First report of sporadic K layers and comparison with sporadic Na layers at Beijing, China (40.6°N, 116.2°E)
A double‐laser beam lidar was successfully developed to simultaneously measure K and Na layers at Beijing (40.6°N, 116.2°E) in 2010. Statistical analysis of the parameters of sporadic K (Ks) and sporadic Na (Nas) layers was performed over 2 years of lidar data, and different characteristics of them...
Gespeichert in:
Veröffentlicht in: | Journal of geophysical research. Space physics 2015-06, Vol.120 (6), p.5214-5225 |
---|---|
Hauptverfasser: | , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
Zusammenfassung: | A double‐laser beam lidar was successfully developed to simultaneously measure K and Na layers at Beijing (40.6°N, 116.2°E) in 2010. Statistical analysis of the parameters of sporadic K (Ks) and sporadic Na (Nas) layers was performed over 2 years of lidar data, and different characteristics of them were found. The average Ks occurrence (2.9%) was lower than that of Nas (5.9%); the Nas occurrence had a maximum (19.3%) in May–June months and a minimum (1.6%) in January–February months, while the Ks occurrence had a maximum (4.9%) in January–February months and a minimum (1.0%) in September–October months; most Ks peaks tended to occur around 93 km, which was ~2 km lower than that of Nas (~95 km); the Ks peak density was often at least 1 order of magnitude lower than that of Nas; notably, two Ks with high peak densities (>1000 cm−3) were observed, which were much higher than K density (15–300 cm−3) reported before. The ascending time of Ks was often longer than its descending time, but an opposite trend occurred for Nas. During the 152 cases of joint observation for the K and Na layers, 21% (32/152) were cases in which Ks and Nas events simultaneously occurred, while 79% (120/152) were cases in which only one layer (K or Na) exhibited a strong Ks or Nas.
Key Points
The Ks occurrence rate was much higher than that of Nas in January–February months
Two much high peak densities of Ks existed during observation nights
Ks events need more formation time than do Nas events |
---|---|
ISSN: | 2169-9380 2169-9402 |
DOI: | 10.1002/2014JA020955 |