move_it (version 7/05/06) . ... Don Chance . ... 8/17/05 Chance modified hash-bang for move to python 2.4.1 . ... 10/18/05 Chance add verified constraint window controls . ... separate summaries. do move_it 01198A 2002.007 2002.021 . ... move into that interval from LRP 01198A. Produce both summary files. do move_it 2002.161 2002.175 2002.007 2002.021 . ... from LRP 01198A. Produce only the report showing visits which cannot move (stuck.rpt). do move_it 01198A 2002.161 2002.175 2002.007 2002.021 m . ...

... Archives . ... ArXiv] Kernel Regression, June 20, 2007 . Quote of the Week, June 27, 2007 . Jun 27th, 2007| 02:23 pm | ... Comments on the unified approach to the construction of classical confidence intervals . ... I?ve heard a few discussions about classical confidence intervals and upper limits from particle physicists and theoretical statisticians. ... Tags: confidence interval , coverage , flip-flopping problem , upper limit . ... Chandra Blog . ... SAMSI AstroStat Prog. ...

The technical memorandum: Time and Time Interval Measurement with Application to Computer and Network Performance Evaluation (PostScript) describes a number of techniques for conducting experiments typical of computer network and transmission systems engineering. ... The usual data collected during a performance run of some experiment might include time offsets, time delays, frequency offsets and various error statistics. ...

M obile A stronomical Sy stem of TE lescope- R obots MASTER-II Kislovodsk Lomonosov Moscow State University, Sternberg Astronomical Institute , Moscow Union "Optic" , Kislovodsk Solar Station Latitude = 43 o љ44'.767љN; Longitude = 42 o љ31'.417љE; Altitude = 2067љm MASTERљIIљ(8љsquareљdegress) + MASTERљVWF(VeryљWideљFieldљCameras (FOV=800 square degrees, Timeљresolutionљupљtoљ150љms, with unfiltered m_lim=14m on 5 sec. exposure, and ~10.5m with 0.15 sec) . ... 11h 38m 38.0s , -09d 59m 59s) . ...

... Punta salinas blanks their radar in the AO direction. ... Prior and after this test, the blanking region was set to 90 degrees ( +/- 45 degrees in the AO direction). In nov13 I noticed that the blanking had been changed to 22 degrees. ... The plots below show total power vs time for the mode A frequencies of punta salinas (1232.8,1242.2,1248.9, 1257.0). ... 14may12 (.ps) ( .pdf ) . ... punta salinas blanking sector changed from 78 deg to 22 degrees sometime between 14may12 and 22jun12 . ...

MODULE INTERVAL _ARITHMETICS TYPE INTERVAL REAL LOWER , UPPER END TYPE INTERVAL INTERFACE OPERATOR (+) MODULE PROCEDURE INTERVAL_ADDITION END INTERFACE INTERFACE OPERATOR (-) MODULE PROCEDURE INTERVAL _SUBTRACTION END INTERFACE INTERFACE OPERATOR (*) MODULE PROCEDURE INTERVAL_MULTIPLICATION END INTERFACE INTERFACE OPERATOR (/) MODULE PROCEDURE ...

Collection of the orbital elements | ... The errors of the spacecraft motion extrapolation outside the measuring time interval were estimated by using the comparison of SC positions calclulated by the forward integration ( extrapolation method) and backward integration ( interpolation methods). ... The character of these time shift of the ascending nodes ( D Tn) corresponds to the orbiting period errors, which arise during SC motion extrapolation outside the measuring intervals. ... INTERBALL mission ...

There are two modes to specify the time interval of ephemeris. ... This mode is applicable if the date of opposition belongs to the basic interval of 16 months from November of the year preceding to the title one to February of the subsequent one. In this case the ephemeris is centered at the nearest standard moment (its Julian day minus 0.5 is exactly divisible by 10) which precedes or coincides with the moment of opposition of minor planet in specified year. ...

... They are concerned with Attitude Control System of the spacecraft, satellite visibility from tracking stations, limits on the satellite autonomous operations during the orbit, and needs for auxiliary operations with the spacecraft. ... Among the operational constraints the most important one is the number of programmed slews per orbit, which determines the maximum number of radio sources to be observed during one orbit. ... System temperature (K) . ... Progress of the RadioAstron Project in Pictures...

... Connecting the planned observations and the actual status of the Chandra X-ray Observatory is the observation interval determination pipeline ( OBIDET ). This collection of tools allows the Chandra X-Ray Center Data System automated processing to process the data through the necessary pipelines based on what was actually observed. ... In the case of the Chandra X-ray Observatory, the observation interval determination pipeline ( OBIDET ) is used for this task. ...

