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http://www.sai.msu.su/~megera/gimp/cooltype/hint18/.
http://www.sai.msu.su/~megera/gimp/cooltype/hint18/.
1. CoolType - Glass
... My very last technique, for Photoshop 3.0, that simulates a glass type over a picture. ... STEP 1 . ... Create a new channel (name it "Type") and type your text, with a normal font (here I used Helvetica Extended 80 pts). ... Duplicate this channel and name it "Blur type". Apply Gaussian blur (2 pixels). Duplicate this channel 3 times and name them "Bold Type", "Horizontal displace", "Vertical Displace". ... Load selection from the "Bold Type" channel and apply the "Highlights" channel. ...
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Ссылки http://www.sai.msu.su/~megera/gimp/cooltype/hint19/ -- 5.8 Кб -- 22.12.2007
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2. High-resolution Herschel spectroscopy reveals the proto-planetary disk around
... High-resolution Herschel spectroscopy reveals the proto-planetary disk around the young star T Tau N . ... A study led by Linda Podio ( AstroFIt fellow at the Arcetri Observatory) with Inga Kamp (Kapteyn Institute, the Netherlands), Claudio Codella (Observatory of Arcetri) and other collaborators from Grenoble, UK and USA, makes use of high-resolution spectroscopic observations with HIFI on board the Herschel space observatory to characterize the disk around the young star T Tau N . ...
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Ссылки http://www.arcetri.astro.it/en/previous/204-scientific-news/713-ttaundisk -- 26.2 Кб -- 10.04.2016
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3. Home Page
... The 99 files presented here contain 21 cm HI emission contours around 98 Super Nova Remnants (SNR) in the - V coordinates. ... SNR's were selected mainly from the List of Green (2001) [4] and from some other papers with angular diameters more than 10' and morphological type in continuum emission - S (shell). Four files each contain two objects (these objects have near declinations). ... b) emission of structureless medium, . ... Astrophys. ... Gosachinskij I.V., Bull. ... Gosachinskij I.V., Astr. ...
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Ссылки http://mavr.sao.ru/hq/lrs/supern_en.html -- 3.9 Кб -- 09.04.2016
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lrs/supern_en.html -- 3.9 Кб -- 09.04.2016
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lrs/supern_en.html -- 3.9 Кб -- 09.04.2016
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lrs/supern_en.html -- 3.9 Кб -- 09.04.2016
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lrs/supern_en.html -- 3.9 Кб -- 09.04.2016
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4. Thesis Figures
... Values have been scaled arbitrarily. High ratios are shown in blue, corresponding to blue colors, and low ratios are shown in red, corresponding to red colors. ... Noise combined with background subtraction difficulties in the lower left quadrant of the WISP1 data (see Fig. \ref{Fig:wisp_snr_mskd}) make colors in this area very unreliable. ... The values shown here are typically a factor of ~3 less than those calculated for the Schmidt data, shown in Figure \ref{Fig:bj_alpha}. ...
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Ссылки http://www.naic.edu/~gibson/thesis/fig/fig_ch4.html -- 8.9 Кб -- 27.06.1999
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5. SAO RAS home page
... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...
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Ссылки http://www.sao.ru/ -- 11.4 Кб -- 09.04.2016
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/ -- 11.4 Кб -- 09.04.2016
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[ Сохраненная копия ] Ссылки http://mavr.sao.ru/ -- 11.4 Кб -- 09.04.2016
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6. Astrophysics Group VSA
... Astrophysics Group . ... VSA . ... CAT . ... The Very Small Array is a custom-built radio telescope (operating between 26-36 GHz), designed expressly to make high resolution observations of the cosmic microwave background (CMB) radiation on angular scales around and below one degree. ... The VSA has been operated in ?compact array? and ?extended array? configurations (see the technical description below) and data collected to achieve high sensitivity in both regimes have been analysed. ... 1.75 GHz)...
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Ссылки http://www.mrao.cam.ac.uk/outreach/radio-telescopes/vsa/ -- 20.2 Кб -- 10.04.2016
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7. High Spatial Resolution Mid- and Far-infrared Imaging Study of NGC 2346
We present the first high spatial resolution mid-IR and far-IR images of the planetary nebula NGC 2346 using the Multiband Imaging Photometer for Spitzer (MIPS) on board the Spitzer Space Telescope. The morphology at 24 ЮМm is strikingly similar to that seen in the optical image, with an additional unresolved hot dust component at the center. ... ADS Citation Query . citations = 31 . citations vs. year [year,citations] . ...
