TY - JOUR
T1 - Time/altitude electron density variability above Ebro, Spain
AU - Altadill, D.
N1 - Funding Information:
This work has been partially supported by Spanish project of MCYT (REN2003-08376-C02-02).
PY - 2007
Y1 - 2007
N2 - 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 σ(h) of the individual profiles from Monthly Averaged Representative Profile (MARP) is used for such purpose. The percentage of σ(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 σ(h) are discussed in terms of potential modeling purposes. The potential physical causes driving systematic behavior of σ(h) are discussed also.
AB - 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 σ(h) of the individual profiles from Monthly Averaged Representative Profile (MARP) is used for such purpose. The percentage of σ(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 σ(h) are discussed in terms of potential modeling purposes. The potential physical causes driving systematic behavior of σ(h) are discussed also.
KW - B parameters
KW - Electron density profiles
KW - IRI model
KW - Ionosphere variability
KW - Variability-quartile-median-IRI
UR - http://www.scopus.com/inward/record.url?scp=34249068221&partnerID=8YFLogxK
U2 - 10.1016/j.asr.2006.05.031
DO - 10.1016/j.asr.2006.05.031
M3 - Article
AN - SCOPUS:34249068221
SN - 0273-1177
VL - 39
SP - 962
EP - 969
JO - Advances in Space Research
JF - Advances in Space Research
IS - 5
ER -