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1. A collection of images
... The TRACE images may be used without restrictions in publications of any kind. ... These two images, taken on 18 November 2000 at 15:54UT and 16:11UT, respectively, show such an event: the red circle in the image to the left shows a region where many loops are cooling, with bright loop tops (the intensity scales with the square root of the image to reduce the dynamic range). ... See also a collection of images related to the Sun, other cool stars, and solar-terrestrial effects . ... Images | ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/sun/T171_20001101_101547.html -- 13.0 Кб -- 28.12.2000
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2. Solar Moss
... 27.12.1999 . ... Credit: TRACE Project , NASA Explanation: Discovered in recent close-up pictures of the Sun from NASA's Transition Region And Coronal Explorer (TRACE) spacecraft, this spongy-looking stuff has a temperature of 2 million degrees Fahrenheit ... and has been dubbed "Solar Moss". ... It shows the solar moss associated with hot magnetic plasma loops arching above one of the Sun's active regions . ... December 1999 . ... Publications with keywords: Sun - active region - solar moss . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/apod/1999-12-27 -- 14.2 Кб -- 10.11.2006
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3. TESIS - Telescopes for EUV Spectral Imaging of the Sun
... The TESIS is a set of solar imaging instruments developed by the Lebedev Physical Institute of the Russian Academy of Science, and launched aboard the Russian spacecraft CORONAS-PHOTON on January 30, 2009. The main goal of the TESIS is to provide complex observations of solar active phenomena from the transition region to the inner and outer solar corona with high spatial, spectral and temporal resolution in the EUV and Soft X-ray spectral bands. ... Solar activity hits a new low . ...
[ Сохраненная копия ]  Ссылки http://www.tesis.lebedev.ru/en/ -- 19.2 Кб -- 09.04.2016
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4. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Upflows at the edges of active regions - called AR outflows , are studied using multi-instrument observations. ... The evolution of the photospheric magnetic field associated with the footpoints of the upflow region and the plasma properties of active region upflows are investigated aiming at providing such information for benchmarking data-driven modelling of this solar feature that is presented in Galsgaard et al. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2015/679.html -- 7.9 Кб -- 14.10.2015
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5. INTERBALL IB_TAIL October 2000 magnetic conjugations
... The IB_TAIL magnetic conjugations with the others Spacecraft . ... ASCII file description | Plot description | ... ASCII file | real time plot . ... The IB_TAIL magnetic conjugations with the groundbased magnetic observatories . ... The IB_TAIL magnetic mapping polar diagram, and ASCII files for each decade of month: . ... ASCII files description | DEC 1 (ASCII file, size more then 350Kb!) ... Back to the IB_TAIL Home page. Updated 29 August, 2000 . ... INTERBALL mission  ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/tail/200010/mt0010mc.htm -- 6.7 Кб -- 29.08.2000
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/vprokhor/tail/200010/mt0010mc.htm -- 6.7 Кб -- 29.08.2000
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6. The Interstellar Medium
The interstellar medium is the material that lies between the stars in a galaxy . This material can exist in several phases with a wide range in temperature (from tens of degrees to tens of millions of degrees Kelvin). In the coldest regions the material consists of molecular gas and dust; in the hottest regions the material is almost completely ionized. The Role of the Interstellar Magnetic Field A. Goodman . The Diffuse ISM High-Latitude Clouds A. Goodman . ... 617) 495-7062 . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~juda/ism/ism.html -- 3.7 Кб -- 01.10.2012
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7. APOD: January 6, 1997 - Blue Sun Glaring
... January 6, 1997 . Blue Sun Glaring . Credit: EIT , SOHO , ESA , NASA . ... In this false-color picture , light blue regions are extremely hot - over 1 million degrees , while dark blue regions are slightly cooler. ... This picture was taken in ultraviolet (extremely blue) light by the Extreme-ultraviolet Imaging Telescope (EIT) on board the Solar and Heliospheric Observatory (SOHO) spacecraft, which is orbiting the Sun just ahead of the Earth , at the L1 point . ... About APOD > . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap970106.html -- 4.7 Кб -- 02.10.2012
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8. Polarizer Quad Filter
Optical Filters . The polarizer quads were also designed to map onto a four-faceted WFC configuration and, consequently, also require a partial filter rotation of -33 degrees to move the filter quadrant 1 (nominal polarization angle 135 degrees ) into WFCs 2 and 3, with some vignetting of both camera fields. Several additional partial rotations have been added to allow observations with different polarization angles on the same CCD. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/wfpc2/W2_27.html -- 4.2 Кб -- 24.07.1996
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9. water ice on mercury
... NASA SPACECRAFT FINDS NEW EVIDENCE FOR WATER ICE ON MERCURY . ... The new data indicate the water ice in Mercury's polar regions, if spread over an area the size of Washington, D.C., would be more than 2 miles thick," said David Lawrence, a MESSENGER participating scientist at the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, Md., and lead author of one of three papers describing the findings. ... Water ice concentrations are derived from the hydrogen measurements. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/science/water_ice_mercury.html -- 8.5 Кб -- 03.12.2012
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10. Radio survey for new compact HII regions
... A total of 462 were detected, about half of these for the first time. ... Ojects not Detected ----------------------------------------- l b BRMS mK Notes ----------------------------------------- 6.490 + 0.084 5.1 W28 SNR 6.648 + 0.084 4.2 W28 SNR 8.989 +35.502 3.5 S33 B 11.531 +36.350 3.1 S36 A 13.456 + 0.156 3.5 SNR 16.732 + 0.079 3.5 SNR 19.961 - 0.175 3.5 SNR 21.347 - 0.628 3.8 Extragalactic 25.253 - 0.150 5.7 Extragalactic 25.520 0.215 5.2 28.600 - 0.126 4.0 SNR+HII+? ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/HII_Lockman.html -- 3.5 Кб -- 18.03.2015
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