The freiberg forceful internal rotation test for piriformis syndrome

Author(s):  
Steven D. Waldman
2002 ◽  
Vol 7 (1) ◽  
pp. 26-32 ◽  
Author(s):  
Eiji Suenaga ◽  
Yasuo Noguchi ◽  
Seiya Jingushi ◽  
Toshihide Shuto ◽  
Yasuharu Nakashima ◽  
...  

2019 ◽  
Vol 6 (4) ◽  
pp. 398-405 ◽  
Author(s):  
Victor Ortiz-Declet ◽  
Austin W Chen ◽  
David R Maldonado ◽  
Leslie C Yuen ◽  
Brian Mu ◽  
...  

Abstract The objective of this study was to evaluate the diagnostic accuracy of a new dynamic clinical examination for detection of gluteus medius (GM) tears. A case group of 50 patients undergoing arthroscopy with GM repair was compared with a control group of 50 patients undergoing arthroscopy who had no peritrochanteric symptoms. Both groups were examined clinically, had magnetic resonance imaging studies performed and underwent arthroscopic surgery. Recorded clinical examinations included abnormal gait (Trendelenburg), tenderness to palpation of the greater trochanter, resisted abduction and the test being studied, resisted internal rotation. For all clinical tests, the sensitivity, specificity, positive predictive value, negative predictive value and diagnostic accuracy rates were calculated and compared with the arthroscopic and MRI data for the case group, and the MRI data for the control group. The resisted internal rotation test had a sensitivity of 92%, specificity of 85% and diagnostic accuracy of 88% in the detection of GM tears, with a low rate of false-positive and false-negative recordings. Other traditional clinical examination tests, with the exception of Trendelenburg gait, showed inferior rates. Trendelenburg gait had a higher specificity, but much lower sensitivity. The resisted internal rotation test aides in the detection of GM pathology. Due to the good results of the resisted internal rotation test in all the diagnostic parameters, we recommend incorporating it on the physical exam of patients with hip pain.


2011 ◽  
Vol 36 (5) ◽  
pp. 782-787 ◽  
Author(s):  
Kensuke Ochi ◽  
Yukio Horiuchi ◽  
Aya Tanabe ◽  
Kozo Morita ◽  
Kentaro Takeda ◽  
...  

2015 ◽  
Vol 3 (2) ◽  
pp. 232596711557213 ◽  
Author(s):  
Samuel G. Moulton ◽  
Tyler R. Cram ◽  
Evan W. James ◽  
Grant J. Dornan ◽  
Nicholas I. Kennedy ◽  
...  

2019 ◽  
Vol 8 (3) ◽  
pp. e331-e334 ◽  
Author(s):  
Rafael Walker-Santiago ◽  
Victor Ortiz-Declet ◽  
David R. Maldonado ◽  
Natalia M. Wojnowski ◽  
Benjamin G. Domb

2018 ◽  
Vol Publish Ahead of Print ◽  
Author(s):  
Ajaykumar Shanmugaraj ◽  
Jaymee R. Shell ◽  
Nolan S. Horner ◽  
Andrew Duong ◽  
Nicole Simunovic ◽  
...  

2000 ◽  
Vol 179 ◽  
pp. 379-380
Author(s):  
Gaetano Belvedere ◽  
Kirill Kuzanyan ◽  
Dmitry Sokoloff

Extended abstractHere we outline how asymptotic models may contribute to the investigation of mean field dynamos applied to the solar convective zone. We calculate here a spatial 2-D structure of the mean magnetic field, adopting real profiles of the solar internal rotation (the Ω-effect) and an extended prescription of the turbulent α-effect. In our model assumptions we do not prescribe any meridional flow that might seriously affect the resulting generated magnetic fields. We do not assume apriori any region or layer as a preferred site for the dynamo action (such as the overshoot zone), but the location of the α- and Ω-effects results in the propagation of dynamo waves deep in the convection zone. We consider an axially symmetric magnetic field dynamo model in a differentially rotating spherical shell. The main assumption, when using asymptotic WKB methods, is that the absolute value of the dynamo number (regeneration rate) |D| is large, i.e., the spatial scale of the solution is small. Following the general idea of an asymptotic solution for dynamo waves (e.g., Kuzanyan & Sokoloff 1995), we search for a solution in the form of a power series with respect to the small parameter |D|–1/3(short wavelength scale). This solution is of the order of magnitude of exp(i|D|1/3S), where S is a scalar function of position.


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