Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1768392 | Advances in Space Research | 2007 | 8 Pages |
Abstract
The time series of electron density profiles N(h) obtained at midlatitude station Ebro (40.5°N, 0.5°E) since 1995 up to now have been evaluated in order to obtain the typical time/altitude electron density variability. The standard deviation Ï(h) of the individual profiles from Monthly Averaged Representative Profile (MARP) is used for such purpose. The percentage of Ï(h) vs. MARP shows a distinct daily, seasonal and altitude pattern of variability. As expected, the larger variability occurs during night-time, there being however much better expressed at the base of the F region. Typical values of percentage of variability at altitudes of the electron density maximum are 10-20%, whereas they can be as large as 50% during night-time at the base of the F region. The systematic daily, seasonal and long-term behaviors of Ï(h) are discussed in terms of potential modeling purposes. The potential physical causes driving systematic behavior of Ï(h) are discussed also.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
D. Altadill,