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1. http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20151019.en.txt
Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 12 - 18.10.2015, Forecast on 19 - 26.10.2015, Carrington Rotation 2169 (04,57.10.2015) SUNSPOT-FORMING ACTIVITY OF THE SUN REMAINED AT THE MIDDLE LEVEL. ... ACCORDING TO THE DATA FROM SOHO AND STEREO CORONOGRAPHS >24 CMEs HAVE BEEN OBSERVED. ... A-active geomagnetic condition. ... GEOMAGNETIC CONDITION ALREADY BEEN OCTOBER 12-13 IN A MINOR MAGNETIC STORM (G1, Ams= 29, dur.= 27 h.) ACCORDING TO THE CENTER IN BOULDER DATA. ...
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Ссылки http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20151019.en.txt -- 6.1 Кб -- 19.10.2015
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2. http://zebu.uoregon.edu/2004/es399/lec05.html
The Chi-Square Goodness of Fit Statistic . This statistic enables us to test whether observed frequencies are close to . those we would expect. ... Expected frequencies . ... For example, if we . have an honest die we would expect 1/6 of all cases to show any of . ... So, for example, if we roll a die 60 times we would expect : . ... If we actually roll a die 60 times we wouldn't expect each of the faces . ... times each face actually comes up is the observed frequency for that face. ...
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Ссылки http://zebu.uoregon.edu/2004/es399/lec05.html -- 12.5 Кб -- 19.01.2006
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3. TAC
Duty astronomers at the Compact Array are rostered from ATNF staff and students to provide support to observers at Narrabri for periods of one week at a time. The duty astronomers are required to assist observers prepare observing schedules, help set up the Compact Array at the start of an observing run, diagnose and attempt to solve problems that arise in the course of the observations and help observers with the initial analysis of their data. ... www.atnf.csiro.au/observers/tidbinbilla . ...
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Ссылки http://www.atnf.csiro.au/news/newsletter/jun05/TAC.htm -- 5.8 Кб -- 23.01.2013
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4. Leonids 2006
Trail encounter . ... Expected meteor rates . ... The Leonids are the debris of Comet 55P/Tempel-Tuttle. ... The Earth's passage right through the centre of trails is associated with the most spectacular meteor displays (studies show that, as well as how close to the centre of the trail you are, the strength of the display also depends on how far along a trail's length you are). ... The encounter with the 1932 trail will lead to enhanced meteor activity: a nice outburst, but below storm level. ...
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Ссылки http://star.arm.ac.uk/leonid/2006/info2006.html -- 8.6 Кб -- 21.11.2006
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5. Emission-line galaxies
... The new emission line galaxies are listed in Table 2 containing the following information: . column 1: The object's IAU-type name with the prefix HS. ... This was not corrected in the figure shown in Appendix A. HS1214+3801 : This is seemingly a supergiant H II -region at the very rim of the nearby edge-on disc galaxy (SA(s)cd) NGC 4244 (V hel = 224 kms -1 and B T =10.88). ... To check this option one needs a detailed map of the NGC 4244 velocity field including HS 1214+3801. ...
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Ссылки http://www.sao.ru/precise/Laboratory/Publications/2000/HSSIII/node10.html -- 12.9 Кб -- 08.02.2000
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6. Shifts Are As Would Be Expected. - an Astronomy Net Blackholes2 Forum Message
Blackholes2 Forum Message . ... Post . ... Shifts Are As Would Be Expected. ... Post Message | ... Red and blue shifts can be caused by velocities also. ... The expectd result would be a red or blue shift proportional to the aparent distance an object is from the observer. ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
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Ссылки http://www.astronomy.net/forums/blackholes2/messages/4964.shtml -- 13.6 Кб -- 09.04.2016
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7. http://www.naic.edu/vscience/schedule/2015Fall/DenevatagP2859.pdf
... Begin End IntervalInterval 01:35 04:05 09:30 12:05 16:00 16:50 17:00 22:10 Days Needed at This Interval 6 11 11 11 Time Constraints (Must Be Justified in the Prop osal Text) For J0251+26 (visible at LST 01:35 - 04:05): 6 x 0.75 h monthly sessions. For J1048+23 (visible at LST 09:30 - 12:05): 3 x 1 h daily sessions; 3 x 1 h weekly sessions starting 1 week after the last daily session; 5 x 1 h monthly sessions starting 1 month after the last weekly session. ...
