... To access the measures do the following. ... Each of them can be either a scalar quantity with a scalar or vector for its actual value (see the following example):: from pyrap.quanta import quantity dm.epoch('utc','today') # note that your value will be different {'m0': {'unit': 'd', ' value ': 55147.912709756973}, 'refer': 'UTC', 'type': 'epoch'} dm.direction(' j2000 ','5h20m','-30.2deg') {'m0': {'unit': ' rad ', ' value ': 1.3962634015954634}, 'm1': {'unit': ' ...

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• Polarization/Stokes Handling (stokes and select)
• tmcvt
• ATNF Media Release - December 1, 1998

... Variations in water level along coastlines can be used to drive turbines technology is the same as low-head hydro power . ... Intermittent tidal flow is major problem. Tidal facility produces about 1/3 the electrical energy of a hydro facility of the same peak capacity . Two tidal plants in the world: . ... Bottom Line: There aren't many favorable sites in the world for tidal power and the estimated capacity is 50 times smaller than the world's hydroelectric power capacity. ...

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• Potential Energy
• Lecture XVII.

... When this mode is used, there is a potential error caused by the imbalance in amplitude and phase of the two signals (linear polarization) being input to the hybrid. ... Vaout,Vbout : Hybrid A,B voltage outputs. eps : The relative phase error between the two input signals. w : Frequency of the input signal. ... When a single diode is used (correlated cal.. eg. the calibration button on the gui) then eps is defined and the output cal value in the two channels will vary depending on the phase error...

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• http://www.naic.edu/~phil/hardware/cor/compareBandpass.html
• pntErrVsPlatformMotion
• rotaPlatToSky

Next: Gain steps Up: Additional information Previous: Measuring aperture . ... If the high voltage is changed to vary the gain, as is sometimes done in DC or CI work, the spectral response varies. This must be treated exactly like a variable measuring aperture: only data taken under constant conditions should be reduced together, but sometimes this can be done if adequate calibration data have been measured. The column label is PMTVOLTS. ...

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• Observational data
• Measuring aperture
• Sky problems

... 2000 October 19 . The Farthest Explosion Yet Measured . ... What is known is that satellites across our Solar System reported on 2000 January 31 a tremendous explosion of gamma rays had occurred towards some previously uninteresting direction. ... The VLT not only recorded an optical counterpart , shown above , but also was able to estimate that the cosmologically-induced redshift was an astonishing 4.5 -- placing GRB000131 farther across the universe than any explosion so measured. ...

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• APOD: 2009 April 29 - GRB 090423: The Farthest Explosion Yet Measured
• APOD: 2009 October 28 - JKCS041: The Farthest Galaxy Cluster Yet Measured
• APOD: May 30, 1999 - Tycho Brahe Measures the Sky

... One Jansky (Jy) is defined as 10 -26 Wm -2 Hz -1 , so it is a unit of measurement of the spectral flux density, F . ... 3x10 -12 . ... erg sec -1 cm -2 ?m -1 . ... where m is the magnitude and F o the zero-point flux for the given photometric band. ... Surface brightnesses are generally measured in Janskys arcsec -2 , MJy steradian -1 or magnitudes arcsec -2 . If you have a surface brightness S in MJy steradian -1 , then you can use: S [Jy arcsec -2 ] = S [MJy ster -1 ] x 0.084616. ...

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• Measuring Extinction Curves of Lensing Galaxies
• Gauging the impact of executing science program across different COS/FUV
• The Hubble Deep Field - Cosmic Ray Rejection

Galileo showed convincingly that heavy objects fell no faster that light ones. ... If an iron ball was pulled down with a much greater force than a wooden one of the same size, why didn't it fall any faster? ... 1) It is harder to lift. ... It is the fact that the loaded wagon has a greater mass that gives it a larger inertia , a larger tendency to oppose any change in its state of rest or of constant motion in a straight line. ... One important quantity was the body mass of the astronauts. ...

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• Field-aligned potential drops [Oulu]
• Space Weather Dials Interpretation Guide
• Radar aurora [Oulu]

... 18c. Work . An interesting thing about the final speed of an object descending (with no friction) from some given height h , along a sloping surface: one can change the slope, one can even change the shape of the surface--yet the final speed v with which it reaches the bottom will always be the same. ... Like currencies, different kinds of energy have a certain exchange rate: in the exchange between kinetic or potential energy and heat, for instance, one calorie equals about 4.18 joules. ...

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• Trigonometry beyond 90 degrees
• Energy--Lesson Plan #24
• Polar Orbiting Satellites

... In order to disentangle the effects of different climate variables on tree-ring growth rates of different species, and to explore the possibility that more than one species could improve the accuracy of the reconstructions of climate using tree rings, a methodical study of trees in close proximity to the Armagh Observatory climate station was initiated together with Ana Maria Garc?a Su?rez, and continued as part of the latter's PhD thesis with John Butler and Professor Mike Baillie (QUB). ...

