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Saturn suprathermal O_2 ~+ and mass-28~+ molecular ions: Long-term seasonal and solar variation

机译:土星suprathermal成分~ +和mass-28 ~ +分子离子:长期季节性变化和太阳能

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Suprathermal singly charged molecular ions, O_2 ~+ (at ~32 Da/e) and the Mass-28 ion group ~(28)M~+ (ions at ~28 Da/e, with possible contributions from C_2H_5 ~+, HCNH~+, N_2 ~+, and/or CO ~+), are present throughout Saturn's ~4-20 Rs (1 Saturn radius, Rs = 60,268 km) near-equatorial magnetosphere from mid-2004 until mid-2012. These ~83-167 keV/e heavy ions measured by Cassini's CHarge-Energy-Mass Spectrometer have long-term temporal profiles that differ from each other and differ relative to the dominant water group ions, W~+ (O~+, OH~+, H_2O~+, and H_3O~+). O_2 ~+/W~+, initially ~0.05, declined steadily until equinox in mid-2009 by a factor of ~6, and ~(28)M ~+/W~+, initially ~0.007, declined similarly until early-2007 by a factor of ~2. The O_2 ~+/W~+ decline is consistent with Cassini's in situ ring-ionosphere thermal ion measurements, and with proposed and modeled seasonal photolysis of Saturn's rings for thermal O_2 and O_2 ~+. The water ice-dominated main rings and Enceladus plume depositions thereon are the two most likely O_2 ~+ sources. Enceladus' dynamic plumes, though, have no known long-term dependence. After declining, O_2 ~+/W~+ and ~(28)M~+/W~+ levels remained low until late-2011 when O_2 ~+/W~+ increased, but ~(28)M~+/W~+ did not. The O _2 ~+/W~+ increase was steady and became statistically significant by mid-2012, indicating a clear increase after a decline, that is, a possibly delayed O_2 ~+ "seasonal" recovery. Ring insolation is driven by solar UV flux which itself varies with the sun's 11 year activity cycle. The O_2 ~+/W~+ and ~(28)M~+/W~+ declines are consistent with seasonal ring insolation. No O_2 ~+/W~+ response to the late-2008 solar-cycle UV minimum and recovery is evident. However, the O_2 ~+/W~+ recovery from the postequinox baseline levels in late-2011 coincided with a strong solar UV enhancement. We suggest a scenario/framework in which the O _2 ~+ observations can be understood. Key Points Energized Saturn ring ionosphere O2+ ions show seasonal and solar variation. The long-term O2+/W+ variation is not as anticipated after equinox. Energized local-origin Mass-28 ions initially show likely seasonal variation.
机译:单独Suprathermal带电分子离子,提取成分~ +(~ 32 Da / e)和Mass-28 ~ (28) M ~ +离子组(离子~ 28 Da / e,与可能的贡献在土星的存在~ 4 Rs (1近赤道半径,土星Rs = 60268公里)磁气圈从2004年中期到2012年中期。~ 83 - 167 keV / e重离子由卡西尼号的CHarge-Energy-Mass光谱仪有长期时间配置文件不同于彼此,相对于占主导地位的不同水离子,W (O ~ +,哦~,H_2O ~ +和H_3O ~ +)。最初~ 0.05,直到equinox稳步下降2009年中期~ 6倍,和~ (28)M ~ + / W ~ +,最初~ 0.007,拒绝同样直到初- 2007 ~ 2倍。减少与卡西尼的原位是一致的ring-ionosphere热离子测量,提出和建模季节性的光解土星环热提取成分和成分~ +。水大部分被冰覆盖的主要环和恩克拉多斯羽口供上是两个最有可能提取成分~ +来源。不过,没有已知的长期依赖。下降,提取成分~ + / W ~ +和~ (28)M ~ + / W ~ +的水平保持低直到2011年提取成分~ + / W ~ +增加,但~ (28)M ~ + / W ~ +没有。~ + / W ~ +增长稳定,成为在2012年年中具有统计学意义,表明明显增加后下降,可能推迟提取成分~ +“季节性”复苏。日晒是由太阳能紫外线通量本身随太阳活动11年周期。符合季节性环日晒。提取成分~ + / W ~ +反应后期- 2008太阳周期紫外线最小和恢复是很明显的。提取成分~ + / W ~ +康复postequinox基线水平- 2011年末之际,一个强大的太阳能紫外线增强。O _2 ~ +的观察理解。电离层O2 +离子显示季节性和太阳能变异。春分后如预期般。本地Mass-28离子最初显示的可能性季节性变化。

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