The three events are unambiguously identified with white-light coronal mass ejections (CMEs) that are associated in turn with surface activity of diverse nature: an impulsive (M-class) flare, a weak (B-class) flare, and a filament eruption without a flare. The use of three AIA coronal ...
Attrill, G.D.R., Wills-Davey, M.J.: 2010, Automatic Detection and Extraction of Coronal Dimmings from SDO/AIA Data. Solar Phys. 262, 461 - 480.Attrill, G.D.R., and M.J. Wills-Davey. Automatic detection and extraction of coronal dimmings from SDO/AIA data. Sol. Phys., 262, ...
摘要: This paper reports the obtained analysis data on the spatio-temporal evolution of sources of microwave and hard X-ray pulsations for the SOL2011-06-07T06:16 event based on the observation data of the...关键词: MICROWAVES HARD X-rays STELLAR oscillations SOLAR flares SPECTROMETERS RADIO...
图5: 发生爆发的太阳丝状物 , 影像提供: NASA'sGSFC, SDO AIA Team 图6: 罗塞塔号探测船证实彗星有二个核心 , 影像提供: ESA/Rosetta/MPSfor OSIRIS Team;MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA 图7: 渗漏极光的洞穴 , 影像提供与版权: Ing鏊fur Bjargmundsson ...
图5: Dark Filament of the Sun , 影像提供: NASA /Goddard /SDO AIA Team图6:日盘上的国际太空站及航天飞机 ,影像版权与提供: Thierry Legault图7: 心宿增四星 , 影像提供与版权: Rogelio Bernal Andreo图8: 回首来时路 , 影像提供: MarsExploration Rover Mission,JPL,NASA图9: M13: 武仙座的庞大球状...
The three events are unambiguously identified\nwith white-light coronal mass ejections (CMEs) associated in turn with surface\nactivity of diverse nature: an impulsive (M-class) flare, a weak (B-class)\nflare and a filament eruption without a flare. The use of three AIA coronal\npass...
SDO/AIAdataCoronalholeFluxtubeOscillationsWith high temporal resolution (12 s) of about two hours duration, data of a coronal hole structure in 171 Å , 193 Å and 211 Å taken from SDO/AIA images is considered for examination of oscillations. After estimating the total DN ...
The neural network is trained with nearly 8 years of data of Nobeyama Radioheliograph(No RH) at 17 GHz and SDO/AIA from January 2011 to September 2018. The generated radioheliograph image is in good consistency with the well-calibrated No RH observation. SDO/AIA provides solar atmosphere ...
Following Couvidat (2013), we analyze data from the Helioseismic and Magnetic\nImager (HMI) and the Atmospheric Imaging Assembly (AIA) instruments onboard the\nSolar Dynamics Observatory: Doppler velocity and continuum intensity at 6173 A\nas well as intensity maps at 1600 A and 1700 A. ...
The best two-component fit using ground-based Ca II K-line data was R2=0.873; using AIA 170nm produced R2=0.896. Correlations using the AIA 160nm data were consistently lower with values of R2 as low as 0.793, where R2 is the coefficient of multiple correlation.Cha...