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Ссылки http://www.naic.edu/vscience/schedule/2015Fall/DenevatagP2859.pdf -- 62.3 Кб -- 07.03.2015
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8. Bob Berman's strange universe: Expect a surprise | Astronomy.com
... Tonight's Sky . ... Observing . ... Bob Berman . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... Dave's Universe . ... Bob Berman's Strange Universe . Bob Berman's strange universe: Expect a surprise . ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...
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Ссылки http://www.astronomy.com/magazine/bob-berman/2005/07/bob-bermans-strange-universe-expect-a-surprise -- 63.3 Кб -- 10.04.2016
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9. Space weather forecast September 24, 2015
... Magnetic storms online . ... Geomagnetic activity forecast . ... September : 2015 . ... No magnetic storm is expected . From 25 September 2015 to 21 October 2015 the following magnetic storms and disturbances are expected: . October 14, 2015 geomagnetic disturbances . ... October 09, 2015 geomagnetic storm of level G1 (minor) . ... September 25, 2015 geomagnetic disturbances 25 September 2015 - 21 October 2015 . ... Probability of a magnetic storm . ... Probability of a strong magnetic storm . ...
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Ссылки http://www.tesis.lebedev.ru/en/forecast_activity.html?m=9&d=24&y=2015 -- 22.4 Кб -- 11.04.2016
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10. APOD: 2006 March 6 - Unexpected Comet Pojmanski Now Visible
... 2006 March 6 . Unexpected Comet Pojmanski Now Visible . ... Explanation: Have you ever seen a comet? ... Comet Pojmanski , officially designated C/2006 A1 and discovered only in January, now sports a turquoise tail several times longer than the full moon. Comet Pojmanski 's ion tail is due to gas particles expelled by the comet being pushed away from the Sun by the solar wind , the same wind that ionizes gas in the tail causing its blue tint. ... About APOD | ... NASA Official: Jay Norris. ...
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Ссылки http://www.sai.msu.su/apod/ap060306.html -- 4.9 Кб -- 02.10.2012
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11. Unexpected Comet Pojmanski Now Visible
Astronomy Picture of the Day . ... 6.03.2006 . ... Right now, however, a new comet has brightened unexpectedly and is visible as a faint streak to the unaided northern observer in the eastern morning sky just before sunrise. ... Comet Pojmanski , officially designated C/2006 A1 and discovered only in January, now sports a turquoise tail several times longer than the full moon. ... March 2006 . ... Publications with keywords: comet - comet tail . Publications with words: comet - comet tail . ...
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Ссылки http://www.astronet.ru/db/xware/msg/1212026 -- 14.9 Кб -- 06.03.2006
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12. http://www.stsci.edu/ops/swat/safing/12121/cos_removed_from_12121.txt
... These are the 12603 visits and one 12593. ... The following SUs have been DROPPED from cclist 121217D3 : SU Obsets PC CS 1260346:01 12603 :46:01 VICK WALBORN 124881S:01 12488:1S:01 MEYETT DEUSTUA 1259301:01 12593:01:01 TAYLOR ROMAN-DUVAL 124880S:01 12488:0S:01 MEYETT DEUSTUA 1260304:01 12603 :04:01 VICK WALBORN 1253309:01 12533:09:01 ROMAN MASSA 12533:A9:01 ROMAN MASSA 1260337:01 12603 :37:01 VICK ...
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Ссылки http://www.stsci.edu/ops/swat/safing/12121/cos_removed_from_12121.txt -- 3.7 Кб -- 02.05.2012
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13. ESO - I see unexpected boxy emission-like features in my REDL spectra - where
... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > I see unexpected boxy emission-like features in my REDL spectra - where do they come from? ... Observing with ESO Telescopes . ... ESO-MIDAS . ... ESO Data . ... The pipeline by default interpolates across the bad columns in the REDL CCD when it creates the master bias, but does not so when it processes the science data. This inconsistency can create boxy emission-like features as seen in the figure below. ...
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Ссылки http://www.eso.org/sci/data-processing/faq/i-see-boxy-emission-like-features-in-my-redl-spectra-where-do-they-come-from.html -- 23.1 Кб -- 10.04.2016
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14. Period Criteria
... Actual stars are expected to be more complicated than these simulations. ... The spot may be entirely visible most of the time (one would observe a prolonged flux minimum low), and then part of it may disappear over the horizon briefly and then return (slow rise and then fall back to constant level). ... With the set of observations taken here, I have information available from several comparison stars and color information. ... The period found must be consistent with the data from any given night....
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Ссылки http://hea-www.harvard.edu/~swolk/thesis/period/node9.html -- 7.2 Кб -- 02.10.2012
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15. ASP: Using Multicultural Dimensions to Teach Astronomy
... the time of observation . ... Observing the Changing Position of the Sun To Establish Cardinal Directions . ... Observations of the Sun's apparent movement across the sky and its pattern of rising and setting in the east and west horizon helped to establish the cardinal directions. ... The final stage of the Sun's return was marked by the observation that the Sun had reached its highest altitude when the full width of your mitted hand could fill the gap between the Sun and the horizon. ...
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Ссылки http://www.astrosociety.org/edu/publications/tnl/53/multicultural2.html -- 15.2 Кб -- 02.10.2012
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16. S.P. Korolev RSC Energia - International Space Station
... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... Project History . ISS Russian Segment . Steps of ISS Assembly . Spaceflights Chronology . Chronology of Extravehicular Activity . ISS 45/46 . ... Rocket Space Complexes . ... Launches Chronology . ... Automatic Space Systems . ... AT-SPACE . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...
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Ссылки http://www.energia.ru/en/iss/researches/works/18.html -- 25.8 Кб -- 10.04.2016
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17. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2014/AS01.html
ARCSAT ID NUMBER: AS01 DESCRIPTIVE TITLE: Stromgren Photometry of Galactic Streams PI: Dmitry Bizyaev OBSERVER(S): Dmitry Bizyaev UNCERTIFIED/UNTRAINED OBSERVERS: N/A COLLABORATORS: CONTACT INFORMATION: dmbiz @ apo.nmsu.edu TIME REQUESTED: 3 weeks in the dark time between May and October 2014 The preferred time slots (based on Mon - Sun basis) are: May 5 - 11 June 2-8 September 22 - 28 INSTRUMENT: SurveyCam FILTERS : ... The standard Stromgren set is available at APO. ... 2014). ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2014/AS01.html -- 3.6 Кб -- 06.05.2014
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18. FIRPO Help 1
... This gives a nice opportunity to check the quality of the FIRPO photometry against that of TIRGO. ... The values are Program POLYFIT V 10/Jul/90 ( A.Richichi ) - 24-Aug-1997 13:38:25 File : diff_temp_jc.dat Pol. degree: 1- N = 10- [ 2786.00- 4095.00 ] - [ 0.00- 1194.00] 1 -.10304E+01 0.26412E+00 2 0.29958E-03 0.74406E-04 sdev: 0.16063E+00 chi2 :0.24486E+01 Program POLYFIT V 10/Jul/90 ( A.Richichi ) - 24-Aug-1997 13:42:59 File : diff_temp_hc.dat Pol. degree: 1- N = 10- [ 2786.00- ...
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Ссылки http://www.arcetri.astro.it/irlab/luna/firpo/firpo_message8.html -- 6.2 Кб -- 28.07.2005
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19. Geomagnetic storms [Oulu]
... Geomagnetic activity can be divided into two main categories, storms and substorms . Storms, the main contributors to space weather , are initiated when enhanced energy transfer from the solar wind/IMF into the magnetosphere leads into intensification of ring current . The ring current development can be monitored with the Dst index . ... Iyemori, T., and D. R. K. Rao, Decay of the Dst field of geomagnetic disturbances after substorm onset and its implication to storm-substorm relation, Ann. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/storms.html -- 7.5 Кб -- 21.12.2007
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20. Generation from In-Orbit Data
... Analysis of in-orbit data closely follow the CSL data analysis. Stars with known astrometric positions are matched with their image centroids. ... The measured position, the expected position and the offset between the measured and expected positions are calculated and written into a file. ... select catalogued positions for different observations/pointings (e.g. positions of objects in photometric sequence) . ... The new distortion map was generated from in-flight observations of the G153 field. ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node912.html -- 5.9 Кб -- 20.09.2011
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