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• WDC-C2 Kyoto, final Dst monthly plot and table

... 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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• cat4COS
• Index of /stp/data/cosmic.ray/Neutron_Monitors(monthly_values)

Armagh Observatory reports that October was wetter, duller and warmer than average. ... The mean monthly temperature was 11.8 degrees Celsius (53.2 degrees Fahrenheit), considerably higher than the average value of 10.2 degrees C. The maximum temperature of the month, 18.7 degrees C (65.7 degrees F), occurred on the 27th. ... These data refer to observations at Armagh Observatory, which has been recording the weather at Armagh since 1795. ... Last Revised: 2005 November 7th . ...

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• Armagh Observatory
• Armagh Observatory Weather June 2005

THE RELATIVE MONTHLY MEAN SUNSPOT NUMBER ON OCTOBER 2015 HAS MADE Woct. = 37.1 (old), 61.7 (new) THAT GIVES FOR 75 MONTHS (2015, APRIL) DEVELOPMENT CURRENT 24 CYCLE OF SOLAR ACTIVITY THE SMOOTHED MONTHLY MEAN SUNSPOT NUMBER W*apr. = 50.0 - old; 61.7 - new; W*march = 49.3 - old; 82.7 - new; - On July 1, 2015 Centre in Brussels moved to a new system of cal- culation the relative number of sunspots and practically all of the values were replaced throughout the numbered series of Wolf numbers (see link). ...

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• http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20151005.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20150504.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2014/obzor20141103.en.txt

daily,monthly plots . yearly plots The temperature on the platform is measured every two minutes by the laser ranging system. ... no data . ... dec00 .ps .pdf At the end of each year, summary plots are made for the temperature. ... A histogram of the yearly temperatures is plotted for each year. ... The daily median temperature varies by 6 degrees over the year. 98% of the time the temperature is between 65 and 85 F. The daily (Max - Min) temperature is relatively constant throughout the year. ...

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• wst idl routines
• gps rfi aug08
• system Performance

metric_cycle_monthly (version 15.05.21) . ... metric_cycle_monthly.py . ... Excel) and plots (cycle completion and gto) . USAGE: do metric_cycle_monthly [-verbose] . ... o Python 2.5 app 07/30/09 . o Allow instr in GTO plot, more colors app 08/31/10 . ... Modules . ... line plot routine . xy - list of (X,Y) axis variable pairs . yc - color specifier; None or a list of color values . ... ylw - line width specifier; None or a list of width values . ... Produce Active cycle history plot . ...

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• Time Dependence of UV Response
• Python: module metric_calib_monthly
• Short-term Time Dependence of UV Response

Astronotes Armagh Planetarium's Stellar Blog! ... Monthly Sky Notes . ... Posted on November 6, 2013 | No Comments Incredibly as we near the close of yet another year, a year that has already been rich in celestial sights for the sky-watcher, perhaps the climax of all-things-cosmic from the [ ] . Continue Reading.. Posted on October 4, 2013 | ... No Comments The skies have been quite exciting for just the first two months of 2013, with a near earth asteroid and a crazy Russian Meteorite. ...

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• Monthly Sky Notes | Astronotes
• Monthly Sky Notes | Astronotes - Part 2
• Monthly Sky Notes | Astronotes - Part 5

... New engineering model of the feed system is under development now. ... Appendix (The list of used acronyms) ASC Cold Plate DC Astro Space Center of Lebedev Physical Instutute cooled LNAs and antenna feed hermetic device container (part of payload); it contains Formatter, Rb oscillators, synthesizer, control unit and is placed under dish DM Device Module = DC + H-maser EGSE Electronic Ground Support Equipment Electronic Complex ­ all SRT electronics EM Engineering Model FC Focal ...

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• http://www.asc.rssi.ru/RadioAstron/meetings/telecon/nov16_2011.pdf
• RadioAstron Monthly Notices
• RadioAstron main page, english version

... Liftoff With the Space Shuttle . ... M31: The Andromeda Galaxy . ... The diffuse light from Andromeda is caused by the hundreds of billions of stars that compose it. ... Almost lost in this cosmic jumble of stars, gas and dust is a faint but definite blue arc -- a stream of young stars whose formation was probably triggered as a small dwarf galaxy was torn apart approaching the giant elliptical galaxy Centaurus A. Oklo: Ancient African Nuclear Reactors . ... IC 5146: The Cocoon Nebula . ... October ...

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... There are TPM log files for every night of the dark run except for the nights of 08 October and 14 October 1999. ... The figures below are plots of the MIG data with the y-axis in TPM MIG units (real MIG units*1000) and the x-axis in seconds since midnight. ... Figure: Plot of MIG values vs elapsed time from midnight 10 October 1999. ... Figure: Plot of MIG values vs elapsed time from midnight 08 October 1999.The plot starts recording data from 21:26:52.0 on that day. ... 11/24/1999 ...

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• Scale adjustment
• Astrophysical Research Consortium - Apache Point Observatory
• Focus sweep data

Next: Column label: MOONE Up: MOUNTING= 'FORK' Previous: Column label: DEC . The values in this column are the corresponding hour angles of the eastern ``observation'' limits, in decimal degrees. ... Most telescopes read out hours and minutes instead; these should be acceptable inputs to the table-making program, which should do the conversion. ... In some cases, hour angles east of the meridian are read as negative values; in other cases, values will lie between and ( and ). ...

