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1. The CORONAS-PHOTON has registered the formation of the Sun's southern belt of
... The Russian TESIS/ CORONAS-PHOTON Solar Observatory, which has been working in orbit since January 30th, 2009, has photographed one of the most important events in the build up to the upcoming solar cycle - the formation of our star's new southern belt of activity. The first magnetic fields of the new cycle in the southern hemisphere appeared on the Sun's surface on May 23-24th. ... The belt of activity is one of the primary concepts, characterizing the solar cycle. ...
[ Сохраненная копия ]  Ссылки http://www.tesis.lebedev.ru/en/info/tesis_20090527_en.php -- 10.6 Кб -- 01.10.2012
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2. cash register cafeteria
... 22mar13:emissions in 327 Mhz Rcvr vs 904Efield probe strength. ... The emissions from an ELO model esy15e1 touch screen cash register was checked on 14feb13 in the screen room (by angel) and on 22mar13 using the 327 receiver on the telescope. People would like to use this cash register in the cafeteria. ... 100 to 3000 Mhz was covered in 100 Mhz sections. ... There is a 6.181Mhz comb that peaks at 245.83 Mhz. the strong birdie at 237.821 had harmonics at 475.9,713.385,951.. 1426.77 Mhz . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/rfi/miscdevice/elocashreg/cashRegCaf.html -- 11.6 Кб -- 01.04.2013
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3. REGISTER/ROMAFOT
... REGISTER/ROMAFOT int_tab reg_tab [wnd_opt] [obj_opt] . ... However, all the photometric information obtained from the frame as the absolute quantities (magnitudes, colour equations etc.) still have to be derived. ... Table: Romafot Registration Table . ... In case of program stars (search made with SEARCH/ROMAFOT ), these columns are filled with zeros. The instrumental magnitude MAG_CNV is calculated as , where VOL is the integral over the elementary surface to fit the star, calculated from to . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node105.html -- 3.7 Кб -- 23.02.1996
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4. "STP Data" STP Data
... 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) . ...
[ Сохраненная копия ]  Ссылки http://www.wdcb.ru/stp/welcome.shtml -- 11.9 Кб -- 18.01.2010
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5. Prediction technique
Geomagnetic storms and substorms are a natural hazard similar to hurricanes, floods etc. ... Solar and geomagnetic activity also probably influences the Earth's climate and human health. ... Under southward directed IMF the Earth's magnetosphere is open to input from the solar wind flow. ... Since practical importance of solar wind measurements was recognized, a number of approaches was developed for prediction of the geomagnetic activity basing on the solar wind data. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/apetruko/forecast/epsilon.html -- 7.5 Кб -- 27.01.2000
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/forecast/epsilon.html -- 7.5 Кб -- 27.01.2000
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6. Registering, PSF-Matching and Intensity-Matching Images in IRAF
... We have developed a set of tasks in the IRAF environment for registering, matching the point-spread functions, and matching the intensity scales of two or more images. ... The current software performs spatial registration by supplying the registration task with a reference and input image list, and a list of features common to both images. ... The current software requires the input and reference images to be spatially-registered and PSF-matched. ... CTIO 4-m images courtesy of Nelson Calwell.) ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/phillipsa.html -- 12.5 Кб -- 03.11.2000
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7. Geomagnetic Kp Index
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. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/KP_INDEX/kp.html -- 6.3 Кб -- 27.07.2001