Sparse classification of discriminant nystagmus features using combined video-oculography tests and pupil tracking for common vestibular disorder recognition

Author(s):  
Aymen Mouelhi ◽  
Amine Ben Slama ◽  
Jihene Marrakchi ◽  
Hedi Trabelsi ◽  
Mounir Sayadi ◽  
...  
2020 ◽  
Vol 40 (01) ◽  
pp. 130-137 ◽  
Author(s):  
Jeffrey P. Staab

AbstractPersistent postural-perceptual dizziness (PPPD) was defined for the International Classification of Vestibular Disorders in 2017. It is a chronic vestibular disorder that manifests with waxing and waning symptoms of dizziness, unsteadiness, or nonspinning vertigo that last for 3 months or more and are exacerbated by upright posture, active or passive motion of self, and exposure to environments with complex or moving visual stimuli. Triggers of PPPD include a wide variety of conditions that may cause vestibular symptoms or disrupt balance functioning, including neuro-otologic and other medical conditions and psychological distress. The diagnosis is made by identifying key symptoms in patients' histories and conducting physical examinations and diagnostic testing of sufficient detail to establish PPPD as opposed to other illnesses. Ongoing research is providing insights into the pathophysiological mechanisms underlying PPPD and support for multimodality treatment plans incorporating specially adapted vestibular rehabilitation, serotonergic medications, and cognitive-behavior therapy.


2017 ◽  
Vol 46 (5) ◽  
pp. 1464-1473 ◽  
Author(s):  
Ahmed M. Elkady ◽  
Dana Cobzas ◽  
Hongfu Sun ◽  
Gregg Blevins ◽  
Alan H. Wilman

NeuroImage ◽  
2012 ◽  
Vol 60 (2) ◽  
pp. 1106-1116 ◽  
Author(s):  
Manhua Liu ◽  
Daoqiang Zhang ◽  
Dinggang Shen

Mechatronics ◽  
2015 ◽  
Vol 31 ◽  
pp. 60-67 ◽  
Author(s):  
Gang Tang ◽  
Qin Yang ◽  
Hua-Qing Wang ◽  
Gang-gang Luo ◽  
Jian-wei Ma

1966 ◽  
Vol 24 ◽  
pp. 21-23
Author(s):  
Y. Fujita

We have investigated the spectrograms (dispersion: 8Å/mm) in the photographic infrared region fromλ7500 toλ9000 of some carbon stars obtained by the coudé spectrograph of the 74-inch reflector attached to the Okayama Astrophysical Observatory. The names of the stars investigated are listed in Table 1.


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