Correlated flashes of masers H2O . ... In 1981 - 1982 years it was revealed several Flashes of maser radiation of H2O radioline at wavelength 1.35 cm in the radio-sourse W49, developing practically synchronously at several radial velocities. It's known that components of the maser radiation of H2O radioline profile with different radial velocities arise in separate spatially diverse areas of a starformation. ...

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... It is found that the correlation coefficients between these two parameters calculated separately inside and outside the sunspot formation zone ?30 have cyclic variation and occur in anti-phase. This suggests different mechanisms of formation of the corona in the fields of small, medium, and large scales. ... The relationship between the coronal green line brightness (CGLB) and the magnetic field strength (MFS) has been investigated by constructing the corresponding synoptic maps for the 1977-2001. ...

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• http://www.izmiran.rssi.ru/~eivanov/papers/9.pdf
• http://www.izmiran.rssi.ru/~eivanov/papers/75138986.pdf
• IZMIRAN: Laboratory for Physics and modeling of the ionosphere - publications -

... The file names' construction . The flight (m) stage's file set . ... the orbital data used for the flight operation monthly (m) long-term planning, . ... The orbital calculations are based on the initial orbital data determined by KIAM RAN using the orbital radio- measurement treatment. The determined initial orbital data are presented as a state vector (satellite position and velocity) in the J2000 reference. ... Accept the file with extension '.bgr', where the Moscow time (MT=UT+3h) is used. ...

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• The magnetic conjugations between the INTERBALL (IB_TAIL) and the SUPER-DARN
• The magnetic conjugations between the INTERBALL (IB_AUR) and the SUPER-DARN
• The magnetic conjugations between EISCAT and INTERBALL AURORAL PROBE (IB_AUR)

spaceweb@oulu.fi - last update: 13 September 1998, 1130 UT (RR) . Ground based magnetometer measurements are used to derive several indices that describe magnetic activity in the Earth 's environment. aa , AE , Ak(Hel) , Kp , Dst , PC , MT . ... AE index is an auroral electrojet index obtained from a number (usually greater than 10) of stations distributed in local time in the latitude region that is typical of the northern hemisphere auroral zone (Davis and Sugiura, 1966). ...

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• Isotropic boundary (Oulu)
• A Glossary of space weather terms
• Format Documentation of *.wdc Files

Next: The Scenario Machine: Operational Up: Evolution of Magnetic Rotators Previous: Ejector-propeller hysteresis . ... The length of this segment is determined by the eccentricity. ... In this case no hysteresis occurs and transitions E -- P and the reverse take place in symmetrical points of the orbit. ... Here EP means a mixed state of the rotator at which it is in the ejector state during one part of the orbit, and in the propeller state during the rest of the orbital cycle. ...

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• Initial Distributions of Binary Parameters
• Initial parameters of compact stars

... 1997: . For the most representative sample of 277 most nearby galaxies, their masses, separations and tidal indexes were determined based on the BTA observations. ... The most detailed light curve of optical star-like source (corresponding to the gamma-burst of May 8, 1997) was obtained from the BTA observations simultaneously in 4 photometric bands. ... An effect of an abrupt rate slowdown is noticeable in the infrared (~8000A) 36 days after the gamma-ray burst. ... Archive . ...

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• Galaxy sector, archive 2009
• Detection of polarized radiation sources with unusual spectral characteristics
• Solar activity

FGS Instrument Handbook for Cycle 24 . ... Fine Guidance Sensor Instrument Handbook for Cycle 24 > Appendix B: FGS1r PerformanceSummary > B.2 Angular Resolution Test . ... At the time of the test, the predicted angular separation of the components was 0.085" (Franz and Wasserman, private communication). ... By rolling the HST in 6 increments, the projected separation along the X axis varied from the predicted angular resolution limit of FGS1r (~6 mas) to the resolution limit of FGS3 (~20 mas). ...

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• Projected SAA-Free Times
• Python: module reduce_obad_pcs_separation
• Geometric Distortion

An Ancient Universe: How Astronomers Know the Vast Scale of Cosmic Time . ... Astronomers can also determine the speed a galaxy is moving by breaking up its light into its component colors, rainbow-fashion. ... This pattern is now called "the expanding universe", since the entire universe of galaxies seems to be moving away. ... The Ancient Universe - The Age of the Expanding Universe - The Age of the Oldest Stars - The Age of Light From Distant Galaxies - The Age of the Chemical Elements | ...

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• ASP: Family ASTRO: Night Sky Adventure
• ASP: Black Holes
• ASP: The Return of Halley's Comet

reconstruction with Fast Simulation M. Iwasaki University of Oregon At the Sitges meting: tt 6jets 4jets analysis Ї Charged/Neutral cluster separation with Track- cluster matching Ї Reconstruction performance in Energy flow analysis Ї B-tag effect After the meeting: Ї In FastMC, set the cluster position resolution determined by FullMC Ї Study Cluster width with FullMC Ї ...

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• http://zebu.uoregon.edu/51peg.html
• Inflationary Epoch

The image on the left shows the 7 horns with the X axis along the azimuth arm. ... The beams on the sky are elliptical with the major axis along the azimuth arm. ... If we rotate the feed array by + phi degrees then the projection of each horn center on the X axis is: Px1= S*sin(phi) Px2=S*cos(phi+30) Px3=S*cos(phi-30) . The separation between the projected horn centers are: Distance(Px1-Px0)=S*sin(phi) Distance(Px2-Px1)=S*(cos(30+phi)-sin(phi)=S*(cos(30)cos(phi)-sin(30)sin(phi)-sin(phi)) . ...

