Martian Ionosphere-Thermosphere Coupling in Longitude Structures: Statistical Results for the Main Ionization Peak Height

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2024-11-02 DOI:10.1029/2024JA032839
Yiding Chen, Libo Liu, Huijun Le, Ruilong Zhang
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Abstract

The Martian ionosphere-thermosphere (I-T) coupling is variable due to complex variations of the driving factors such as atmospheric tides and crustal magnetic fields. In this study, variability of the I-T coupling in longitude structures was investigated using a series of data segments of the MGS ionospheric measurements. Measurements in each data segment can cover different longitudes, and the solar forcing and local solar time just change a little. Ionospheric and thermospheric longitude variations are statistically correlated. Ionospheric peak electron density (NmM2) decreases while ionospheric main peak height (hmM2) increases with increasing neutral scale height (Hn) along longitudes. These correlated longitude variations are consistent with the photochemical coupling that Hn longitude disturbances induce ionospheric longitude structure through photochemical processes. Statistically, NmM2 is a better indicator than hmM2 for the Hn disturbances in the lower thermosphere. Hn longitude variation intensity is a crucial factor affecting the photochemical I-T coupling in longitude structures; it is closely related to NmM2 longitude variation intensity and tends to decline with increasing altitudes. The I-T coupling in longitude structures tends to decline near the terminator, which is in line with the declining longitude variation of Hn with increasing altitudes since hmM2 significantly increases near the terminator. Moreover, it tends to enhance at high solar activity level due to increased photoionization rate. The I-T coupling in longitude structures also shows seasonal dependence, as seasonal variation of hmM2 can affect the Hn longitude variation intensity nearby the ionospheric main peak.

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经度结构中的火星电离层-热层耦合:主电离峰高的统计结果
由于大气潮汐和地壳磁场等驱动因素的复杂变化,火星电离层-热层(I-T)耦合是可变的。在这项研究中,利用 MGS 电离层测量的一系列数据段研究了经度结构中 I-T 耦合的可变性。每个数据段的测量可以覆盖不同的经度,太阳强迫和当地太阳时只是略有变化。电离层和热层的经度变化在统计学上是相关的。电离层峰值电子密度(NmM2)随着中性尺度高度(Hn)沿经度的增加而降低,而电离层主峰高度(hmM2)则随着中性尺度高度(Hn)的增加而增加。这些相关的经度变化与 Hn 经度扰动通过光化学过程诱发电离层经度结构的光化学耦合相一致。从统计学角度看,NmM2 比 hmM2 更能反映低温层的 Hn 扰动。Hn经度变化强度是影响经度结构中光化学I-T耦合的一个关键因素;它与NmM2经度变化强度密切相关,并且随着高度的增加呈下降趋势。由于 hmM2 在终结点附近显著增加,因此经度结构中的 I-T 耦合在终结点附近呈下降趋势,这与 Hn 的经度变化随海拔升高而下降的趋势是一致的。此外,在太阳活动水平较高时,由于光离子化率的增加,I-T 耦合也有增强的趋势。经度结构中的 I-T 耦合也显示出季节依赖性,因为 hmM2 的季节变化会影响电离层主峰附近的 Hn 经度变化强度。
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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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