| Title |
In situ measurements of Saturn’s ionosphere show that it is dynamic and interacts with the rings
|
|---|---|
| Published in |
Science, December 2017
|
| DOI | 10.1126/science.aao4134 |
| Pubmed ID | |
| Authors | |
| Abstract |
The ionized upper layer of Saturn's atmosphere, its ionosphere, provides a closure of currents mediated by the magnetic field to other electrically charged regions (e.g., rings) and hosts ion - molecule chemistry. In 2017, the Cassini spacecraft passed inside the planet's rings, allowing in situ measurements of the ionosphere. The Radio and Plasma Wave Science (RPWS) instrument detected a cold, dense and dynamic ionosphere at Saturn that interacts with the rings. Plasma densities reached up to 1000 cm-3 and electron temperatures were below 1160 K near closest approach. The density varied between orbits by up to 2 orders of magnitude. Saturn's A- and B-rings cast a shadow on the planet that reduced ionization in the upper atmosphere, causing a North-South asymmetry. |
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X Demographics
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| Country | Count | As % |
|---|---|---|
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| Italy | 2 | 12% |
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Demographic breakdown
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| Scientists | 1 | 6% |
Mendeley demographics
Geographical breakdown
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|---|---|---|
| Unknown | 32 | 100% |
Demographic breakdown
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| Researcher | 6 | 19% |
| Professor | 2 | 6% |
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| Lecturer > Senior Lecturer | 1 | 3% |
| Other | 1 | 3% |
| Unknown | 9 | 28% |
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| Economics, Econometrics and Finance | 1 | 3% |
| Materials Science | 1 | 3% |
| Other | 1 | 3% |
| Unknown | 8 | 25% |