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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• http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20150309.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20150330.en.txt
• http://www.izmiran.rssi.ru/services/saf/archive/en/2015/obzor20150209.en.txt

... 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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• Space weather forecast March 16, 2015
• Space weather forecast March 14, 2015
• Space weather forecast March 13, 2015

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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... 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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• Radio survey for new compact HII regions

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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• I Expected More Sense Than That. - an Astronomy Net Exploration Forum Message

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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• Leonid Meteors
• Code of Good Practice for Scholarly and Scientific Research
• Terry Mosely's Bulletins

... VLBI Schedule . ... Observers Wiki . ... Main / . ... Each DF has a header of 4 32-bit words followed by 2500 32-bit words of data (10000 bytes). ... m5data 2630/tcp # Mark5 data . ... Used to set the output data rate of the Mark5 at the station. Expected response: . ... Used to make the Mark5 stop playing if it was playing back data from disk. ... Used to make the Mark5 at the station start sending data. ... Used to make the Mark5 at the station stop sending data and terminate the connection. ...

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• lbaops:eapt:mark5control [ATNF VLBI Wiki]
• G Quirks and Unexpected Behaviour
• lbaops:mark5evlbi [ATNF VLBI Wiki]

... 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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• template for DFS Trouble Shooting Guide
• FORS1 Photometric System Characterization
• ESO - Real Time Follow-up of Transient Objects From PESSTO

Instrument Science Report WFC3 2004-09 Preliminary Assessment of Image Persistence in the WFC3 UVIS CCD Detector G. F. Hartig and S. Baggett 16 April 2004 ABSTRACT We have performed an initial assessment of the level of residual image persistence in the WFC3 UVIS CCD flight detectors. ... Highly saturated point source image at field point UV14 at 350 nm (left) and 100 s dark (right) at the same detector location, approximately 4 minutes later, showing no indication of image persistence. ...

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• http://www.stsci.edu/smov/SMOV4%20WEB%20PAGE%20OCT2007/SMOV4%20Activity%20Summaries/TCS.pdf
• FOC Data Handbook
• ST ScI Preprint #1401

Astronomy Picture of the Day . An Unexpected Aurora over Norway . ... 4.05.2015 . ... Credit Copyright: Tommy Richardsen Explanation: Sometimes the sky lights up unexpectedly. A trip to northern Norway to photograph auroras was not going as well as hoped. It was now past midnight in Steinsvik , Troms , in northern Norway , and the date was 2014 February 8. ... When the sky suddenly exploded with spectacular aurora . ... Publications with keywords: aurora . ... Aurora over Clouds . ...

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• Unexpected Comet Pojmanski Now Visible
• Астронет > Rays from an Unexpected Aurora
• Rays from an Unexpected Aurora

Geomagnetic disturbances can be monitored by ground-based magnetic observatories recording the three magnetic field components. The global Kp index is obtained as the mean value of the disturbance levels in the two horizontal field components, observed at 13 selected, subauroral stations . ... Geomagnetic activity is the occurrence of K variations. ... But K still remains a local index, describing disturbances in the vicinity of each observatory. ...

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• Energetic Particles
• Geomagnetic storms [Oulu]
• Incoherent scatter [Oulu]