dc.contributor.author | Verma, V. K. | |
dc.contributor.author | Pande, M. C. | |
dc.date.accessioned | 2010-02-08T06:53:20Z | |
dc.date.available | 2010-02-08T06:53:20Z | |
dc.date.issued | 1985 | |
dc.identifier.uri | http://hdl.handle.net/123456789/488 | |
dc.description.abstract | The analysis of 315 hard X-ray bursts (HXR) producing solar flares observed by Hinotori satellite shows that the HXR bursts occur most prominently at 110°, 140°, 290° and 320° longitude, respectively. These longitudes are not only prolific in producing flares in number but also in producing flares with large photon counts. | en_US |
dc.language.iso | en | en_US |
dc.relation.ispartofseries | sp99-285 | |
dc.subject | Solar System, X-ray | en_US |
dc.title | Longitudinal distribution of the hard X-ray bursts on the sun | en_US |
dc.type | Article | en_US |