One of the main conclusions that Peter Alexander states in the last paragraph of his article (Eos, October 13, 1992, p. 433) is: “It is also desirable to find an appropriate description of the electron heat conductivity for the distant collisionless solar wind because the classical Spitzer‐Harm conductivity represents an inadequate expression for that fluid.” ©1993. American Geophysical Union. All Rights Reserved.
Documento: | Artículo |
Título: | Comment to “History of solar coronal expansion studies” |
Autor: | Duhau, S. |
Filiación: | Laboratorio de Geofisica, Ciudad Universitaria, Buenos Aires, Argentina |
Año: | 1993 |
Volumen: | 74 |
Número: | 42 |
Página de inicio: | 484 |
Página de fin: | 484 |
DOI: | http://dx.doi.org/10.1029/93EO00314 |
Título revista: | Eos, Transactions American Geophysical Union |
Título revista abreviado: | Eos |
ISSN: | 00963941 |
Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00963941_v74_n42_p484_Duhau |