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Ссылки http://www.stsci.edu/~kgordon/papers/2004ApJS..154..302S.html -- 4.2 Кб -- 21.01.2016
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8. Auroral Images
... In principle, two observers on the ground can tell, by comparing the position of the same auroral arc against the background stars. ... The display stretches across Canada; just below it, in the middle of the picture, are the lights of Chicago, next to Lake Michigan. ... The Canadian scientific satellite Isis-2 (1971) carried an auroral imaging camera and discovered the diffuse aurora, a broad ribbon around the auroral oval, too spread-out to be noticed from the ground. ... Auroral Acceleration . ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/wimage.html -- 7.3 Кб -- 21.12.2007
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9. LSSS - Photogallery - Subatomic resolution on Cu(014)-O
Subatomic resolution on Cu(014)-O . 3nm x 3nm STM image of the Cu(014)-O 0.5ML surface measured with MnNi tip. ... This result has been discussed in Phys. Rev. Letters, 98, 206101 (2007) (A.N.Chaika, V.N.Semenov, S.S.Nazin, S.I.Bozhko, S. Murphy, K. Radican, I.V.Shvets, "Atomic Row Doubling in the STM Images of Cu(014)-O Obtained with MnNi Tips"). Image courtesy of A.Chaika. The image was measured in constant current mode using RT STM GPI-300. Copyright ISSP RAS, LSSS, 2006-2007 . ...
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Ссылки http://www.issp.ac.ru/lsss/gallery/22_eng.html -- 3.6 Кб -- 24.07.2007
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10. lbaops:lbadec2009:v255h [ATNF VLBI Wiki]
... You are here: start €Ё lbaops €Ё lbadec2009 €Ё v255h . ... VLBI Schedule . ... Observer's Wiki . ... lbaops:lbadec2009:v255h . v255h . ... ATNF recording . ... Setup v255h.5cm-icrf: . ... Channel 1 . IFP#1-LO 6300 - 6316 MHz USB RCP . ... IFP#1-HI 6316 - 6332 MHz USB RCP . ... Setup v255h.5cm: . ... Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v255/v255h . ... For Hobart the LOs should be set to 468 MHz (IFP#1) and 810 MHz (IFP#2) for the 4 x 16 MHz setup and 810 MHz for the 2 x 16 MHz setup. ...
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Ссылки http://www.atnf.csiro.au/vlbi/dokuwiki/doku.php/lbaops/lbadec2009/v255h -- 27.1 Кб -- 11.04.2016
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11. Ring Around the Galaxy
... The closer galaxy's gravity will act like a huge lens , pulling images of the background galaxy around both sides. ... The distorted galaxy is said to appear as an Einstein ring , named after Albert Einstein who accurately predicted many attributes of the gravitational lens effect -- although he also guessed that such an effect was unlikely to be seen in practice. ... NASA Official: Jay Norris. ... Abell 2218: A Galaxy Cluster Lens . Dark Matter Ring Modeled around Galaxy Cluster CL0024 17 . ...
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Ссылки http://www.astronet.ru/db/xware/msg/apod/1998-12-23 -- 14.5 Кб -- 15.08.2004
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12. High-Resolution Spectrum of the Ant Planetary Nebula around 12.8ѕ®m | ESO
... ESO, the European Southern Observatory . ... ESO's Governing Bodies . ... Travel and Contacts . Travel to ESO Headquarters . ... Travel to Guesthouse . ... Survey Telescopes . ... ESO 3.6-metre telescope . ... MPG/ESO 2.2-metre telescope . ... ESO 1-metre Schmidt telescope . ... Reproduction of a high-resolution spectrum of the Ne II line (ionised Neon) at 12.8135 microns of the Ant Planetary Nebula, also known as Mz-3. ... Ant Nebula , Mz3 , Spectrum . ... Milky Way : Nebula : Type : Planetary . ...
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Ссылки http://www.eso.org/public/images/eso0417h/ -- 90.2 Кб -- 10.04.2016
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13. Cosmic Microwave Background Anisotropy
The angular power spectrum of the anisotropy of the CMB contains information about the formation of the Universe and its current contents. ... The image above shows an all-sky map with only ell=2 power on the left, and another map with only ell=16 power on the right. ... The current status of microwave background anisotropy measurements in my compilation from the literature has 95 data points from 25 experiments. These are all plotted in the figure below: . ...
