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. ...

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... 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. ...

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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), . ...

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• radar

... 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 . ...

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• Self-Calibration
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... 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 . ...

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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. ...

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... 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., ...

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• Space Weather Dials Interpretation Guide
• Additional Data
• Dayside aurora [Oulu]

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. ...

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• TS34C-M Wireless long range remote temperature sensor
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• TS34C-M Wireless long range remote temperature sensor - Remote Sensors -

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. ...

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• Project 4 - RFBR - Stepantsov, Determination of the space anisotropy of order
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... 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 ...

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• Light Curve Templete/Observing Form For Visual SNe Observers.

... 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-resolution spectrographs. ...

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• Siding Spring Survey Follow-up Obs
• Although the cement render is flaking off and all wooden doors and hatches are

Below is a table of INTERBALL-2 experiments summary to remind you about specific features of each instrument. ... See bottom of the page for additional information. ... AURORAL PLASMA . ... Spectra of electrons and ions 0.03 < E < 15 keV; anisotropy of electrons and ions (M = 1, 4, 16), 30 < E < 500 keV/Q . ... IKI, Moscow, Russia . ... Electron and ion spectra and anisotropy (M = 1, 2, 4, 16), 0.005 < E < 20 keV/Q . ... Ion composition (M = 1-32) and 3-D energy distribution, 10 eV < E < 30 keV/Q . ...

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• Tail Probe | Additional Information
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Subject, Object and Problems of Astrophysics. Practical and Theoretical Astrophysics. ... Visual Telescope; Problems Which Are Solved with the Its Help. ... Resolution of Telescopes. ... Effectiveness of Telescope in Respect of Resolution. ... Optical Power of Telescopes for Star-like and Extensive Objects. Boundary Magnitude. Reasons of Light Dissipation in Telescopes. ... Spectral Instruments in Astrophysics. ... Basic Photometrical Ideas, Magnitudes and Their Measurement. ...

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Chair of solid state physics . ... Students and postgraduate students . ... The following topics are included: acquaintance with a LabView software most often applied in laboratories to automation of experiment, a photolithography without which the modern manufacturing techniques of low-dimensional structures is impossible, as well as the tasks allowing students to master bases of low-temperature experiment, a technique of a high pressure, work with low-dimensional semiconductor structures. ...

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• Phys. Rev. Lett. 72, 3092 (1994): Neminsky et al. - Temperature dependence of
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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . Armagh Observatory reports that July 2014 was warmer and drier than the average July at Armagh, although there were only a few days with no precipitation at all. The number of hours of strong sunshine, 148.7 hours, was about average. The mean monthly temperature was 16.7 degrees Celsius, approximately 1.0 degree Celsius warmer than the most recent (1981тАУ2010) 30-year average for July. ...

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... User Portal . ... Science Users Information > Observing with ESO Telescopes > Phase 2 Preparation > Additional Information . ... Service Mode Philosophy . ... DDT Observation . TOO Observation . ... Additional Information . Phase 2 Users Workshops . User Feedback . The User Support Department . This section gathers information on past events and documents of interest to ESO telescope users: . Presentations from Phase 2 Users Workshops . Results of User Feedback campaigns . ...

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Pulkovo NEO Page . ... Instrumentation and Observations . ... This Windows application serves for determination of spherical coordinates and magnitudes of the objects. ... The objects coordinates are referred to the system of chosen star catalog. ... 2. choice of reference stars with mouse, . 3. measurement of rectangular frame coordinates of objects and reference stars taking account of predefined background parameters, . 4. calculation of the spherical coordinates of objects. ...

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Next: Historical Notes Up: The Chirplet Transform: Previous: The Chirplet Transform: . ... One of these TF methods, the short-time Fourier transform (STFT), has been used extensively for analyzing speech, music, and other non-stationary signals. ... Another time-frequency representation (which might more appropriately be called a time-scale representation) is the well-known wavelet transformheil-walnut,mallat:theory,daubechies:transform,strangwavelets. ... Historical Notes . ...

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• Additional problems at the transition

Microsymposium 38, MS082, 2003 (A4 format) EVALUATING THE STRUCTURE OF THE SURFACE LAYER OF MERCURY. ... Photometric Analysis of the Lunar Surface Analogue. ... The phase function obtained directly on some segments of the lunar surface: 1- phase function of the Moon, 2 - phase function of Mercury, 3 - phase function of segments, converted to the lunar phase function system (correlation 0.8), 4 - phase function of segments, converted to the Mercurian phase function (correlation 0.9). ...

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• http://selena.sai.msu.ru/Pug/Publications/ms34/MS058.pdf
• http://selena.sai.msu.ru/Symposium/sternber.doc
• http://selena.sai.msu.ru/Symposium/sternber.pdf

. This artist s impression shows how photons in the cosmic microwave background (CMB) are deflected by the gravitational lensing effect of massive cosmic structures as they travel across the universe. Gravitational lensing creates tiny, additional distortions to the mottled pattern of the CMB temperature fluctuations. A small fraction of the CMB is polarized; one component of this polarized light, B-modes, have been given an additional signature by gravitational lensing. ESA/Planck Collaboration

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA5F15BE3-08D5-4AA1-91DC-C1743ED7FD1A%7D
• How does the New Horizons mission team intend to target additional objects in
• Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets,