Absorption of methane in the Saturn's atmosphere near 2009 equinox

2013

Full text Open access: Gold Metadata (CSL-JSON)
DOI 10.18372/2411-6602.09.2176
Data confidence 70 medium
How this score is calculated

It is built from checkable properties of the record itself: whether the article has a DOI, how many independent sources confirmed its data, whether the required fields are filled in, and how recent the latest confirmation is. Disagreement between sources and a missing identifier lower it. A value of 80 or above means the record was published without further checking; 60 to 79 means it is published at reduced confidence, with a manual check advisable. A record verified by an editor by hand is never pushed below 90 by a recalculation. This scores our data about the article, not the article itself.

Abstract

The latitudinal variations of intensity of the absorption bands of methane on Saturn before and after the equinox in 2009 are considered, when the tilt of the planet's equator to the direction to the Sun was close to zero and both hemispheres were in equal insolation. The basic global changes of meridional distribution of absorption in the weak and moderate bands of methane in the wavelength range of 580-800 nm are extracted. The most characteristic feature of Saturn – a reduced absorption of methane in the equatorial belt – retains.