... Opportunityт??s devilish view from on high . ... Does temperature have an upper limit like the lower limit of absolute zero? What's the highest measured value? ... The universe s absolute high temperature correlates to the energy and heat that existed during the Big Bang. ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ...

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 ...

IONOSPHERIC DATA h'F2 1.0 km Station PK553 PETROPAVLOVSK Time: UT ——————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————————— Data Sta 00 01 02 03 04 05 06 07 08 09 10 11 12 13 14 15 16 17 18 19 20 21 22 23 ——————————————————————————————————————————————————— ...

... When selecting the initial sources (up to about 3/4 of the total) in a geodetic sequence, SCHED tries to find one that are especially low or high at some stations. GEOLOWEL sets the upper bound of the region considered to be low. OPMINEL sets the lower bound. The related parameter GEOHIEL sets the lower bound to the ``high'' region. The default GEOLOWEL of 23 degrees has a SecZ of 2.55 which differs by 1.0 from the SecZ of 40 degrees, the default for GEOHIEL . ... Default: 23.0 . ...

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... INPUTS ; data the data (any IDL array) ; ; OUTPUTS ; out(0) = number of pixels ; out(1) = mean ; out(2) = median ; out(3) = standard deviation ; out(4) = minimum pixel ; out(5) = maximum pixel ; ; KEYWORD PARAMETERS ; lower lower limit of data to find stats ; upper lower limit of data to find stats ; nolabel output results w/o the column headings ; nobadval exclude BADVAL pixels from calculation of ...

... Meta Index / Home Page / DSS utilities . ... This is similar to RangeT except that no type is given for the upper and lower bounds. Where I have translated GTIs into ranges (see for example section 9.6.3 ) I have taken the lower GTI bound to be INCLUSIVE and the upper to be EXCLUSIVE. ... For each GTI in the sequence, the upper bound value must exceed the lower bound value. For all i from 1 to N-1, the upper bound of GTI i must be less than the lower bound of GTI i+1. ... See also section 16 . ...

The upper chromosphere and lower transition re­ gion of dMe stars A.C. Lanzafame Models for the upper chromosphere and the lower transition region of dM0e­ dM2e stars are presented. ... Ambipolar diffusion is found ineffective for the ionisation balance and therefore for the energy transport in the lower transition region of dMe stars. ... Key words: Stars: atmospheres ­ Stars: chromospheres ­ Stars: late­type ­ Radiative transfer ­ Line: profiles 1 ...

... SELECT s.id, CONCAT(UPPER(SUBSTRING(s.name,1,1)),LOWER(SUBSTRING(s.name FROM 2))) as name, CONCAT(UPPER(SUBSTRING(s.secondname,1,1)),LOWER(SUBSTRING(s.secondname FROM 2))) as secondname, CONCAT(UPPER(SUBSTRING(s.surname,1,1)),LOWER(SUBSTRING(s.surname FROM 2))) as surname FROM staff s, depstaff d, officercls o WHERE ((s.id = d.id_staff AND d.id_officercls=o.id AND o.id IN (85036001,85037001,86613001,99505462)) OR (s.id = 60918001) ) AND s.flag_hide=0 AND s.surname REGEXP '^Э'AND s.id != ... Тел.: ...

ESO PR Photo 18b/00 . ... Caption : Images of two of the novae in NGC 1316 that were discovered during the observational programme described in this Press Release. ... In particular, no less than four novae were detected in a single giant galaxy within only 11 days . ... Moreover, the discovery of four novae in one galaxy in the Fornax cluster was possible with only 3 hours of observing time per filter. ... ESO Press Information is available on the WWW at . http://www.eso.org/outreach/press-rel/ . ...

... As the SN activity in the first generation stellar population must be small at present, the net SN rate in the vicinity of the Sun is approximately proportional to the local density of stars of second generation (or to the star formation rate, which is the same), especially for SN II and SN Ib. If a -like star formation of the first generation stars took place, a hump on the observed - showing the relative fraction of the first generation stars should be observed. ...

