利用地面数据和 COSMIC 卫星数据研究北半球热带和亚热带对流层低层温度(TLST)的长期趋势

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2024-07-14 DOI:10.1016/j.jastp.2024.106306
Tsehaye Negash , U. Prakash Raju
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引用次数: 0

摘要

对流层是大气层中最低和最接近的一层,是所有气象事件发生的地方。对流层-低平流层(TLS)温度趋势是通过线性回归确定的,对于理解未来气候变化的后果至关重要。在这篇文章中,我们利用 2006-2020 年期间在热带站点 Addis(北纬 90°,东经 38°,南纬 80°)和亚热带站点 Addis(北纬 90°,东经 38°,南纬 80°)上的 COSMIC 卫星和地面无线电探空仪(RS)的月平均带状平均观测数据,探讨了对流层-下平流层(1-25 公里)温度的长期变化和趋势,以及厄尔尼诺南方涛动(ENSO)、太阳通量(SF)、准半年度涛动(QBO)、印度洋偶极子(IOD)和气溶胶指数(AI)等自然驱动因素对其的响应。80 E)和亚热带站点开罗(北纬 30.030,东经 31.230)。热带站点 Addis 的对流层顶位于 17 公里处,温度为 190-194 K,而亚热带站点开罗的对流层顶位于 15 公里处,温度为 201 K。利用小波分析技术可以看到 TLS 区域的两大振荡:半年度振荡(SAO)和年度振荡(AO),其中对流层下部的 AO 尤为强烈。此外,对流层顶冷点温度 CPTt 的莫雷特小波分析显示了 AO,对流层顶冷点高度 CPTh 显示了类似 QBO 的信号。受厄尔尼诺/南方涛动、SF、QBO、IOD 和气溶胶等自然驱动因素的影响,对流层顶温度区域在亚的斯亚贝巴站的 7、21、22、13 和 4 千米高度以及开罗站的 15、19、25、15 和 16 千米高度出现了正峰值。滞后分析表明,除海洋指数和 SSF 外,所有自然影响因子在对流层顶以下(15 公里以下)都会出现一个月的延迟。对流层顶以上的每次振荡都有 3 到 4 个月的明显滞后。通过 MLR 趋势分析,对流层区域呈现变暖趋势,UTLS 区域呈现冷却趋势。亚热带的开罗站在 2 千米处的升温速率最高,为 0.38 千帕/十年,在 10 千米处的降温速率最高,为-0.2 千帕/十年;而热带的阿迪斯站在 12 千米处的降温速率最高,为-0.38 千帕/十年,在 3 千米处的升温速率最高,为 0.28 千帕/十年。我们的趋势研究结果与之前的研究结果一致。
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Study on long term troposphere lower stratosphere temperature (TLST) trend in tropical and subtropical northern hemisphere using ground based and COSMIC satellite data

The troposphere, the lowest and closest layer of the atmosphere, is where all meteorological events take place. The tropospheric — lower stratospheric (TLS) temperature trend is determined using linear regression and is essential to comprehending the consequences of climate change in the future. In this article, we explored the long-term temperature variabilities and trends of TLS (1–25 km) temperature and its responses by natural drivers such as El Nino southern oscillation (ENSO), solar flux (SF), quasi-biannual oscillation (QBO), Indian ocean dipole (IOD), and aerosol indexes (AI) using monthly averaged zonal mean COSMIC satellite and ground — based Radiosonde (RS) observations for the period of 2006 – 2020 over tropical station Addis (90 N, 38.80 E) and subtropical station Cairo (30.030 N, 31.230 E). The tropopause is located at the tropical station Addis at 17 km with a temperature of 190–194 K, and for the subtropical station Cairo, it is located at 15 km with a temperature of 201 K, which supports the decrement of tropopause height from the tropics to the subtropics with a slight increase in temperature. The two main oscillations in the TLS region can be seen by using the wavelet analysis technique: the semiannual oscillation (SAO) and the annual oscillation (AO), with the AO being especially strong in the lower troposphere. Furthermore, Morlet wavelet analysis on cold-point tropopause temperature CPTt displays AO and cold point tropopause height CPTh reveals a QBO-like signal. The TLS region has positive peaks at heights of 7, 21, 22, 13, and 4 km for the Addis station, and at 15, 19, 25, 15, and 16 km for the Cairo station in response to natural drivers such as ENSO, SF, QBO, IOD, and aerosol. Lag analyses demonstrate a one-month delay for all natural forcings, except for oceanic indices and SSF, up to three months below the tropopause (below 15 km). There is a noticeable 3 to 4 months lag in every oscillation above the tropopause. A warming trend in the tropospheric region and a cooling trend in the UTLS regions are revealed by MLR trend analysis. In contrast to the subtropical Cairo station, which has the highest warming rate of 0.38 K/decade at 2 km and the maximum cooling rate of −0.2 K/decade at 10 km, the tropical Addis station has the highest cooling rate of −0.38 K/decade at 12 km and the highest warming rate of 0.28 K/decade at 3 km. Our trend findings are consistent with previous research.

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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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