... UPS Mustek . ... Max . Average . Current . ... 100.0 % (100.0%) . ... 7.0 % (7.0%) . ... Incoming Traffic in Bytes per Second . ... Outgoing Traffic in Bytes per Second . ...
The "red leaks" in the UV filters are shown in Figure 3.10 for F122M, F160BW (the new Wood's filter), F170W, F185W, F218W F255W, F300W, and F336W. The presence of significant red leaks in the UV filters, together with the much greater sensitivity and wavelength coverage in the red part of the spectrum, makes calibration of UV observations difficult. ... Figure 3.10: UV Filter Red Leaks. ... Table 3.13: Red Leak in UV Filters. ... Filter Central (nm) . ... 0.4 . ... 100.0 . ...
... Анк а дня . ... 7 марта 1494 года было видно полноеn (тип Tn) затмение с максимальной фазой 1.037 в 13:59 UT в точке с коодинатами 71.4 северной широты 100.0 западной долготы. Продолжительность затмения 02 мин. 05 сек. Это затмение является затмением 102-го сароса . 30 августа 1494 года было видно частное (тип P) затмение с максимальной фазой 0.651 в 21:40 UT в точке с коодинатами 71.8 южной широты 141.6 восточной долготы. ... Посмотреть затмения на другой год или вернуться в календарь ? ...
pro wtcalc, bwt, bmask1 print,"Set the percent level below which to delete " dellev=1.0 read,dellev dellev=long(dellev) adim=size(bmask1,/dim) dellev = float(dellev)/100.0*float(adim[2]) bwt[*,*]=adim[2] for yi = 0, 5 do begin for yk = 0, 1023 do begin bwt[yk,yi] = total(bmask1[yk,yi,*]) endfor bwt[*,yi] = (bwt[*,yi] gt dellev) * bwt[*,yi] ;bwt[*,yi] = (bwt[*,yi] lt dellev) * bwt[*,yi] endfor end
Communications For Your Astronomy Event . ... For many years two-way radios had a feature called by many names including Motorola's Private Line, GE/Ericsson's "Channel Guard", E.F. Johnson's "Call Guard", RCA's "Quiet Channel." ... Some call it by the most correct name (probably) of Continuous Tone Coded Squelch System (CTCSS). ... Since most radios seem to have adopted a 1 - 38 sub-channel system we at last have a way to express what CTCSS tone we all wish to utilize with a simple number. ... Tone . ...
bx = EXP(A[1] * X) F = A[0] * bx + A[2] IF N_PARAMS() GE 4 THEN $ pder= [[bx], [A[0] * X * bx], [replicate(1.0, N_ELEMENTS(X))]] END function intenzity,pole vel=n_elements(pole(*,0)) intt=make_array(vel,2,/float) intt(*,0)=pole(*,1) atlas=make_array(4400,/float ...
... *solvesavefinishc***c*** Enter post processor and calculate the variance of the error weightedc*** with area.c***/post1resumesetc*** a01 = 2.749e-04a03 = -3.482e-09a05 = 1.475e-14a07 = -1.387e-22vsum=0.0c*** nd01 =528* get ,uy1, node , nd01-1 ,u,y* get ,uy2, node , nd01 +1,u,y* get ,x1, node , nd01-1 , loc ,x* get ,x2, node , nd01 +1, loc ,xsplg=(uy1-uy2)/(x1-x2)* get ,t1, node , nd01 , loc ,xt1=( ...
... The package stsdas.graphics needs to be loaded (to run imdisp_pos for getting # the NDC's of the display image) # set imtype="fits" # print " " print " *** Start of impol FOC demo *** " print " [stecf.impol and stsdas.graphics need to be loaded] " print " " # # (First delete any model reflection nebulae left over from previous demos) # print " Deleting any old demo files " imdel reflneb1*.fits verify=yes # # An input (intensity) image is required. ... First delete any previous list files # ! ...