A Comment on the Letter by G.G. Howes, Phys. Rev. Lett.PRLTAO0031-9007 100, 065004 (2008)10.1103/PhysRevLett.100.065004. The authors of the Letter offer a Reply. © 2008 The American Physical Society.Fil: Matthaeus, W. H.. University of Delaware Newark; Estados UnidosFil: Servidio, S.. University of Delaware Newark; Estados UnidosFil: Dmitruk, Pablo Ariel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentin
This recent paper reports some real advances in experimental technique, but is misleading or incorre...
We welcome the comment made by Lund [this is-sue] as this provides us an opportunity to clarify some...
2 pages. Accepted at "Astronomy and Astrophysics".International audienceTsiklauri et al. recently pu...
In their preceding comment on our paper [Matthaeus et al., 1994] (hereinafter reffered to as paper 1...
In this response, we address the three main comments by Tsurutani et al. (2018, http://doi.org/10.10...
In a recent publication, viz. [Phys. Lett. A 326 (2004) 267], Jovanovic and Shukla (J. and S. in the...
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Collisionless shocks and plasma turbulence are crucial ingredients for a broad range of astrophysica...
The magnetorotational instability (MRI) is a fundamental mechanism determining the macroscopic dynam...
International audienceAn alternative scenario to the Ngwira et al. (2014, https://doi-org.insu.bib.c...
tions to our interpretation of dayside auroral transients and associated azimuthal flow bursts in te...
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAM...
The comment addresses questions raised on the derivation of the momentum pinch velocity due to the C...
A Comment on the Letter by L. Deng, M. G. Payne, and E. W. Hagley, Phys. Rev. Lett. 104 050402 (2010...
Despite the increasing sophistication of numerical models of hot Jupiter atmospheres, the large time...
This recent paper reports some real advances in experimental technique, but is misleading or incorre...
We welcome the comment made by Lund [this is-sue] as this provides us an opportunity to clarify some...
2 pages. Accepted at "Astronomy and Astrophysics".International audienceTsiklauri et al. recently pu...
In their preceding comment on our paper [Matthaeus et al., 1994] (hereinafter reffered to as paper 1...
In this response, we address the three main comments by Tsurutani et al. (2018, http://doi.org/10.10...
In a recent publication, viz. [Phys. Lett. A 326 (2004) 267], Jovanovic and Shukla (J. and S. in the...
We respond to Dikpati et al.'s criticism of our recent solar dynamo model. A different treatment of ...
Collisionless shocks and plasma turbulence are crucial ingredients for a broad range of astrophysica...
The magnetorotational instability (MRI) is a fundamental mechanism determining the macroscopic dynam...
International audienceAn alternative scenario to the Ngwira et al. (2014, https://doi-org.insu.bib.c...
tions to our interpretation of dayside auroral transients and associated azimuthal flow bursts in te...
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAM...
The comment addresses questions raised on the derivation of the momentum pinch velocity due to the C...
A Comment on the Letter by L. Deng, M. G. Payne, and E. W. Hagley, Phys. Rev. Lett. 104 050402 (2010...
Despite the increasing sophistication of numerical models of hot Jupiter atmospheres, the large time...
This recent paper reports some real advances in experimental technique, but is misleading or incorre...
We welcome the comment made by Lund [this is-sue] as this provides us an opportunity to clarify some...
2 pages. Accepted at "Astronomy and Astrophysics".International audienceTsiklauri et al. recently pu...