... Normally, cloud bottoms are flat . The flatness is caused by moist warm air that rises and cools and so condenses into water droplets at a specific temperature, which usually corresponds to a very specific height. As water droplets grow , an opaque cloud forms. Under some conditions, however, cloud pockets can develop that contain large droplets of water or ice that fall into clear air as they evaporate. ... Publications with keywords: clouds . Publications with words: clouds . ...

... 2004 June 7 . Mammatus Clouds Over Mexico . ... Normal cloud bottoms are flat because moist warm air that rises and cools will condense into water droplets at a very specific temperature, which usually corresponds to a very specific height. After water droplets form that air becomes an opaque cloud. Under some conditions, however, cloud pockets can develop that contain large droplets of water or ice that fall into clear air as they evaporate. ... About APOD | ... NASA Official: Jay Norris. ...

... Index / Home Page / Description / Basic Idea If there is a difference between the NEPDH counter (see Table 1), giving info on the number of events which have been transmitted from the Event Analyser [EPEA] to the Data Handling Unit [EPDH]) and the number of raw events in the corresponding time interval in all active CCDs for this quadrant then the interval associated with these raw ...

... User Portal . ... Science Users Information > Observing with ESO Telescopes > Phase 2 Preparation > Phase 2 Instrument Table . ... Phase 2 Instrument Table . ... Manuals and Tutorials . ... Calibration Plan . ... The P2PP Tool (version 3) . ... Phase 2 Users Workshops . ... If one instrument has special requirements, this is visualized in the relevant row of the table. A summary table of the main characteristics of all instruments is available here . Instrument . ... FAQ . ... User Manual . ...

The HyperNews Linux KHG Discussion Pages . Forum: Other Sources of Information . Re : Multi-architecture support ( Michael K. Johnson ) . Keywords: instructions kernel header file intro . Date: Mon, 27 May 1996 17:38:34 GMT . From: Drew Puch < aapuch@eos.ncsu.edu > . Here is some kernel info by header files . Thanks goes out to Michael Hohmuth of TU Dresden, Dept. of Computer Science, OS Group .

... SET/IRSPEC flat=.. ... SKYSUB/IRS . ... However, in SKYSUB/IRS you can avoid caring about the dark if -- and only if -- you use this command to make a straight subtraction (see last example of TUTORIAL/SKYSUB), in which case the dark frame is effectively not used. ... SKYSUB/IRSPEC . ... When using this mode remember to apply -- using the above command -- the same calibration to the object and to the standard otherwise you will not be able to run FLUX/IRSPEC. ... RECTIFY/IRSPEC . ... STANDARD/IRSPEC...

HST Call for Proposals and HST Primer for Cycle 24 . ... Hubble Space Telescope Primer for Cycle 24 > Chapter 6: Orbit Calculation for a Phase I Proposal > 6.2 HST Visits . ... HST Visits . 6.2.1 Defining New Visits and Optimizing Scheduling Efficiency and Flexibility . 6.2.2 Instrument Specific Limitations on Visits . ... STIS: CCD and MAMA Observations in the Same Visit . ... Most STIS coronagraphic observations will likely be single visits that use the full orbit for science observations. ...

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... This section gives a brief description of each of the parameters available to SCHED that are specifically for VLA observations or are especially useful for VLA observations. ... Should be provided for non-VLBI observations. ... This used to be required in order to obtain calibration data for the VLBI observations. ... FREQ: and DOPPLER Warning -- these parameters cannot be used for non-VLBI observations at the VLA since they are only used to adjust the baseband converter frequencies. ...

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Astronomy Discussion Forums . ... A Number Is A Very Specific Thing . ... Post Message | ... Posted by Harvey on October 9, 2002 16:41:15 UTC . ... When you use the word 'number', you are introducing a specific kind of symbol that is known within the context of mathematics. ... You know what - harvey1 - October 9, 2002 - 20:53 UTC . ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

Next: TAP 26 Up: Results Previous: Results . While the bulk of these stars were located in the Orion OB1a and OB1b fields, two stars of particular interest were monitored from our Mount Stony Brook Observatory. One of these stars was TAP 26 (NTTS 041559+1716, HBC 376). This star, located in Taurus, had a measured rotational period which was inconsistent with its . The other star was P1724, located near Orion OB1d, for which x--ray periodicity had been observed. TAP 26 . P1724 . ...

... In spite of the good potential possibilities, some of the station "Dnepr" design characteristics did not allow us to apply the usual special IS radar measurement methods. ... Thus for IS signal measurements at the "Dnepr" station, we have developed special methods for recording and processing IS signals in order to determine plasma ionospheric parameters. ... Equations (4-5) from the basis for data post processing to obtain ionosphere parameters. ...

. email: rgonzale@naic.edu

. Lines are sorted character by character, starting at the first character in the line. You can also sort the contents of a file on a specific part of each line. Each line of text is a series of fields - words and other characters - separated from each other by a delimiter character - the spaces between the words. Changing the field delimiter . Defining the sort field . Sorting on several fields . Sorting on a specific part of a field .

. Comedi Documentation . Prev . Next . comedi_maxdata_is_chan_specific -- maximum sample depends on channel . #include <comedilib.h> . int comedi_maxdata_is_chan_specific (comedi_t * device, unsigned int subdevice); . If each channel of the specified subdevice has different maximum sample values, this function returns 1. Otherwise, this function returns 0. On error, this function returns -1. Prev . Home . Next . comedi_range_is_chan_specific . Up . comedi_get_maxdata

Next: The ESO VLT CCD Detectors Software . ... Up: Instrument-Specific Software . ... The framework for data calibration and analysis of the VLT instrumentation is presented, based on the concepts of a calibration plan, pipeline calibration, quality control, and archiving of calibrated data for a ground-based observatory. ... Quality Control Pipeline provides quality assessment for instrument performance data and observing conditions, and tests the results of the Reduction Pipeline. ...

... Copyright of Images . I would like to thank each one of you who has taken the time to browse through this tour of the solar system. ... Here are some general conditions for use of this information. The Views of the Solar System web site along with many of the images and information are copyrighted by Calvin J. Hamilton . Many of the images come from NASA or other government sources and are in the public domain. ... Any NASA or JPL image can be freely used, but please give them credit. ...