Heart Rate Variations During Two Historic Geomagnetic Storms: October and November 2003

Abstract

The investigation of the two phenomena of Space Weather, i.e., Forbush decreases in the cosmic ray intensity and geomagnetic storms, is a highly developing field of modern scientific research, since these two phenomena can affect not only technological activities, e.g., electronics, telecommunications, navigations, etc., but also, as evidenced by recent studies, human life as well. This study analyses data of heart rate of volunteers of the Polyclinico Tor Vergata, Rome, Italy, with regard to geomagnetic field’s variations (i.e., geomagnetic storms) and cosmic ray intensity’s fluctuations (i.e., Forbush decreases). Data concerning geomagnetic (Dst- and Ap-index values) and cosmic ray activity derived from the Rome Cosmic Ray Station (Studio Variazioni Intensità Raggi Cosmici: S.V.I.R.CO.) were analyzed. The analysis expands from 24 April 2003 to 12 May 2004 and includes October–November 2003, which was a period of severe activity, when extreme events were recorded (i.e., the Great Halloween Solar Storms and the super storm on November 2003). The variations in heart rate were studied using the ANalysis Of Variance—ANOVA (for various levels of activity of the geophysical environment) and the superimposed epochs methods (during an event’s temporal evolution). Results revealed that high geomagnetic (defined by Dst-index values) and cosmic rays activity is related to heart rate increase. Moreover, the most significant heart rate variations are observed two days before until two days after the development of an event (either geomagnetic storm or a variation in the cosmic ray intensity). The results are in agreement with conclusions presented in the international scientific literature.

Keywords

• heliobiology
• heart rate
• Forbush decreases
• geomagnetic storms
• space weather
• physiological parameters