When emitted at the same time, solar hard X-rays reflected by the photosphere arrive at an observer at later times than primary hard X-rays coming directly from the source. This time lag of albedo photons, therefore, should be taken into account in interpreting fine-scale hard X-ray time profiles. I
Determination of noise source heights, part II: Measurement of the equivalent source height of highway vehicles
β Scribed by S.A.L. Glegg; J.R. Yoon
- Book ID
- 103251513
- Publisher
- Elsevier Science
- Year
- 1990
- Tongue
- English
- Weight
- 813 KB
- Volume
- 143
- Category
- Article
- ISSN
- 0022-460X
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