... User Guide ] Task: mfcal Purpose: Multifrequency antenna and passband calibration. ... No default. This can (indeed should) contain multiple channels and spectral windows. ... Key: flux Three to five numbers, giving the source flux density, a reference frequency (in GHz) and the source spectral index parameters. ... Key: interval This gives one, two or three numbers, all in units of minutes, being used to determine the lengths of the antenna gain and passband calibration solution interval. ...

... R = 2.5R0 [6]. ­ .. 1 330 o () () 15 o 60 o 105 o 150 o 195 o 240 o 285 o 330 o 1980 1985 1990 1995 2000 1988 1989 1990 1991 1992 1993 II 330 o I II I II I ( ) , >90 o () 15 o 60 o 105 o 150 o 195 o 240 o 285 o 330 o 1978 1979 1980 1981 1982 1983 1978 1979 1980 1981 1982 19 83 . ... 105-150 285-330 () . ... 135- , , .. ... 5 330 o 105 o 150 o 285 o 330 1978 285 o o 1979 1980 () 1981 1982 1983 60 o 105 o 240 o 285 1988 o 1989 1990 ( ) 1991 1992 1993 . ... 105-150 285-330 21- 60-105 240-285 22-, : . ...

... Directives | ... Apache HTTP Server Version 2.2 . ... This module controls the setting of the Expires HTTP header and the max-age directive of the Cache-Control HTTP header in server responses. The expiration date can set to be relative to either the time the source file was last modified, or to the time of the client access. ... access . ... If set to On , the headers will be added to served documents according to the criteria defined by the ExpiresByType and ExpiresDefault directives ( q.v. ). ...

A year is a time interval approximately equal to the period of the Earth's rotation around the Sun. ... 2) a tropical year is a time interval between the Sun's two centre successive passing through the medium point of the vernal equinox (365,2422 days); . 3) anomalistic year is a time interval between the Sun's two centre successive passing through the perihelion of its visible heliocentric orbit (365,2596 days); . ... 6) lunar year includes 12 lunar synodic months (about 354, 367 days); . ...

This module provides for the generation of Expires HTTP headers according to user-specified criteria. ... This module controls the setting of the Expires HTTP header in server responses. The expiration date can set to be relative to either the time the source file was last modified, or to the time of the client access. ... ExpiresByType . ExpiresDefault . The ExpiresDefault and ExpiresByType directives can also be defined in a more readable syntax of the form: . ... Module: mod_expires . ...

T his page contains synthetic Hertzsprung-Russell Diagrams (HRDs) for a simulated Star Forming Region, assuming different scenarios and timescales for the history of star formation. ... In the paper we only presented the best fits to the HRD of the CMa R1 Star Forming Region. ... Download movie (1.90 MB) . Scenario II: Constant rate of star formation during a time interval delta t . delta t = 0.1 Myr . ... Scenario IV: Linearly decreasing rate of star formation during a time interval delta t . ...

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... subroutine attid1 (ts,u1,u2, dir ) common /z/ z(2) common /c/ x(12) dimension s(3),e(3),p2(3), dir (3), dra (3),pa(3,3) ux= atan (1.)/45.*u1 uy= atan (1.)/45.*u2 dra (1)= cos (ux) dra (2)= sin (ux)* cos (uy) dra (3)= sin (ux)* sin (uy) alf=x(1)+x(2)* sin (x(11)*ts)+x(3)* cos (x(11)*ts)+x(4)* sin (x(12)*ts)+ *x(5)* cos (x(12)*ts) bet=x(6)+x(7)* sin (x(11)*ts)+x(8)* cos (x(11)*ts)+x(9)* ...

1) Find the variable star and the comparison stars marked in the map. 2) Seeing the the variable star, try to imagine its location in the brightness interval between the reference stars. 3) Looking at the specially prepared scale, try to reproduce the location of variable in the brightness scale from memory. ... The grades of arbitrary scale are marked relative to brightness intervals between the reference stars. ...

The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Re : Timers don't work?? ( Joshua Liew ) . Keywords: timer . Date: Wed, 03 Dec 1997 01:25:06 GMT . From: Balaji Srinivasan < balaji@hegel.ittc.ukans.edu > . The mistake with your code is that you need to . update INTERVAL every time you add_timer. The expires field in timer_list is an absolute . time not a relative time. for example: . irq() { . timer.expires = jiffies + INTERVAL; . add_timer(&timer); . } .