There has been ripple in the lband wide bandpass near 1400 Mhz during the a1861 run of may04 and during the a1914 run in aug04. ... The first two sbc were polA, polB at 25Mhz while the last two sbc were polA,polB at 12.5 Mhz. When they observed above 1370 Mhz, the 1320 hipass and 1370 hipass wave guide filters were installed. ... Project a1914 used the 1st two sbc for polA and polB at 25 Mhz. ... Fig 1. (on/off-1) degK vs frequency with offsets for plotting. ... The bumps at 1381 Mhz are gps L3. ...

... НЕПРЕРЫВНОГО МАТЕМАТИЧЕСКОГО ОБРАЗОВАНИЯ . ... Кружок ?Олимпиады и математика? ... Московская математическая олимпиада . Заочный математический конкурс . ... Устные математические олимпиады . Олимпиады по программированию . Математический праздник . Математические регаты . ... Математические бои . Олимпиада по геометрии им. И.Ф.Шарыгина . ... Программа ?Math in Moscow? Научные конкурсы . Творческий конкурс . ... График олимпиад . ... XXVII Математический праздник . ...

Kermit output files are named ker number_object_filter_time .fits. number is a four-digit integer that increments for each subsequent exposure. object is the object name (with spaced removed) as entered by the observer. filter is the name of the currently selected filter wheel position. time is the current UTC time as a six-digit integer, HHMMSS. ... Kermit has three selectable pixel timing modes: fast readout, slow readout, and slow readout with reset. ... Kermit has three readout modes: . ...

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Chirp ionosonde main technical characteristics . ... Linear frequency modulated continuous signals sounding method is relatively simple and has wide application in various special-purpose systems. ... Chirp signals which are applying for ionosphere channel diagnostics usually have10KHz/s -- 1MHz/s. We must point out that under modulation speed increasing there is an increase in noise suppression and resolution power. ...

Describes how spatial region boundaries are handled. The golden rule for spatial region filtering was first enunciated by Leon VanSpeybroeck in 1986: . ... With this in mind, the rules for determining whether a boundary image pixel or table row are assigned to a region are defined below. For image filtering, pixels whose center is inside the boundary are included. ... That is, an row is inside the boundary without regard to its integerized pixel value. ...

... An OBJECT column gives the name of the object observed (usually a star name). ... In critical cases, it is common practice to measure sky on two or more positions around a target object, and these positions must be identified. ... A general treatment of this problem requires a column called OBJECT, bearing the usual name of the object (as in the star tables); a column labelled STARSKY, to distinguish between star+sky, star alone, or sky alone; and additional columns to identify the sky position. ...

Recent Changes - Search : . VLBI Schedule . ... Observers Wiki . ... Other VLBI . Recent Changes . ... Main / . A fine tuner profile has been setup which user a type 2 8 MHz bandsplitter filter (2x8 MHz ). A 0.5 MHz type 1 filter is then tunable within the 8 MHz . To center the 0.5 MHz filter within the 8 MHz filter the fine tuner NCO oscillator should be set to 4 MHz . If the tone is above the DAS central frequency choose the profile cassini_0.5MHz_ft.pro . ...

Next: NICMOS/HST H-band (F160W) Images Up: NICMOS Science Previous: HST NICMOS Observations of . ... Observations of P . ... The NICMOS team has devised a comprehensive program of observations of the Galactic Center. ... Data in hand give a first look at variability and a detailed look at the search for the tip of the main sequence will be discussed where NICMOS has demonstrated adequate sensitivity and photometric precision to identify likely O8-B1 stars at the Galactic Center. ...

... BDR FAX: (303) 497-6513 ------------------------------------------------------------------------------- SELECTED GEOMAGNETIC AND SOLAR ACTIVITY INDICES ------------------------------------------------------------------------------- WORLDWIDE INDICES -------------------------------------------------------------- The subscript p means planetary and designates a global magnetic activity in- dex ... 13-14 I2 Kp or PLANETARY 3-HOUR RANGE INDEX for 0000 - 0300 UT. ...

