m-wireless-remote-temperature-and-humidity-sensor.html -- 84.6 Кб -- 09.04.2016
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9. Thin Film Oxide Electronics Laboratory. Equipment
The HTSC group has an access to a set of technological equipment for thin film preparation and laboratory measurement system for low temperature electrical measurements. The technological complex of the " Thin Film Oxide Electronics " Laboratory includes two clean rooms of the "1000" class, with a complete set of equipment for photolithography (spinner, oven, hot plate, mask aligner, chemical bench, de-ionized water source) in each clean room. ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/html/oxide233/equipment.htm -- 16.6 Кб -- 29.01.2008
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10. Additional Data
... Gravity Esc vel M.O.V Axial Ascend Peri- Equilib Surface Press Atmospheric Name (g) (km/s) (km/s) incl Oblate node helion (K) (K) (atm) Composition --------- ------- ------- ------ --- ... - ------ ----------- Mercury 0.378 4.44 47.87 0 48.35 77.44 449 440 0 -- Venus 0.907 10.36 35.02 177.36 76.72 131.56 328 730 93 CO2 , N2 Earth 1.000 11.19 29.79 23.45 .00335 354.90 102.83 279 287 1 N2, O2, Ar Mars 0.377 5.03 24.13 25.19 .00519 49.60 335.99 226 ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/tnp/data2.html -- 4.4 Кб -- 01.10.2012
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11. http://www.mso.anu.edu.au/seminars/abstracts/20150619-1400.html
... Additionally, noise from stellar activity is becoming increasingly important, particularly in giant stars, where the amplitude of pulsations is comparable to RV signals from hot-Jupiters. ... This is impractical using large telescopes, but possible to do on bright stars with 0.2-0.4m class telescopes, provided they can be fitted with cheap high-