Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 13 - 19.05.2013 , Forecast on 20 - 27.05.2013, Carrington Rotations 2136, 2137 (17,78.04; 15,02.05.2013) SUNSPOT-FORMING ACTIVITY OF THE SUN CHANGED FROM THE AVERAGE TO HIGH AND BACK TO THE AVERAGE LEVELS. ... NEXT WEEK THE LEVEL OF SUNSPOT ACTIVITY IS EXPECTED TO BE THE AVERAGE AND THE LOW. THE CALCULATED MOST LIKELY WEEKLY AVERAGE VALUE OF SUN- SPOT NUMBER IN THE INTERNATIONAL SYSTEM FOR THE NEXT WEEK IS EXPECTED W = 060+20/-20. ...

... FIELD | ... public interface Blitter . ImageJ bit blitting classes must implement this interface. ... static int . ... dst=dst+src . ... Field Detail static final int COPY . ... Constant Field Values . static final int COPY_INVERTED . ... static final int COPY_TRANSPARENT . ... static final int ADD . ... static final int SUBTRACT . ... static final int MULTIPLY . ... static final int DIVIDE . ... static final int AVERAGE . ... static final int DIFFERENCE . ... static final int AND . ...

... angle (degrees) . inches . ... average . ... range . ... specification . ... tolerance . ... 2ry baffle tip thickness . ... 2ry baffle tip overhang . ...

program tripos1 implicit none real :: p1, p2, p3, maths real :: av1, av2 ! read in the marks read(*,*) p1, p2, p3, maths ! work out the two averages av1 = p1 + p2 + p3 av2 = av1 + maths av1 = av1 / 3.0 ; av2 = av2 / 4.0 ! use an if statement if (av2 > av1) then write(*,*) 'Final average = ',av2 else write(*,*) 'Final average = ',av1 end if end program tripos1

... Up: Algorithms . ... Non-linear and non-parametric algorithms for data averaging, smoothing and clipping in the RATAN-600 flexible astronomical data processing system are proposed. Algorithms are based on robust methods and non-linear filters using an iterative approach to smoothing and clipping. ... The history of algorithms, based on the robust methods and non-linear filters using an iterative approach to smoothing and clipping, began twelve years ago in the data reduction at the RATAN-600. ...

... THE SIMPLEST MODEL. ... 13, Moscow 119992, Russia E-mail: san@sai.msu.ru Abstract: The analysis of the simplest model shows that an asteroid ­ rubble pile evolves, depending on the parameter V2d (where V is the average velocity of fragments and d is the average distance between fragments), either as a conglomerate of "independent mutually gravitating clusters" (when V2d < fm, where f is the gravitational constant and m is the average mass of a fragment) or as a "receding cluster" (when V2d > fm). ...

Astronotes Armagh Planetarium's Stellar Blog! ... Space Flight . ... Earth Satellites . ... Leonid meteors seen from 13 km altitude aboard an aircraft during the 1999 Leonids Multi-Instrument Aircraft Campaign (Leonid-MAC). Comet Tempel-Tuttle provides the cometary debris for the Leonid meteor shower. ... Every 17-19 November Earth crosses Tempel-TuttleтАЩs orbit and the Leonids become visible. With clear, dark skies observers may see 10 to 15 Leonid meteors every hour on those mornings. ...

Radio pulsars strictly periodic signals 14.03.2016 B 10 G;E 10 V / cm 12 10 2 Individual pulses and average profile of pulsar 14.03.2016 3 Average profiles of pulsars 14.03.2016 average energy distribution of pulses by phase of period. ... 14.03.2016 5 2695 Giant pulses (GPs) of pulsar Intensity, a.u. Time, ms Pulses that exceed the average profile over 30 times were called giant pulses. ... 2005) 14.03.2016 8 Individual pulses energy distribution 1937+21. ...

Organisers: Michel Balazard (CNRS, Laboratoire Poncelet) , Michael Tsfasman (CNRS, Laboratoire Poncelet, Institute for Information Transmission Problems) , Alexey Zykin (Laboratoire Poncelet, State University Higher School of Economics) . ... General Information . ... Number theory semester web page . ... Our main result is a characterization of the Lebesgue points of $\Phi$. Poncelet Laboratory web page . ...

Next: Amplitude Distribution Previous: Gravitational Wave Background from . To get rid of the extragalactic GWB produced by binaries, one can use the above considerations to find the optimal detector halfwidth and frequency for observations. ... for the flat red end of the GWB, and . ... Equating to unity, one finds the critical detector halfwidth . ... In contrast, by observing the sky with a GW detector with a narrow enough halfwidth , one will not ``see'' the extragalactic GWB at frequencies . ...