... Viking Orbiter Mission 1975 . ... YY = sequential number of image during orbit . FILTER . ... Scale of one pixel at center of image . ... Azimuth of (direction to) North, measured clockwise from zero line defined by a horizontal line drawn from the center of the image perpendicular to the right edge . SUN AZ . Azimuth of (direction to) Sun, measured clockwise from zero line defined by a horizontal line drawn from the center of the image perpendicular to the right edge . ... SUNS LS . ...

DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...

XMM­Newton CCF Release Note XMM­CCF­REL­55 OM Astrometry R. Much December 11, 2000 1 CCF components Name of CCF VALDATE List of Blocks changed CAL VERSION XSCS flag OM ASTROMET 0008 2000­01­01T00:00:00 FILTER­U Yes FILTER­B Yes FILTER­UVW1 Yes FILTER­UVW2 Yes FILTER­UVM2 Yes FILTER­WHITE Yes FILTER­MAGNI Yes FILTER­GRISM1 Yes FILTER­GRISM2 Yes POLYNOM MAP No 2 Changes Compared to the previous version the distortion maps of the U­, B­ and the three UV­filters have been updated. ... UVW2­positions). ...

... Each file has a header and number of data records. ... -23) 2 I3 Minute (0-59) 3 I3 Second (0-59) 4 I4 Millisecond 5 F3.0 Code F/S (1,2,3,4,5) Defines the pair of the electromagnetic field components measured, see Table 2.1 6 A3 Electromagnetic field component measured in the filters ACP1-ACP5 (BX, BX45 ,BZ,EH,EZ) 7 E11.3 Field Intensity in the Filter ACP1 nT/ sqrt (Hz) if BX, BX45 , or BZ; V/ m.sqrt (Hz) if EH, or EZ 8 E9.3 Field Intensity in the Filter ACP2 nT/ ...

... Институт прикладной математики им. М.В.Келдыша . БАЛЛИСТИЧЕСКИЙ ЦЕНТР . О Центре . ... Баллистический Центр Института прикладной математики им. М.В.Келдыша РАН . Баллистический центр (БЦ) ИПМ им. М.В. Келдыша создан по предложению С.П. Королева и М.В. Келдыша в 1965 году. На него были возложены работы по баллистико-навигационному обеспечению (БНО) управления полетом пилотируемых кораблей и автоматических космических аппаратов научного и народно-хозяйственного назначения. ...

... An Orion Deep Field . ... Adrift 1,500 light-years away in one of the night sky's most recognizable constellations, the glowing Orion Nebula and the dark Horsehead Nebula are contrasting cosmic vistas. ... This crowded star field towards the center of our Milky Way Galaxy turns out to be a great place to search for planets beyond our solar system. ... In the vast Orion Molecular Cloud complex, several bright blue nebulas are particularly apparent. ... Hidden Galaxy IC 342 . ...

... public class ParticleAnalyzer . ... static int . ... Add particles to ROI Manager. protected boolean . ... Clear ImageJ console before starting. static int . ... protected static int . ... Do not measure particles touching edge of image. protected boolean . ... Flood fill to ignore interior holes. protected static int . ... Display image containing binary masks of measured particles. static int . ... Field Detail public static final int SHOW_RESULTS . ... protected static final int NOTHING . ...

... PhD 1971 in Astrophysics . Doctoral Degree 1997 in Astrophysics . ... Department Number . 01 (Theoretical Astrophysics) . ... Astro Space Center . ... Telephone Number . 7(495) 333 3366 . FAX Number . 7(495) 333 2378 . ... rpol@asc.rssi.ru . ...

... Inst Data Fit allows one to determine various parameters needed for instrument data files, including: scale, orientation and the position of the rotator with respect to the instrument. ... Run Inst Data Fit. ... Specify all fields above the "Fit Scale and Orientation" button New Rot_Inst_ang . ... Modified the instructions so that new scale and orientation values are applied to the instrument block before measuring center-of-rotation data (to solve a problem brought to light by SPICam). ... R.O. ...