Abstract
We explore a possibility that the daily sea-level pressure (SLP) over South Korea responds to the high-speed solar wind event. This is of interest in two aspects: first, if there is a statistical association this can be another piece of evidence showing that various meteorological observables indeed respond to variations in the interplanetary environment. Second, this can be a very crucial observational constraint since most models proposed so far are expected to preferentially work in higher latitude regions than the low latitude region studied here. We have examined daily solar wind speed V, daily SLP difference ΔSLP, and daily log(BV 2 ) using the superposed epoch analysis in which the key date is set such that the daily solar wind speed exceeds 800 km s -1 . We find that the daily ΔSLP averaged out of 12 events reaches its peak at day +1 and gradually decreases back to its normal level. The amount of positive deviation of ΔSLP is +2.5 hPa. The duration of deviation is a few days. We also find that ΔSLP is well correlated with both the speed of solar wind and log(BV 2 ). The obtained linear correlation coefficients and chance probabilities with one-day lag for two cases are r ≃ 0.81 with P > 99.9%, and r ≃ 0.84 with P > 99.9%, respectively. We conclude by briefly discussing future direction to pursue.
Original language | English |
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Pages (from-to) | 777-782 |
Number of pages | 6 |
Journal | Advances in Space Research |
Volume | 50 |
Issue number | 6 |
DOIs | |
State | Published - 15 Sep 2012 |
Keywords
- Sea-level pressure
- Solar wind
- Solar-terrestrial weather