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Ссылки http://www.sao.ru/cats/~satr/cosmo/CMB-DT.html -- 5.6 Кб -- 16.10.2000
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14. Free Mars Wallpapers
Armagh Planetarium Mars HiRISE Wallpapers . High Resolution Imaging Science Experiment (HiRISE) is flying onboard the Mars Reconnaissance Orbiter (MRO) mission. Mouse over the thumbnails for a larger view of the image. ... When the image has entirely loaded, right click on it and choose option 'Set as background' or 'Set as wallpaper' depending of your Windows version. ... Historical Images . ... Mars Wallpapers . 1024 x 768 px . 1600 x 1200 px . Image Info . ... 1600 x 1200 pix . ...
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Ссылки http://www.armaghplanet.com/html/gallery_MarsHiRise.html -- 45.6 Кб -- 06.10.2011
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15. Background: motivation for developing this procedure
... Meta Index / Home Page / Description / Soft flare rejection for . The EPIC-pn fast timing mode was designed so that a time resolution of 0.029 milliseconds can be achieved. ... Below this energy the data is affected by so-called soft flares which are caused by stack overflows generated by high energy particles. These so-called soft flares have sharp rise (from 0 counts/sec to several thousand counts/sec in 0.10-0.15 sec) then decaying back 0 counts/sec slightly slower in about 0.3-0.4 sec). ...
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Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/epreject/node9.html -- 5.2 Кб -- 15.11.2007
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16. A New Entropy Measure Based on Multiple Resolution and Noise Modeling
... Previous: Background Fluctuation Analysis from the Multiscale Entropy . ... A new measure of information is defined which is based on noise modeling and incorporates resolution scale. Properties of this measure are discussed. ... Additionally it allows for image noise modeling, and subsequent noise removal. ... Hence information- and entropy-based processing technologies will be necessary for the effective design and implementation of large, future generation, image databases. ...
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Ссылки http://www.adass.org/adass/proceedings/adass98/murtaghfd/ -- 17.8 Кб -- 16.07.1999
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17. Photo album: Japan: Kyoto and Nara, August 1997
... Day-by-day lines contain complete set and intended for those who have been there (I mean, in Kyoto :) . ... Large format is mainly for 1600x1200 screens and fast link (pictures are up to 150K in size). Normal is for typical 1024x768 screen (i.e. 15" monitors). ... Photos look incredible on it. ... Large . ... Normal . ... Thumbnails . ... Contents with thumbnails: Large | ... Nara, one of the historical cities of Japan . ... August 17, Sunday. ... Nara. ... return to photo album contents | ...
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Ссылки http://crydee.sai.msu.ru/photo/japan/ -- 9.3 Кб -- 10.05.1998
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18. *imcalc* - Obtain a background subtracted image for ROSAT PSPC Data
... Use the ROSAT broad band background which is a array file at 1/30 the *.qp file resolution, and contains data from PI bins 7-240. input files: xdata$rp110590.qp; xdata$rp110590_bk1.imh . ... xr> ximages xi> imcalc input file ('-' for STDIN) or imcalc commands: - # Interactive mode IMC) IMC) rp90_a.imh = xdata$rp110590.qp[bl=30,pi=7:240] - xdata$rp110590_bkl.imh # Select same size and channels as the background map # and subtract the background IMC) quit # To exit the interactive mode and imcalc . ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node117.html -- 4.5 Кб -- 01.10.2012
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19. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE6C0FE6C-F335-43EC-A971-3208E1DEDB82%7D
Danielson and Kalocsa craters in the Arabia Terra region of Mars were imaged during orbit June 19, 2011, by ESAтАЩs Mars Express High-Resolution Stereo Camera (HRSC). Centered at around 7€ђN and 353€ђE, this anaglyph 3D image has a ground resolution of about 26m per pixel. Data from HRSCтАЩs nadir channel and one stereo channel are combined to produce this 3D image that can be viewed using stereoscopic glasses with redтАУgreen or redтАУblue filters. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE6C0FE6C-F335-43EC-A971-3208E1DEDB82%7D -- 4.0 Кб -- 10.04.2016
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- http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB04A97D7-1CEC-400A-9F2E-DE543AE4674D%7D
- http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B4B5EEC0A-8305-4178-813D-92569181349D%7D
- http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BCA7AD535-FACB-49B1-88E1-FD6ECE9348AA%7D
20. NICMOS and the VLT: A New Era of High Resolution Near Infrared Imaging and
... ST-ECF, ESO, STScI and the NICMOS IDT organized a workshop on near infrared imaging from space and ground was held in Pula on May 26-27, 1998. ... The meeting was held in May 1998, about one year after science observations started with NICMOS, and about half a year before the Infrared Spectrometer and Array Camera (ISAAC) starts to operate on the VLT. Currently, it is expected that NICMOS will operate until the end of 1998. ...
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Ссылки http://www.stecf.org/conferences/meeting/ -- 4.8 Кб -- 13.06.2006
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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