scholarly journals In vivo magnetic recording of neuronal activity

2016 ◽  
Author(s):  
Laure Caruso ◽  
Thomas Wunderle ◽  
Christopher Murphy Lewis ◽  
Joao Valadeiro ◽  
Vincent Trauchessec ◽  
...  

SUMMARYNeuronal activity generates ionic flows and thereby both magnetic fields and electric potential differences, i.e. voltages. Voltage measurements are widely used, but suffer from isolating and smearing properties of tissue between source and sensor, are blind to ionic flow direction, and reflect the difference between two electrodes, complicating interpretation. Magnetic field measurements could overcome these limitations, but have been essentially limited to magnetoencephalography (MEG), using centimeter-sized, helium-cooled extracranial sensors. Here, we report on in vivo magnetic recordings of neuronal activity from visual cortex of cats with magnetrodes, specially developed needle-shaped probes carrying micron-sized, non-cooled magnetic sensors based on spin electronics. Event-related magnetic fields inside the neuropil were on the order of several nanoteslas, informing MEG source models and efforts for magnetic field measurements through MRI. Though the signal-to-noise ratio is still inferior to electrophysiology, this proof of concept demonstrates the potential to exploit the fundamental advantages of magnetophysiology.HIGHLIGHTSSpin-electronics based probes achieve local magnetic recordings inside the neuropilMagnetic field recordings were performed in vivo, in anesthetized cat visual cortexEvent-related fields (ERFs) to visual stimuli were up to several nanoteslas in sizeERFs could be detected after averaging less than 20 trialsIN BRIEFCaruso et al. report in vivo, intra-cortical recordings of magnetic fields that reflect neuronal activity, using magnetrodes, i.e. micron size magnetic sensors based on spin electronics.

2005 ◽  
Author(s):  
Animesh Jain ◽  
John Escallier ◽  
George Ganetis ◽  
Wing Louie ◽  
Andrew Marone ◽  
...  

2017 ◽  
Vol 338 (8) ◽  
pp. 910-918 ◽  
Author(s):  
A. S. Medvedev ◽  
A. F. Kholtygin ◽  
S. Hubrig ◽  
M. Schöller ◽  
S. Fabrika ◽  
...  

2014 ◽  
Vol 9 (S307) ◽  
pp. 401-403 ◽  
Author(s):  
G. A. Wade ◽  
C. P. Folsom ◽  
J. Grunhut ◽  
J. D. Landstreet ◽  
V. Petit

AbstractWe have obtained high-quality magnetic field measurements of 19 sharp-lined B-type stars with precisely-measured N/C abundance ratios (Nieva & Przybilla 2012). Our primary goal is to test the idea (Meynetet al. 2011) that a magnetic field may explain extra drag (through the wind) on the surface rotation, thus producing more internal shear and mixing, and thus could provide an explanation for the appearance of slowly rotating N-rich main sequence B stars.


2001 ◽  
Vol 22 (5) ◽  
pp. 294-305 ◽  
Author(s):  
W. T. Kaune ◽  
R. S. Banks ◽  
M. S. Linet ◽  
E. E. Hatch ◽  
R. A. Kleinerman ◽  
...  

2008 ◽  
Vol 4 (S259) ◽  
pp. 389-390
Author(s):  
Swetlana Hubrig ◽  
M. Briquet ◽  
P. De Cat ◽  
M. Schöller ◽  
T. Morel ◽  
...  

AbstractWe present the results of the continuation of our magnetic survey with FORS 1 at the VLT of a sample of B-type stars consisting of confirmed or candidate β Cephei stars and Slowly Pulsating B stars. Roughly one third of the studied β Cephei stars have detected magnetic fields. The fraction of magnetic Slowly Pulsating B and candidate Slowly Pulsating B stars is found to be higher, up to 50%. We find that the domains of magnetic and non-magnetic pulsating stars in the H-R diagram largely overlap, and no clear picture emerges as to the possible evolution of the magnetic field across the main sequence.


2005 ◽  
Vol 15 (2) ◽  
pp. 1221-1224 ◽  
Author(s):  
A. Jain ◽  
J. Escallier ◽  
G. Ganetis ◽  
W. Louie ◽  
A. Marone ◽  
...  

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