Abstract

The Jamaican primary dry season extends from November-April with the driest period being January-March each year. Examination of the rainfall records over several decades reveal months that experienced a sharp increase in rainfall while sometimes they are drier than normal. During this dry season, some of the weather systems that impact the island significantly are cold fronts, highs pressure systems and troughs that migrate from the mainland USA. Major Sudden Stratospheric Warmings (SSW) occur routinely north of 60°N and severely impact weather over the North American continent. The islands of the Greater Antilles also experience inclement weather during this period as weather systems migrate southwards and impact the Caribbean. Severe winter weather due to the increase frequency and intensity of storms related to SSW events over North America is important to the Jamaican economy as tourists escape harsh winters by travelling to the island. Predicting the variability of rainfall during the primary dry season is therefore important as it has significant implications for event planning, tourism and agriculture. Cosmic-ray Muon flux has been found to be positively correlated with the atmospheric effective temperature used to indicate the occurrence of SSW events. Current research investigates the relationship between cosmic-ray Muon flux, SSW events and primary dry season rainfall. Our findings suggest that a significant change in rainfall occur over Jamaica during the primary dry season on average 29 days after the central date or on average 15 days after the SSW events end. Our study also suggests apparent similarities in the behaviour of cosmic-ray Muon flux over Jamaica to those when major SSW occurs at high latitudes. We therefore argue that the Muon detectors at low latitudes have practical use with respect to identifying SSWs and merits further study.

Highlights

  • While astronomical seasons have fixed periods based on the position of the Sun with the boreal winter starting December 21 and ending March 20, the meteorological seasons are based on changes in the climatological temperature and cover a portion of the astronomical season

  • An examination of the Stratospheric Warming (SSW)-primary dry season (PDS) profile developed for this study indicated that while the number of SSWs has increased, there has been significant variability in rainfall during the driest period (Jan-Mar)

  • Cosmic ray Muons are sub-atomicparticles formed when cosmic radiation interact with molecules within the Earth’s atmosphere. This interaction initially takes place in the lower stratosphere resulting in formation of other Pions and Kaons, which decay almost immediately to Muons

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Summary

Introduction

While astronomical seasons have fixed periods based on the position of the Sun with the boreal winter starting December 21 and ending March 20, the meteorological seasons are based on changes in the climatological temperature and cover a portion of the astronomical season. An examination of the SSW-PDS profile developed for this study indicated that while the number of SSWs has increased, there has been significant variability in rainfall during the driest period (Jan-Mar). In their study [29] used Geiger Muller detectors to measure Muon counts for different 5-hour periods throughout the day and suggest that the cosmic-ray Muon counts were most times inversely correlated to the altitude of the freezing level (0 ̊C level) They observed that when meteorological fronts and troughs were near the detector, a reversal pattern occurs, that is, the graph would show negative slope at the first increment of a date rather than a positive one. This greater travel path increases the probability of Muons decaying before reaching ground based detectors

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