... The ultraviolet flux standard BD+28D4211 is observed with the GHRS and grat­ ing G140L to monitor the long­term stability of the instrument sensitivity between 1100 љ A and 1640 љ A. Four observations obtained on days 94.098, 94.164, 94.213, and 94.294 are avail­ able for the wavelength range 1100 љ A -- 1350 љ A. Data for the range 1350 љ A -- 1600 љ A are available for days 94.164, 94.213, and 94.294. ... As an example we show in Figure 1 the spectrum centered on 1200 љ A obtained on day 94.294. ...

Художественно-эстетическая направленность | Ф.И.О. |Пн. ... Сулаева Э.В. |1500- |1500-170|1500- |1500- |1500- | Золушка» |2000 |0 |1900 |1700 |2000 | ... 1600 - | 1600 - |1300 - | ... 1800 | 1800 |1500 | ... 1400 - | 1400 - |1000 - | ... 2000 | 2000 |1600 | ... 1500- | ... Мясникова Т.П. |1500- | 1700 - | ... Студия «Веер» |2000 | ... 1630 - | ... 1900 | Люкова О.В. |1700 - | ... 1700 - |1400 - | ... 2000 |1700 | ... Пискарева М.А. |1500-1700 | ... 1600-210|1700-19| ...

... Reception/Dinner (poolside) . ... Wake-me-up Coffee & Conference Registration (L.C.) . ... 0930 - 1030 . Science Highlights from the Arecibo & Green Bank Telescopes - C. Salter PDF & J. Lockman PDF . 1030 - 1100 . Coffee Break (V.C.) . ... Tracing the Signal down the Telescope - R. Maddalena PPTX . ... The Hands-On Projects - Organization and Logistics . 1730 - 1900 . Dinner with Hands-on teams planning strategy (poolside) . 1900 - 2100 . ... 1900 - 0000 . ... 0730 - 0830 . ...

... Acetone analysed by SERS C-phycocyanin OH O OH O 1230 1380 1448 O 1517 711 885 964 1000 1540 1560 1323 1553 N H N H N N H O H scytonemin N HO H O N O OH 1156 500 600 700 800 900 1000 1066 1100 1200 1300 1400 Raman Shift (cm-1) 1500 1520 , carotene 1176 1600 1608 1609 1700 1800 1900 2000 Biomolecules in hydrothermal system II scy scy phyc b,b phyc scy b,b b,b Green Orange Brown/purple D2 C­S, C=S C­O­C D1 Sinter Blank 500 ...

... 1419.977 . ... 1419.978 . ... NaN . 0.00E+00 . ... 1420.021 . ... 1420.023 . ... 1420.024 . ... 1419.976 . ...

... Астронет | ... Пояснение: Находящиеся на расстоянии 1500 световых лет в одном из самых легко узнаваемых на ночном небе созвездий , сияющая туманность Ориона и темная туманность Конская Голова представляют собой резко контрастирующие космические объекты. ... Публикации с ключевыми словами: Orion Nebula - M 42 - Horsehead Nebula - emission nebula - reflection nebula - dark nebula - Туманность Ориона - туманность Конская Голова - эмиссионная туманность - отражательные туманности - темная туманность . ...

... Справочник по полевым транзисторам . Транзисторы КП801 - КП840 . ... 100 . ... 2.5 . ... МДП . ... 1500- /3 . ... 100мкА . ... 220 . ... 1300-3000/2.5 . ...

... Wavelength Calibration . ... 30s wavecal plot . 30s flatfield plot . ... HeNeAr 4400 . B rQrtz 4400 . ... HeNeAr 4500 . ... BrQrtz 4200 . BrQrtz 4500 . ... These figures in the above table show the number of counts received from each of the lamps in a 30 second exposure with the 1.5 arcsec slit. ... Users have the option of taking calibration lamp data at the rotator angle of each object, but in many cases, it should be possible to measure the shift using observations of night sky lines. ...

... The first task assumes the searching for chemical composition and sizes of particles which give the wavelength dependence of the extinction efficiencies close to the observed dependence of . Figure 7: Wavelength dependence of the extinction efficiency factors for homogeneous spherical particles of different sizes consisting of astronomical silicate and amorphous carbon. The dashed segment shows the approximate wavelength dependence of the mean galactic extinction curve at optical wavelengths. ...

Next: Imaging Polarimetry with NICMOS Up: NICMOS Data Calibration and Previous: The Photometric Performance of . ... NICMOSlook and Calnic C . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... NICMOSlook and Calnic-C are two programs that were designed to take advantage of the fact that the NICMOS grism mode typically consists of taking both a direct and a grism image. ...

... You are here: start €Ё difx €Ё haystack2011agenda . ... difx:haystack2011agenda . ... Each day lunch will be provided, and we plan to have coffee, tea, and snacks at the breaks. ... 1045 Coffee break . ... mm VLBI, ALMA phasing, and the EHT - Shep Doeleman . ... 0945 Hack-a-thon . ... difx/haystack2011agenda.txt €§ Last modified: 2015/10/21 10:08 (external edit) . ... Except where otherwise noted, content on this wiki is licensed under the following license: CC Attribution-Share Alike 3.0 Unported ....