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• Values, Variables, and Literals
• Numerical Values of Image Pixels
• HMS(3)

Next: NCHAN Up: Details of SCHED Parameters Previous: MINPAUSE Contents . MONTH is the month of the stop time of the scan. The day of year of the first day of the MONTH , minus 1, is added to the value for SCHED parameter DAY to get the day of year of the project. Thus MONTH can be specified and DAY given as the day of the month, or MONTH can be left at the default of 1 and DAY can be given as the Day of Year (DOY). ... Argument: Integer. ... Usage: Defaults to previous scan. ...

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• casacore: casa::Near< L, R > Struct Template Reference
• blflag
• Package: ex

... October 14, 1997 . Venus On The Horizon . Credit: STS 30 Crew , NASA . Explanation: The month of October features a sky full of planets, including Venus as the brilliant evening star. Besides the sun and moon, Venus is the brightest object visible in Earth's sky. ... Because it is closer to the sun than Earth, Venus never strays far from the sun in its apparent position and is seen during the year as either a bright morning or evening star . ... About APOD > . ... NASA Technical Rep.: ...

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• APOD: 2003 October 15 - Space Rock SQ222 Noticed After Pass
• APOD: 2008 February 5 - Three Month Composite of Comet Holmes
• APOD: 2012 October 17 - Aurora Over White Dome Geyser

... Files with sunspot magnetic fields data ============================================== Column Format Description ______________________________________________ 1-2 I2 Day of month 3-4 I2 Month (numerical) 5-8 I4 Year 9 A1 Blank 10-13 I4 UT in hhmm 14 A1 Blank 15-19 A5 Sc - atmospheric flutter in arc sec 20 A1 Blank 21-25 A5 S - quality of the Sun image 26-27 A2 Blank 28-31 A4 Number of sunspots (numbering from unit every day ) 32 A1 ...

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• Datafile structure
• Pulkovo NEO Page: Estimation of Accuracy of the Observations

... Meta Index / Home Page / General-purpose array-processing utilities / Array or vector scalar . ... If is outside the range 0 to 1, the smallest or largest element , whichever is appropriate, is returned. interface valueAtHistoFraction real ( single ) function valueAtHistoFractionVector(vector, binFraction , maskVector) real ( single ), intent (in) :: vector(:), binFraction logical(bool), intent (in), optional :: maskVector(:) end function valueAtHistoFractionVector real ( single ) ...

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• Estimation of the optimal weights
• Null Values

http://hea-www.harvard.edu/AstroStat/slog/2007/p-values-what-they-are-and-how-to-use-them/ Weaving together Astronomy+Statistics+Computer Science+Engineering+Intrumentation, far beyond the growing borders Fri, 01 Jun 2012 18:47:52 +0000 hourly 1 http://wordpress.org/?v=3.4

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• Mapping Pixel Values to Screen Intensity
• *ftpplot* - Distribution of FFT coefficient values
• The AstroStat Slog Blog Archive P Values: What They Are and How to Use Them

Lectures . ... Home Lectures Lecture Series 2010-2011 Lecture Series 2010-2011 ? The History of the Universe in One Hour? by Max Tegmark . ... Lecture Series 2010-2011 . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... Amateur Astronomers Medal . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

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• This Month?s Sky ? 2015 ? Amateur Astronomers Association of New York
• This Month?s Sky ? 2014 ? Amateur Astronomers Association of New York
• Lecture Series 2015-2016 ? Amateur Astronomers Association of New York

The magnetic mapping is fulfilled by the magnetic field line tracing from the satellite position up to the Ionosphere (stop trace at the altitude 110 km). ... As a rule the Tsyganenko [1987] external magnetic field model and IOPT = 3 (Kp = 2) are used. ... The output file includes the following information: . ... For example the file with name aa9610d1.geo contains the information corresponding to the aposteriory magnetic mapping for INTERBALL Auroral Probe for the first decade of October 1996. ...

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• STDA files
• INTERBALL IB_AUR October 1996 magnetic conjugations
• INTERBALL IB_AUR October 1998 magnetic conjugations

... Appropriate values of DIT the integration time (DIT secs) for each individual integration, are lmited by various considerations. N.B. Ndit individual Integration s each of DIT secs are coadded to form a single Exposure of time Ndit*DIT]. The recommended minimum DIT is one sec (the minimum possible exposure time) or the value at which the noise becomes sky (rather than detector) limited. ... The recommended maximum DIT is such as to keep the detector wells less than half full. ... 40 sec . ...

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• SADT - Survey Area Definition Tool - for VISTA
• VISTA ETC - Exposure Time Calculator
• Observing with VISTA

minmax - Find extreme values in data tables minmax [ files ] [ -C ] [ -H [ nrec ] ] [ -I dx [/ dy ] ] [ -M [ flag ] ] [ -: ] [ -bi [ s ][ n ] ] minmax reads its standard input [or from files] and finds the extreme values in each of the columns. It recognizes NaNs and will print warnings if the number of columns vary from record to record. ... C Report the min/max values per column in separate columns [Default uses <min/max> format] -H Input file(s) has Header record(s). ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/nearneighbor.html
• http://xray.sai.msu.ru/~ivan/gmt/man/grdmask.html
• Test of the Initial Mass-Ratio Distribution