Statistical Associations between Geomagnetic Activity, Solar Wind, Cosmic Ray Intensity, and Heart Rate Variability in Patients after Open-Heart Surgery

被引:2
作者
Vencloviene, Jone [1 ,2 ]
Beresnevaite, Margarita [2 ]
Cerkauskaite, Sonata [1 ]
Ragaisyte, Nijole [3 ]
Pilviniene, Rugile [3 ]
Benetis, Rimantas [2 ,4 ]
机构
[1] Vytautas Magnus Univ, Dept Environm Sci, Donelaicio St 58, LT-44248 Kaunas, Lithuania
[2] Lithuanian Univ Hlth Sci, Inst Cardiol, Sukileliu St 15, LT-50103 Kaunas, Lithuania
[3] Lithuanian Univ Hlth Sci, Inst Physiol & Pharmacol, A Mickeviciaus St 9, LT-44307 Kaunas, Lithuania
[4] Lithuanian Univ Hlth Sci, Clin Dept Cardiac Thorac & Vasc Surg, Eiveniu St 2, LT-50161 Kaunas, Lithuania
关键词
heart rate variability; geomagnetic activity; solar wind; cosmic ray intensity; patients after open-heart surgery; CLOUD MICROPHYSICS; CIRCULATION; VORTICITY; WEATHER; HRV;
D O I
10.3390/atmos13081330
中图分类号
X [环境科学、安全科学];
学科分类号
08 ; 0830 ;
摘要
The aim of this study was to identify associations of the parameters of heart rate variability (HRV) with the variations in geomagnetic activity (GMA), solar wind, and cosmic ray intensity (CRI) in patients after coronary artery bypass grafting or valve surgery in Kaunas, Lithuania, during 2008-2012. The data from 5-minute electrocardiograms (ECGs) in 220 patients were used. ECGs were carried out at 1.5 months, 1 year, and 2 years after the surgery (N = 495). A lower (higher) very-low-frequency-band (VLF) and a higher (lower) high-frequency band (HF) in normalised units (n.u.) were associated with a low maximal daily 3-hourly ap (the DST index > 1). A lower mean standard deviation of beat-to-beat intervals (SDNN) and VLF, LF, and HF powers were lower in patients when Ap < 8 occurred two days after the surgery, and a low solar wind speed (SWS) occurred two days before the ECG. The effect of CRI was non-significant if the linear trend was included in the model. Low GMA and a low SWS may effect some HRV variables in patients after open-heart surgery. The GMA during the surgery may affect the SDNN in short-term ECG during the longer period.
引用
收藏
页数:12
相关论文
共 64 条
[1]   Focused exposures to airborne traffic particles and heart rate variability in the elderly [J].
Adar, Sara Dubowsky ;
Gold, Diane R. ;
Coull, Brent A. ;
Schwartz, Joel ;
Stone, Peter H. ;
Suh, Helen .
EPIDEMIOLOGY, 2007, 18 (01) :95-103
[2]   Long-Term Study of Heart Rate Variability Responses to Changes in the Solar and Geomagnetic Environment [J].
Alabdulgader, Abdullah ;
McCraty, Rollin ;
Atkinson, Michael ;
Dobyns, York ;
Vainoras, Alfonsas ;
Ragulskis, Minvydas ;
Stolc, Viktor .
SCIENTIFIC REPORTS, 2018, 8
[3]   Solar wind drivers of energetic electron precipitation [J].
Asikainen, T. ;
Ruopsa, M. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2016, 121 (03) :2209-2225
[4]  
Baevsky R. M., 1997, Scripta Medica (Brno), V70, P201
[5]   Is the Dst Index Sufficient to Define All Geospace Storms? [J].
Borovsky, Joseph E. ;
Shprits, Yuri Y. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2017, 122 (11) :11543-11547
[6]  
Breiman L., 2017, Classification and Regression Trees
[7]  
Breus T.K., 2012, J. Biomed. Sci. Eng, V5, P341, DOI [DOI 10.4236/JBISE.2012.56044, 10.4236/jbise.2012.56044]
[8]   Simulated sudden increase in geomagnetic activity and its effect on heart rate variability: Experimental verification of correlation studies [J].
Caswell, Joseph M. ;
Singh, Manraj ;
Persinger, Michael A. .
LIFE SCIENCES IN SPACE RESEARCH, 2016, 10 :47-52
[9]   Is Low Heart Rate Variability Associated with Emotional Dysregulation, Psychopathological Dimensions, and Prefrontal Dysfunctions? An Integrative View [J].
Cattaneo, Lorena Angela ;
Franquillo, Anna Chiara ;
Grecucci, Alessandro ;
Beccia, Laura ;
Caretti, Vincenzo ;
Dadomo, Harold .
JOURNAL OF PERSONALIZED MEDICINE, 2021, 11 (09)
[10]   Non-photic solar associations of heart rate variability and myocardial infarction [J].
Cornélissen, G ;
Halberg, F ;
Breus, T ;
Syutkina, EV ;
Baevsky, R ;
Weydahl, A ;
Watanabe, Y ;
Otsuka, K ;
Siegelova, J ;
Fiser, B ;
Bakken, EE .
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2002, 64 (5-6) :707-720