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Glossary term: 电磁辐射

Also known as Electromagnetic Waves

Description: 当19世纪的物理学家在描述电磁现象时发现,即使在附近没有电荷的情况下,电场和磁场也能以光速在空间传播。这些波被称为电磁波或电磁辐射。基本电磁波可根据其波长进行分类,由此产生的电磁波谱从较短波长到较长波长包括:伽马射线、X射线、紫外线、可见光、红外线、亚毫米波和射电波(包括毫米波/微波)。来自遥远天体的电磁辐射是天文学家了解这些天体的最重要的信息来源。

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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher
The translation of this term and its definition is still awaiting approval

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".

Related Diagrams


三条曲线,Y 轴为辐射,X 轴为波长。较冷的曲线峰值较红和较低

黑体辐射

Caption: 不同温度黑体的辐射曲线。x 轴表示波长,y 轴表示黑体表面每平方米在每个波长下每秒发射的能量。 温度越高的物体,波长越短,发出的最大能量光也越蓝。尽管图中最冷的天体发出的红光达到峰值,但其他较热的天体发出的红光都比最冷的天体多。
Credit: IAU OAE/Niall Deacon

License: CC-BY-4.0 Creative Commons 署名 4.0 国际 (CC BY 4.0) icons


三条曲线,Y 轴为辐射,X 轴为波长。较冷的曲线峰值较红和较低

黑体辐射--紫外线灾难

Caption: 不同温度黑体的辐射曲线。x 轴表示波长,y 轴表示黑体表面每平方米在每个波长下每秒发射的能量。 温度越高的物体,波长越短,发出的最大能量光也越蓝。尽管图中最冷的天体发出的红光达到峰值,但其他较热的天体发出的红光都比最冷的天体多。 虚线显示的是现代量子力学之前的经典理论所预测的辐射量。对于任何温度高于零的黑体,这一预测在较短波长处都趋于无穷大,被称为 "紫外线灾难"。
Credit: IAU OAE/Niall Deacon

License: CC-BY-4.0 Creative Commons 署名 4.0 国际 (CC BY 4.0) icons