... of this exceptional solar flare and we have been able to use these data to better characterise the flare's X-ray peak ... These flares reveal that, even when we simulate saturation of the GOES-12 sensor, we can still determine the flare peak ...
... timescale of flares is such that the currents through the photosphere do not have time to change over the course of the flare ... within active regions may undergo multiple flaring events, the maximum current need not be transferred in a single flare ...
... flares Mark Bennett University of Melbourne with thanks to Chris Thompson Orange Pulsar Meeting 27 September 2010 Outline 1 ... flares, avalanches) time (seconds) (Woods & Thompson 2006) bursts per 10 day interval 103 counts/second year (Hurley 2010 ...
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Ссылки http://www.atnf.csiro.au/research/pulsar/orange10/pdf/MarkBennettOrange2010.pdf -- 2113.0 Кб -- 27.09.2010 Похожие документы
... CASS News . Cheap Aussie telescope captures world's biggest solar flare. ... Using a "simple" 20 MHz interferometer, ATNF staff have made unique measurements of the 5 November 2003 solar flare. ...
... al. reported that one source, G9.62+0.20E, exhibited flares at 12.2 and 6.7 GHz that ... A subsequent flare was observed with the VLBA (Goedhart et al. 2005) at 12.2 GHz at ...
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Ссылки http://www.atnf.csiro.au/research/masermeeting/web_papers/316_Gaylard.pdf -- 1217.1 Кб -- 25.03.2007 Похожие документы
... Do you think it is possibility that the flare might be delayed by a few hours? ... be that we'll catch some flaring activity during the ATCA observations before VLBI ...
... Do you think it is possibility that the flare might be delayed by a few . hours? ... It could be that we'll catch some flaring activity during the ATCA . ... during the non-flaring state, where average flux is usually within +/- . 10 . mJy. ...