solar wind in the Oxford-Paravia Italian Dictionary

Translations for solar wind in the English»Italian Dictionary

Translations for solar wind in the English»Italian Dictionary

solar [Brit ˈsəʊlə, Am ˈsoʊlər] ADJ

I.wind1 [Brit wɪnd, Am wɪnd] N

II.wind1 [Brit wɪnd, Am wɪnd] VB trans

I.wind2 [Brit wʌɪnd, Am waɪnd] N

II.wind2 <pt/pp wound> [Brit wʌɪnd, Am waɪnd] VB trans

III.wind2 <pt/pp wound> [Brit wʌɪnd, Am waɪnd] VB intr

solar wind in the PONS Dictionary

Translations for solar wind in the English»Italian Dictionary

I.wind2 <wound, wound> [waɪnd] VB trans

II.wind2 <wound, wound> [waɪnd] VB intr

Monolingual examples (not verified by PONS Editors)

English
On the night side, the dust is negatively charged by electrons in the solar wind.
en.wikipedia.org
More significantly, the optical surfaces of small bodies are subject to modification by intense radiation, solar wind and micrometeorites.
en.wikipedia.org
Interactions between energetic solar wind particles and cometary material evaporating from the nucleus is likely to contribute significantly to this effect.
en.wikipedia.org
The solar wind flows outward supersonically to great distances, filling a region known as the heliosphere, an enormous bubble-like volume surrounded by the interstellar medium.
en.wikipedia.org
This would produce a large and sustained eruption similar to a solar flare at the target location, feeding the solar wind.
en.wikipedia.org
For example, coronal holes allow fast-moving plasma to escape from the photosphere, which can effect a local increase in the solar wind speed.
en.wikipedia.org
The heliopause is the point at which pressure from the solar wind is equal to the opposing pressure of interstellar wind.
en.wikipedia.org
Figures here assume the spacecraft is traveling towards the sun (since the solar wind is directional), under the worst conditions for thrust.
en.wikipedia.org
Cluster monitors particles from the ionosphere and the solar wind as they pass through the magnetotail lobes.
en.wikipedia.org
A common erroneous belief is that the primary non-thermal escape mechanism is atmospheric stripping by a solar wind in the absence of a magnetosphere.
en.wikipedia.org

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