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• http://www.naic.edu/~tghosh/FOT/FEB07/arecibo_proposal_sc_justi_2.pdf
• http://www.naic.edu/~gibson/m42/m42_HST.txt
• I-GALFA Reveals Dynamic Events in Our Galaxy

ISSN 0016 7932, Geomagnetism and Aeronomy, 2012, Vol. ... Special Points in 11 Year Variations in the Latitudinal Characteristics of Sunspot Activity E. V. Miletsky and Yu. ... 65, St. Petersburg, 196140 Russia e mail: eugenm@gao.spb.ru Received March 5, 2012 Abstract--It has been indicated that special moments (turning points), when certain characteristics of the latitudinal (equatorward) drift of the sunspot drift zone suddenly change, exist in each 11 year solar cycle. ... Vol. ...

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• http://www.gao.spb.ru/personal/miletsky/papers/mil+iv-2014_gia.pdf
• Extended time series of Solar Activity Indices
• Страница Е.В.Милецкого / Page of Eugen Miletsky

... Russian Foundation for Basic Research , Project number 98-02-17366 . ... A number of experiments proposes the d -type of the wave function, having two directions with positive and two (in orthogonal direction) - with negative sign of the order parameter. ... The effect of the wave function phase is most efficiently revealed in the experiments with Josephson structures, that are used for determination of the dependences on the pulse direction. ... The project goals are: . ...

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• Lab234 - Development, study and optimization of the superconducting phase
• Separation of chaotic signals - Reports to the Russian Academy of Sciences
• Separation of chaotic signals - COC-2000

Cosmic ray intensities (left) compared with predictions (right) from IBEX. The similarity between these observations and predictions as evidenced by the similar color regions supports the local galactic magnetic field direction determined from IBEX observations made from particles at vastly lower energies than the cosmic ray observations shown here. The blue area represents regions of lower fluxes of cosmic rays. ...

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• WMAP reveals infant universe | Astronomy.com
• NASA spacecraft reveals new observations of interstellar matter | Astronomy.com
• Frantic activity revealed in dusty stellar factories | Astronomy.com

... The calculator on this page allows you to calculate the angular separation of two sources in the sky using the corresponding equation derived on the Spherical geometry page. JavaScript must be enabled for the calculator to work. ... Source 1 / l : / b : . ... Note: the allowed format of right ascension / longitude is hh:mm:ss.s , hh mm ss.s , or d.d , while the format of declination / latitude is dd:mm:ss.s , dd mm ss.s , or d.d . ... 2016 Tobias Westmeier Contact | ...

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• Plans and Activities
• Planetary_nebula
• Determining Gains and Polarimetric Properties - GPCAL

... ESO, the European Southern Observatory . ... Survey Telescopes . ... Galaxies . ... ESO 3.6-metre telescope . ... MPG/ESO 2.2-metre telescope . ... Thanks to the Very Large Telescope's acute and powerful near-infrared eye, astronomers have uncovered a host of new young, massive and dusty stellar nurseries in nearby galaxy NGC 253. ... NACO revealed features in the galaxy that were only 11 light-years across. ... NGC 253 is known as a starburst galaxy, after its very intense star formation activity. ...

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• Infrared/visible crossfade of the Monoceros R2 star-forming region | ESO
• Frantic activity revealed in dusty stellar factories | ESO Nederland
• POLIMPLOT (V2.00) --- November00 --- POLIMPLOT (V2.00)

... true false . A boolean switch determining whether the list of to be considered HK parameters shall be explicitly specified with parameter parameters . ... blank separated list of HK parameter names . ... If set to true overrideparameters must contain a list of HK parameter names and overrideparametervalues a corresponding list of validity ranges for those parameters (see below). overrideparameters . ... If withoverrideparameters is set to true the list must contain valid HK parameter names. ...

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... October 21, 1997 This Hubble Space Telescope image provides a detailed look at a brilliant "fireworks show" at the center of a collision between two galaxies. ... The respective cores of the twin galaxies are the orange blobs, left and right of image center, crisscrossed by filaments of dark dust. A wide band of chaotic dust, called the overlap region, stretches between the cores of the two galaxies. ...

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• IBIS - Installation
• High-resolution Herschel spectroscopy reveals the proto-planetary disk around
• Arcetri Solar Physics Group: Solar Activity

... Most people that are interested in supernovae use whatever telescopes they can get access to, but researchers at certain colleges and universities are able to access specialized telescopes like NASA?s Chandra X-ray Observatory . It?s a telescope that orbits the Earth and that has a specialized purpose of being able to observe X-ray emissions from supernovae, clustered galaxies and the materials around black holes. ... super@supernovae.net . ... Copyright x000A9; 2016 Supernovae.net ...

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• APOD: 2000 May 9 - The Race to Reveal Our Universe
• APOD: April 23, 1998 - Three Dusty Stars
• APOD: May 4, 1999 - Magnetic Mars

If necessary, the observations and corresponding O ? C values belonging to some observatory can be separated from the other data. Besides, O ? C satisfying some conditions imposed on their value can be separated. ... To separate O ? C by value, mark O ? C check box and enter positive numbers limiting absolute values of O ? C from above or from bottom or both and click on Run . ... The restrictions imposed on observatory code and on O ? C values are indicated in status bar. ...

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• Values of asteroid masses

... Minute Values of Geomagnetic Field Components . ... AA 1868 - Present (3 hourly and daily) (monthly) (yearly) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) KP_AP 1932 - Present (3 hourly and daily) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) AE_HV 1957-75, 78-88 (hourly) AE_MIN 1978-881-6;198903;1990-94 (minute) DST 1957 - Present (hourly) PC 1975 - Present (15-minute) AMANAS 1959 - Present (3 hourly and daily) KMKNKS 1983 - Present (3 hourly) . ...

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• cat1aa
• WDC for STP