About the correlation between solar micro bursts and the change of the solar wind parameters
| dc.creator | Oliveros, Juan Carlos Martinez | |
| dc.creator | P, Daniel Ricardo Izquierdo | |
| dc.date | 2005-08-02 | |
| dc.date.accessioned | 2026-07-07T02:18:23Z | |
| dc.date.available | 2026-07-07T02:18:23Z | |
| dc.description | The Sun is the closest star to our planet and it is the most studied, perhaps, there exist too much procesess not-understood. One of the solar processes that have a direct interaction with the earth is the solar wind. The solar wind is defined as the plasma expulsed from the solar atmosphere, this wind was cataloged and is considered that have three components: - Passive solar wind: Is the constant component of the solar wind. - Supersonic and quasistady flux. - Sporadic supersonic flux. We present and brief explanation of the Parker's model of the solar wind and a correlation analysis between solar micro radio bursts and the change of the solar wind parameters. | |
| dc.description | Spanish text, 6 figures, 10 pages | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0508084 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0508084 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/9467 | |
| dc.subject | Astrophysics | |
| dc.title | About the correlation between solar micro bursts and the change of the solar wind parameters | |
| dc.type | text |