Ring current ion flows and convection electric field as expected from observations by SAC-B/ISENA
In the present paper, ENA energy spectra at the location at the SAC‐B satellite are simulated by using AMPTE/CCE/CHEM ion distributions as originating source, with the purpose of analysing the SACB/ISENA response at different magnetic local times and latitudes. The shape of the ENA spectra simulated...
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| Veröffentlicht in: | Geophysical research letters 1996-11, Vol.23 (23), p.3285-3288 |
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| container_end_page | 3288 |
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| container_issue | 23 |
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| container_title | Geophysical research letters |
| container_volume | 23 |
| creator | Milillo, A. Orsini, S. Daglis, I. A. Candidi, M. |
| description | In the present paper, ENA energy spectra at the location at the SAC‐B satellite are simulated by using AMPTE/CCE/CHEM ion distributions as originating source, with the purpose of analysing the SACB/ISENA response at different magnetic local times and latitudes. The shape of the ENA spectra simulated along different lines of sight on the equatorial plane is analysed to show that an instantaneous estimate of the global convection electric field will be possible with the ISENA data every few minutes. This unprecedented time resolution for the measurement of such a crucial parameter of the Earths magnetosphere will allow testing of many theories, like tail convection, pressure balance, global circuits, ring‐current shielding, etc, |
| doi_str_mv | 10.1029/96GL02925 |
| format | Article |
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A.</au><au>Candidi, M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Ring current ion flows and convection electric field as expected from observations by SAC-B/ISENA</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>1996-11-15</date><risdate>1996</risdate><volume>23</volume><issue>23</issue><spage>3285</spage><epage>3288</epage><pages>3285-3288</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><coden>GPRLAJ</coden><abstract>In the present paper, ENA energy spectra at the location at the SAC‐B satellite are simulated by using AMPTE/CCE/CHEM ion distributions as originating source, with the purpose of analysing the SACB/ISENA response at different magnetic local times and latitudes. The shape of the ENA spectra simulated along different lines of sight on the equatorial plane is analysed to show that an instantaneous estimate of the global convection electric field will be possible with the ISENA data every few minutes. This unprecedented time resolution for the measurement of such a crucial parameter of the Earths magnetosphere will allow testing of many theories, like tail convection, pressure balance, global circuits, ring‐current shielding, etc,</abstract><cop>Washington, DC</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/96GL02925</doi><tpages>4</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0094-8276 |
| ispartof | Geophysical research letters, 1996-11, Vol.23 (23), p.3285-3288 |
| issn | 0094-8276 1944-8007 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_18150430 |
| source | Wiley Online Library Journals Frontfile Complete |
| subjects | Convection Earth magnetosphere Earth, ocean, space Electric fields Estimates Exact sciences and technology External geophysics Geophysics Physics of the magnetosphere Planes Position (location) Simulation Trapped particles |
| title | Ring current ion flows and convection electric field as expected from observations by SAC-B/ISENA |
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