To a special Solar Physics issue on the Bastille Day Event: . ... Multi-scale temporal features of the 14 July 2000 meter-wavelength dynamic radio spectrum compared with TRACE data . ... Figure 1 (100 KB). SOHO/EIT (a) and LASCO/C2 (b) images show the region of the eruptive flare event of 14 July 2000 and related halo CME. ... Figure 2 (47 KB). ... Figure 3 (115 KB). Medium-scale dynamic spectrum (a), 204 MHz metric (b) and 3000 MHz microwave (c) profiles of the "Bastille Day" event. ...

- . . VIII « » . 9­10 2012 . 9 () -- 1100­1200 -- 1230­1400 -- 1500­1800 10 () -- 900­1300 -- 1400­1500 -- 1600 : -- -- -- -- -- -- 2012 . : 1. . 2. . 3. . 4. . 5. . 6. VII--XIV . 7. . 8. : 110- XII . 9 2012 . 800 : . , . 4, . . , ( , 5 ). . «» «». 10 2012 . : , , . . , . 4, . , 61077, . E-mail: hiao@mail.ru ( : Conference HIAO). : +38 (057) 707-51-66 -- ; +38 (057) 702-00-85 () -- ; +38 (050) 933-17-99 -- ; +38 (066) 293-47-30 -- . . . -- http://www-history.univer.kharkov.ua; http://khiao.wordpress.com/

... 940-1130 |1 заседание; председатель Е.Г. Понятовский | ... O-30 |Фуллерены под высоким давлением | ... O-25 |Непростое поведение простых металлов при высоких давлениях | ... Кинетика фазовых превращений при высоких давлениях. ... 1115-1130 |А.Э. Хейфец, В.И. Зельдович, Н.Ю. Фролова, Б.В. Литвинов, | ... Жуков, С.В. Кидалов, М.Н.Корытов, А.В.Нащекин, С.И.Розов, | ... 1250-1310 |А.В. Курдюмов, В.Ф. Бритун, Н.И. Боримчук, А.И. Даниленко, | ... Атомные колебания и фазовые переходы при высоких давлениях ...

ChangeLog for rgsspecplot =============================== Version 2.16.13 - 2002-12-12 (NW) ------------------------------- Changed the way of embedding figures to \epsfig, so that the figures appear in the electronic documentation. ... The documentation has also been updated. ... Version 2.17.2 - 2002-07-25 (NW) ------------------------------- Removed the dependency on the STAT_ERR column, now use the square root of the counts as the error, to close the SPR 2949, `Task unable to plot total spectrum'. ...

Приложение 2. ... figure . subplot(2,1,1); . plot(t,y) . zoom xon . yfft=abs(fft(y)); . ... plot(freal, abs(h)) . plot(freal, abs(h).*abs(h)) . ... title ('а') . ... soutfft=abs(fft(sout1)); . ... flen=length(fhis); . ... plot(fhis(1:flen),sumyfft1(1:flen)) . ... plot(fhis(1:flen),sumsoutfft1(1:flen)) . ... plot(fhis(1:flen),sigrechis(1:flen)) . ... plot(freal, abs(h).*abs(h),'r',... fhis(2:flen), sigrechis(2:flen).*sigrechis(2:flen)) %,... % fhis(2:flen), sumsigrec2(2:flen)) . ...

... Resolution - 1.5-2.0 km . Swath - 450 km . ... Swath - 550 km . ... Resolution - 370 km . ... Spectral bands - 0.6-0.7 um; 0.8-1.1 um . ... Kondor - system for collection and transmission of data from sea and ice stations . ... Downlinking to ground stations (main centers) . ... Satellite's information system operates in both direct transmission mode and recording to on-board recorder mode with later downlink to ground station. ... For more information send a mail to: info@sputnik.infospace.ru . ...

Next: Results & Discussion Up: Coronal Hole Diagnostics out Previous: Introduction . ... The dates of the observations discussed here, their locations, pointing, slit sizes and exposure times are given in BTDW. ... Line fits are given by the dotted line. ... An estimation of the errors in the derived parameters was obtained using the GA-derived parameters as an input for a ``classical'' IDL-CURVEFIT procedure (Peter, 1999; Peter & Judge, 1999). ...

. F IGURE . 3. Plots of V S against cos for the thick disk and the old halo samples. In this graph a constant V rot appears as a straight line. Higher-weight points are plotted with larger symbols. discussion in the text | previous figure | next figure .

. Density plot as given by our finite-difference SFS method with gamma=1.2 at T=20 orbital period. Postscript version . If you have comments or suggestions, email me at spxhmjb@astro.cf.ac.uk Last update: May 26, 1998 .