dc.contributor.author |
Sastri, J. H |
|
dc.date.accessioned |
2009-03-25T10:54:37Z |
|
dc.date.available |
2009-03-25T10:54:37Z |
|
dc.date.issued |
1981-07 |
|
dc.identifier.citation |
Planetary and Space Science, Vol. 29, No. 7, pp. 741 - 745 |
en |
dc.identifier.issn |
0032-0633 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4421 |
|
dc.description |
Restricted Access |
|
dc.description.abstract |
From an analysis of published geomagnetic data of stations in the Indian equatorial region, it is shown that on days with an abnormal Sq (H) phase limited to the electrojet belt, conditions characteristic of complete or partial counter-electrojet prevail around the usual time interval of the diurnal maximum of the H-field. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Pergamon Press Ltd. |
en |
dc.relation.uri |
http://dx.doi.org/10.1016/0032-0633(81)90045-3 |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1981P%26SS...29..741S |
en |
dc.subject |
Equatorial Electrojet Region |
en |
dc.title |
Occurrence of abnormal Sq (H) phase in the equatorial electrojet region |
en |
dc.type |
Article |
en |