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• Time zones
• Abstract
• Armagh Astronomers to observe Ringing Star with Global Telescope

... Archives . ... If you do not mind the time predictor, it is hard to believe that this is a light curve, time dependent data. ... It?s hard to say this data set is designed for time series analysis apart from the complication in statistical inference due to measurement errors. How to design the statistical study with measurement errors, huge gaps in time, and unequal time intervals is complex and unexplored. ... The following is R output without measurement errors. ... Chandra Blog . ...

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• zhtools
• Comments on: keV vs keV [Eqn] By: Simon Vaughan
• The AstroStat Slog measurement error

. Next: Output Up: Calling Parameters Previous: Calling Parameters Contents . rawX, rawY . - arrays with CCD pixel co-ordinates in the PIXCOORD reference frame . E . - arrays with uncorrected energies referring to the raw measured signal in ADU's. Note from above I suspect we need to convert all E1,E2,E3,E4 values (TBC) because the CTI correction may be proportionally different in the smaller peripheral charge cloud packets than in a combined event. Michael Smith 2011-09-20

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• Generation from In-Orbit Data
• Different types of detector map
• Generation from Ground Data

ON-LINE STATIC EIT RECONSTRUCTION SERVER . ... Static image reconstruction from the data measured in vivo is still intriguing problem in EIT. ... dipole (adjacent) current injection and voltage measurements on pairs of adjacent electrodes (like in Sheffield systems) . ... You can view examples of the text files for polar , dipole and trigonometric injection, use them for testing the server and find more details on HOW TO PREPARE INPUT FILE FOR THE ON-LINE EIT RECONSTRUCTION SERVER page. ...

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• Atmospheric influence on the different radioengineering systems functioning.

This lesson introduces you to the different types of uncertainty, and how you can estimate them from the scatter in your measurements, or from knowledge of your experimental set-up. It also outlines how to quote uncertainties. Back Main Uncertainties Page .

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• Clearing the library. Note the different floor levels. There were at least 4
• Proposed Facility
• Lab Skills Video Tutorials: Uncertainties

The HyperNews Linux KHG Discussion Pages . ... Keywords: scheduler overhead . ... From: Jasleen Kaur < jks@cs.utexas.edu > . Hi, I am implementing a different scheduling policy in the scheduler of Linux 2.0.0. I need to measure the time taken for choosing the next task to be scheduled, i.e., the actual time spent in the schedule() function, without the actual context switch having taken place. Since I clear interrupts in schedule(), how do I measure the time? ... Thanks, Jasleen Kaur . ...

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• APOD: 2000 September 28 - Heating Coronal Loops
• APOD: May 25, 1999 - NGC 6872: A Stretched Spiral
• Sakigake

... the time of observation . ... Observing the Changing Position of the Sun To Establish Cardinal Directions . ... Observations of the Sun's apparent movement across the sky and its pattern of rising and setting in the east and west horizon helped to establish the cardinal directions. ... The final stage of the Sun's return was marked by the observation that the Sun had reached its highest altitude when the full width of your mitted hand could fill the gap between the Sun and the horizon. ...

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• ASP: Good Astronomy Activities on the WWW
• ASP: Steering by Different Stars? Astronomers and the Dark-Sky Movement
• ASP: Cosmic Collisions

. This image is a screen capture of the full width half max of the imager array taken on February 15, 2000. The left portion of the image is simply the fwhm calculations for each of the chips in the array. On the right side is the estimated fwhm corrected for wavelength. This takes all the different filters and converts the estimated seeing as if it were in i' I believe. It is useful as a measure of the consistency of image quality across the array. As you can see, it is quite good! . long@apo.nmsu.edu

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• M1 Airflow Lab Tests
• Deforming Plug-plates
• Primary mirror support

. There are several different shells available for Unix; the most popular are described here. You can use any one of these shells if they are available on your system. And you can switch between the different shells once you have found out if they are available. Bourne shell (sh) . C shell (csh) . TC shell (tcsh) . Korn shell (ksh) . Bourne Again SHell (bash) .

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• Using a different printer
• Example of using a different printer
• Different types of file

Next: Model of clusters Up: paper2 Previous: paper2 . ... It allows estimating different microphysical properties of scatterers (size, complex refractive index, shape, etc.) from measured characteristics of the scattered radiation. ... The complexity of the direct problem depends on its input parameters characterizing the shape, size and structure of the scattering particle. ... Next: Model of clusters Up: paper2 Previous: paper2 root 2003-04-11 ...

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• Database of Optical Constants -- Level: welcome
• Nebular Abundances For PNe of Different Central Star Masses
• Examples of data contained in the JPDOC

To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...

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... Institute of Solid-State Physics, Russian Academy of Sciences, Chernogolovka, Moscow region, 142432 Russia . Received June 15, 2000) . Temperature dependences of the resistivity tensor components ab and c were measured for YBa 2 Cu 3 O 7 - x single crystals with different oxygen contents. The resistivity anisotropy c / ab was found to grow exponentially with decreasing temperature. ... PACS: 74.25.Fy, 74.72.Bk ...

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• Phys. Rev. B 54, 454 (1996): Neminsky et al. - ac susceptibility of Rb
• LPCBC: Abstract 2_29
• LEK - Equipment