On the invariant representation of spin tensors with applications

The invariant representation of the spin tensor defined as the rotation rate of a principal triad for a symmetric and non-degenerate tensor is derived on the basis of the general solution of a linear tensorial equation. The result can be naturally specified to study the. spin of the stretch tensors and to investigate the relations between various rotation rate tensors encountered frequently in modern continuum mechanics. A remarkable formula which relates the generalized stress conjugate to the generalized strain in Hill's sense. to Cauchy stress, is obtained in invariant form through the work conjugate principle. Particularly, a detailed discussion on the time rate of logarithmic strain and its conjugate stress is made as the principal axes of strain arc not fixed during deformation.

The influence of momentum addition on the acceleration of the solar and stellar winds

The influence of the momentum addition, which may be associated with the average or fluctuation transverse component of the magnetic field or others, on the acceleration the solar wind or stellar wind is studied in a local streamtube. The results show that the larger the momentum addition the stronger the acceleration of the wind. For example, if the typical transverse magnetic field is about 0.1 of the longitudinal field, the velocity of the solar wind at 1 AU may be increased by 40%. The coronal hole may be considered as a streamtube, the presence of a high stream from the coronal hole may be explained by the existence of an average or fluctuation transverse magnetic field in the streamtube. A similar conclusion may be applied to the polar region, where the velocity of the solar wind will be larger than elsewhere as if there is a transverse component of magnetic field, as well as to the stellar wind. The influence of other parameters on the acceleration of the solar wind is also discussed. From the viewpoint of the solar wind mechanism, the present paper shows that the momentum addition in the subsonic flow region can increase the velocity of the solar wind at 1 AU.

Non-linear theory of a positive-column in a magnetic-field

A nonlinear theory of an intermediate pressure discharge column in a magnetic field is presented. Motion of the neutral gas is considered. The continuity and momentum transfer equations for charged particles and neutral particles are solved by numerical methods. The main result obtained is that the rotating velocities of ionic gas and neutral gas are approximately equal. Bohm's criterion and potential inversion in the presence of neutral gas motion are also discussed.

Los programas de apoyo a la creación de spin-offs académicas en las universidades españolas: una comparación internacional

XXII,1021 p.

Tipología de las spin-offs en un contexto universitario: una propuesta de clasificación

[ES] En los últimos tiempos existe un énfasis creciente en la comercialización de la investigación universitaria a través de la creación de empresas (spin-offs). Ahora bien, los fenómenos que el concepto de spin-off universitaria trata de abarcar no son homogéneos. Por esta razón, parece conveniente dilucidar las múltiples realidades que abarca organizándolas mediante tipologías.

La gestión empresarial como factor clave de desarrollo de las spin-offs universitarias. Análisis organizativo y financiero

[ES] En las últimas décadas el número de spin-offs universitarias creadas en el Sistema Universitario Español ha aumentado considerablemente; sin embargo, estas empresas tienen que hacer frente a problemas como la falta de financiación o de capacidades empresariales por parte de los fundadores. A partir de los datos extraídos de una encuesta a 72 spin-offs creadas en España, tratamos de detectar y analizar cuáles son los problemas más habituales con los que se encuentran estas empresas, y proponemos posibles vías de solución.