scholarly journals Automatic Real-time Beat-to-beat Detection of Arrhythmia Conditions

Author(s):  
Giovanni Rosa ◽  
Gennaro Laudato ◽  
Angela Colavita ◽  
Simone Scalabrino ◽  
Rocco Oliveto
Keyword(s):  
Sensors ◽  
2019 ◽  
Vol 19 (16) ◽  
pp. 3472 ◽  
Author(s):  
D’Mello ◽  
Skoric ◽  
Xu ◽  
Roche ◽  
Lortie ◽  
...  

Cardiography is an indispensable element of health care. However, the accessibility of at-home cardiac monitoring is limited by device complexity, accuracy, and cost. We have developed a real-time algorithm for heart rate monitoring and beat detection implemented in a custom-built, affordable system. These measurements were processed from seismocardiography (SCG) and gyrocardiography (GCG) signals recorded at the sternum, with concurrent electrocardiography (ECG) used as a reference. Our system demonstrated the feasibility of non-invasive electro-mechanical cardiac monitoring on supine, stationary subjects at a cost of $100, and with the SCG–GCG and ECG algorithms decoupled as standalone measurements. Testing was performed on 25 subjects in the supine position when relaxed, and when recovering from physical exercise, to record 23,984 cardiac cycles at heart rates in the range of 36–140 bpm. The correlation between the two measurements had r2 coefficients of 0.9783 and 0.9982 for normal (averaged) and instantaneous (beat identification) heart rates, respectively. At a sampling frequency of 250 Hz, the average computational time required was 0.088 s per measurement cycle, indicating the maximum refresh rate. A combined SCG and GCG measurement was found to improve accuracy due to fundamentally different noise rejection criteria in the mutually orthogonal signals. The speed, accuracy, and simplicity of our system validated its potential as a real-time, non-invasive, and affordable solution for outpatient cardiac monitoring in situations with negligible motion artifact.


2013 ◽  
Vol 401-403 ◽  
pp. 1234-1238
Author(s):  
Yong Bin Cheng ◽  
Li Qiang Zhu ◽  
Da Cheng Bi

In this study, a non-load blanket device for heart rate detection was designed, based on the function of ballistocardiogram (BCG) to characterize each heart beat. A bed blanket with underlaid pressure-sensitive cables was employed to simultaneously collect the BCGs and record the amplitude as well as frequency of heart beat in real time. The noise jamming was reasonably eliminated according to the Mallat fast algorithm with characteristics of BCG retained in the process. The obtained results of ballistocar-waveforms with obvious characters and values of cardiac rate demonstrated that good effects could be obtained by our heart beat detection device. This study proves to be a significant attempt for the BCG application on physiological parameters detections.


Author(s):  
Tom Torfs ◽  
Refet Firat Yazicioglu ◽  
Sunyoung Kim ◽  
Hyejung Kim ◽  
Chris Van Hoof ◽  
...  

Author(s):  
Fikana Mahardika Cantri ◽  
Zaqiatud Darojah ◽  
Endah Suryawati Ningrum

2020 ◽  
Vol 41 (5) ◽  
pp. 054004 ◽  
Author(s):  
Zhipeng Cai ◽  
Jianqing Li ◽  
Alistair E W Johnson ◽  
Xiangyu Zhang ◽  
Qin Shen ◽  
...  

Author(s):  
Yamin Arefeen ◽  
Philip Taffet ◽  
Daniel Zdeblick ◽  
Jorge Quintero ◽  
Greg Harper ◽  
...  

2015 ◽  
Vol 30 (5) ◽  
pp. 715-725 ◽  
Author(s):  
Xiaochang Liu ◽  
Gaofeng Wang ◽  
Jia Liu

1979 ◽  
Vol 44 ◽  
pp. 41-47
Author(s):  
Donald A. Landman

This paper describes some recent results of our quiescent prominence spectrometry program at the Mees Solar Observatory on Haleakala. The observations were made with the 25 cm coronagraph/coudé spectrograph system using a silicon vidicon detector. This detector consists of 500 contiguous channels covering approximately 6 or 80 Å, depending on the grating used. The instrument is interfaced to the Observatory’s PDP 11/45 computer system, and has the important advantages of wide spectral response, linearity and signal-averaging with real-time display. Its principal drawback is the relatively small target size. For the present work, the aperture was about 3″ × 5″. Absolute intensity calibrations were made by measuring quiet regions near sun center.


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