Home - News - Download - Documentation - Search - FTP . About NEdit . ... Download . Get NEdit . ... Documentation . ... nedit man page . ... Mirror Sites . ... Mark Edel . ... Christian Denat . ... Back ] . Small macros to make upper/lower case. Change the case of the next character rather than the previous one. if ($selection_start == -1) { forward_character() uppercase() } else uppercase() if ($selection_start == -1) { forward_character() lowercase() } else lowercase() [ Back ] . ...

... Upper 2{sigma} error in GammaUV 25- 29 F5.2 --- e_GammaUV ? ... GammaUV is fitted at {lambda}_rest_<4200{AA}. ... ------------------------------------------------------------------------ 1- 11 A11 --- NSpect Spectrum name (G1) 14- 19 I6 km/s FWHM _ly Rest frame Full Width at Half Maximum of total Lya 22- 27 I6 km/s E_FWHM Upper 2{ sigma } error limit on FWHM of total Lya 30- 35 I6 km/s e_FWHM Lower 2{ sigma } error limit on FWHM of total Lya 38- 43 I6 km/s FWHM _c4 ...

... However, to avoid excessive central obscuration, a conical baffle is necessary in addition to the usual primary and secondary baffles. ... At that time, it was complete except several outside ribs remained to be attached and the upper and lower edges needed to be chamferred. ... The cone was measured at four equally spaced locations very near its upper and lower edge (Table 3). ... A tape measure was used to measure four diameters of the baffle at its upper and lower edges (Table 4). ...

Communications For Your Astronomy Event . Articles | ... GMRS has been around for many many years. ... If you are reading this you probably do not care about the old school and are only interested in what GMRS has to offer for your basic communication needs. ... However, you really only need to pay attention to the "Well Known Channel" the radio manufacturers like Cobra, Uniden, Midland, etc. seem to have agreed on. ... Channel . ... 462.5625 MHz . ... 5.0 Watts . ... www.astronomy.net . ...

The upper image above shows a 3 color image of the sky with RED=3.5 microns, GREEN=2.2 microns and BLUE=1.25 microns. ... The lowest level is 3.95 kJy/sr at 3.5 microns, 6.67 kJy/sr at 2.2 microns, and 7.08 kJy/sr at 1.25 microns for the upper and middle images, but 0.395 kJy/sr for the lower image. ... The lowest level is 223.2 kJy/sr at 240 microns, 555.3 kJy/sr at 100 microns, and 508.2 kJy/sr at 60 microns for the upper and middle images, but 30.7 kJy/sr for the lower image. ...

Markarians Chain of Galaxies . ... SSRO ) Explanation: Across the heart of the Virgo Cluster of Galaxies lies a striking string of galaxies known as Markarian's Chain. ... The home Virgo Cluster is the nearest cluster of galaxies , contains over 2000 galaxies, and has a noticeable gravitationally pull on the galaxies of the Local Group of Galaxies surrounding our Milky Way Galaxy . ... At least seven galaxies in the chain appear to move coherently , although others appear to be superposed by chance. ...

... autoOutline (int startX, int startY) . ... 0 and the boundary points can be accessed in the public xpoints and ypoints fields. public void autoOutline (int startX, int startY, double lower, double upper) . 0 and the boundary points can be accessed in the public xpoints and ypoints fields. public void autoOutline (int startX, int startY, int lower, int upper) . This is a variation of legacy autoOutline that uses int threshold arguments. public void autoOutline (int startX, int startY) . ...

Note: a new task -- "FLOPM" -- is available in recent versions of AIPS (31DEC07 and later), which also reverses the order of spectral channels, making UVFLP as described below unnecessary. ... UVFLP (to re-order channels in GMRT LSB uv data files within AIPS) ================================================================== To flip the oder of spectral channels in uv databases in AIPS. ... 1) Original data: 128 <--- channels <--- 1|1 ---> channels ---> 128 ------------------------|- LSB | ...

Computer Ephemeris for 2014 from DE200/LE200. Planetary configurations. Sorted by event. ...