
Le rayonnement thermique est une source décisive d’informations pour une science de l’observation comme l’astrophysique. Dominant dans l’infrarouge lointain, il est difficile à mesurer, et nécessite le développement de détecteurs innovants et de techniques cryogéniques de pointe. Mise en œuvre à bord de satellite depuis 40 ans, la mesure du rayonnement thermique a permis de nombreuses découvertes liées à la formation stellaire et à l’évolution des galaxies.
[SPI] Engineering Sciences [physics]
[SPI] Engineering Sciences [physics]
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| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
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