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Using the transit of Venus to probe the upper planetary atmosphere
During a planetary transit, atoms with high atomic number absorb short-wavelength radiation in the upper atmosphere, and the planet should appear larger during a primary transit observed in high-energy bands than in the optical band. Here we measure the radius of Venus with subpixel accuracy during...
में बचाया:
| में प्रकाशित: | Nat Commun |
|---|---|
| मुख्य लेखकों: | , , , , , |
| स्वरूप: | Artigo |
| भाषा: | Inglês |
| प्रकाशित: |
Nature Publishing Group
2015
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| विषय: | |
| ऑनलाइन पहुंच: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4557371/ https://ncbi.nlm.nih.gov/pubmed/26102562 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/ncomms8563 |
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