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Things to Do in Boulder, CO.. ... The Flatirons serve as the backdrop for Boulder and provide many outdoor activities, from hiking and biking to rock climbing and kayaking. ... It has 100 miles if bike paths. ... Many of the local restaurants brew their own beer, so you can sample the local brew without going on a brewery tour. ... 1) Pearl Street is in the heart of downtown Boulder and is a walking mall that features local restaurants and shops and many street performers. ...

... 20-24 Heliographic longitude 26-30 Latitude 32-36 Second heliographic longitude (999.9=no data) 38-42 Second latitude (999.9=no data) 44-47 Average group area, in millionths of solar hemisphere (9999=no data) 49-52 Average area of the largest spot (9999=no data) 54-56 Average number of spots in the group (999=no data) 58-59 Length of observation time of the group in days ...

RELATIVE SUNSPOT NUMBERS ------------------------------------------ MAXMIN dates since 1610 of sunspot cycle maxima and minima YEARLY yearly mean numbers beginning in 1700 YEARLY.PLT all yearly means in form suitable for plotting MONTHLY monthly means starting in January 1749 MONTHLY.PLT all monthly means in form suitable for plotting SMOOTHED 12-month running averages since July 1749 SMOOTHED.PLT smoothed averages in form suitable for plotting 1980- daily counts (1 table/year) from January 1980 to present

Magnetic Stars, 2011, pp. ... 2010). ... 463 Figure 2: Difference between individual and average spectra in Fig. 1 with phase (vertically, on the right) Figure 3: Almost in a year repeatability of spectral lines form (2009.07.05 and 2010.05.31) in an identical phase 464 CHOUNTONOV 4000 3000 Magnetic field, Bz(G) 2000 1000 0 -1000 -2000 2008/05/23 2010/05/31 -3000 0.0 0.2 0.4 0.6 0.8 1.0 phase Figure 4: Longitudinal magnetic field variations with phase (the sine curve, Rivinius et al., ...

... Campus . ... Samara State Aerospace University Campus Cafes, dining centres and buffets on campus . Building 3a Buffet . Moskovskoe Shosse, 34, Building 3a, 1st ?oor . ... Buffet in the crossing between buildings 3a and 3 . ... Dining Centre, Building 3 . ... Moskovskoe Shosse, 47, Building 5, 1st ?oor (in the classroom hallway) . ... Gaya St., 41, Building 14, 1st ?oor . ... 4 Buffet . Moskovskoye Sh., 32, 1st ?oor Open: 09.00-21.00 . ... Lukacheva St., 46, 1st ?oor Open: 09.00-21.00 . ...

Trudy GAISH, vol. LXV, 1996 . Abstracts . The global distribution of average (5 O x 5 O ) depths . of Mohorovicic discontinuity on the Earth . ... Such analysis allows detecting whether the sources of the largest anomalies reside within the Earth's core. This is possible if the limit depths of the sources exceed the depths of the core-mantle boundary. ... by Pasinok S.L. Influence of the Earth’s cover on the polar free oscillation of the Earth’s inner core is considered. ...

Astronomy Discussion Forums . ... Investigating Dr.Dick's Recent Revelations . ... Post Message | ... Now suppose a pattern just happened to appear after both shufflings (but in different places in the pack,say). ... So King,Jack also like stayed net-negative-shuffled to new location in pack for King,Jack. ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... Elias Loomis of Yale University compiled, in 1860, a map marking how many times in an average year were auroras observed in various locations (click here to see his map). ... However, it was only in 1954 that auroral electrons were actually observed, by detectors aboard a rocket launched into the aurora by Meredith, Gottlieb and Van Allen , of Van Allen's team at the University of Iowa. ... Exploration" home page (index) Glossary . ... Official GSFC Home Page .. NASA WWW Home Page . ...

Тема : Хвостатые гостьи V (информация для наблюдения комет) .. Показать сообщение отдельно . ... Хвостатые гостьи .. ... после того, как ISON приплыл мимо нас, земля находится на орбитальной траектории, которая пройдет через след частицы кометы (тот, который ISON оставил позади, когда это приближалось к солнцу и это случайно встретит или вокруг 12 января - 15, 2014 . ... лучшее время наблюдения 22:00 LDT (Northern hemisphere 45њ North) .. - радиант расположен вблизи Al'dzhabkhakh (30-Eta Leonis, ? ...