Remote Sensing of Sun-Earth Climate

The proposed monograph on "Remote sensing of Sun-Earth Climate" is a new concept being established by the author after a passionate research in this field for more than two decades.

Main objective of the monograph is to initiate the use of extra terrestrial remote sensing applications to understand the Environment of the Earth and other planets of the solar system. Environmental changes of the Earth and Atmosphere are being studied based on the interaction of different anthropogenic activities and its effects. The influence of Sun and other celestial objects on the Earth and other planets has been observed by using the Solar and Heliospheric Observatory (SOHO) satellite which is placed in between Sun and Earth. Unlike other satellites, SOHO does not rotate around Earth but it rotates around the Sun and it is 1.5 million kilometers away from the Earth. From Sun, the Sunspot erupts through the corona of the Sunspots as well as intermittent solar flare. These variables are measured as Electron flux (E-flux), Proton flux (P-flux), X-ray flux and Planetary indices (Kp). These variables show erratic behavior which is showing pro- and anti- correlation with various environmental changes in space and time. The monograph includes not only the information pertaining with the changes on the Earth but it concerns about the changes in other planets and their Moons also. The information inferred from different Environment other than the Earth may be useful for calibrating the Environmental Changes within the Earth and its comparison with the Environment of other planets and satellites in the Solar system. The monograph will emphasize not only on the Earth and Planetary Sciences fields but it will improve the knowledge on the influence of distantly placed celestial objects including Sun and Star.

The proposed monograph is based on the hypothesis of extra terrestrial changes to initiate the climate change on the Earth. During these extra terrestrial changes it has been observed that the earth changes in its atmosphere as well as geosphere, which may have local effect but the increase of these local effects in large scale may contribute to the climate change. Solar radiation drives atmospheric circulation. Since solar radiation represents almost all the energy available to the Earth, accounting for solar radiation and how it interacts with the atmosphere and the Earth's surface is fundamental to understanding the Earth's energy budget. Similar to the Earth it has been found to be relevant with other planets of the Solar system which also show remarkable changes during the varied influences by the Sun and other materials from the outer space.Most of the statistical scientific data were not able to answer satisfactorily the erratic behavior of climate. Earth is a tiny part of the Universe and it is linked with the changes of Sun and other celestial bodies. We are continuously facing the changes in the climate due to changes in the sun and in the intensity of cosmic rays and other collateral changes imposed on the Earth. It has been observed that these changes are taking place before any episodic changes on the Earth. An attempt is made here to simulate the climate change based on the abrupt changes in the atmosphere and geosphere of the earth during solar eclipse.

提議的專書「遙感太陽-地球氣候」是作者在這個領域進行了二十多年的熱情研究後建立的一個新概念。

專書的主要目標是啟動利用外太空遙感應用來了解地球環境和太陽系其他行星的使用。基於不同人為活動的相互作用及其影響，正在研究地球和大氣環境的變化。通過使用太陽和其他天體對地球和其他行星的影響，已經觀察到了太陽和日地觀測衛星（SOHO）的存在。SOHO衛星不像其他衛星一樣繞地球旋轉，而是繞太陽旋轉，距離地球150萬公里。從太陽，太陽黑子通過太陽黑子的日冕以及間歇性的太陽耀斑爆發。這些變量被測量為電子通量（E-flux）、質子通量（P-flux）、X射線通量和行星指數（Kp）。這些變量表現出不規則的行為，與時空中的各種環境變化呈現正相關和負相關。專書不僅包括地球上的變化信息，還涉及其他行星和其衛星的變化。從地球以外的不同環境中推斷出的信息可能有助於校準地球內的環境變化，並將其與太陽系中其他行星和衛星的環境進行比較。專書將不僅強調地球和行星科學領域，還將提高對遙遠的天體（包括太陽和恆星）影響的認識。

提議的專書基於外太空變化的假設，以啟動地球上的氣候變化。在這些外太空變化中，觀察到地球在大氣層和地球圈層中發生變化，這可能具有局部影響，但這些局部影響在大尺度上的增加可能導致氣候變化。太陽輻射驅動大氣循環。由於太陽輻射代表了地球可利用的幾乎所有能量，計算太陽輻射以及它如何與大氣和地球表面相互作用是理解地球能量平衡的基礎。與地球類似，太陽系的其他行星也顯示出在太陽和外太空物質的不同影響下發生了顯著變化。大多數統計科學數據無法令人滿意地解釋氣候的不規則行為。地球是宇宙的一小部分，與太陽和其他天體的變化相關。由於太陽和宇宙射線強度的變化以及對地球施加的其他相關變化，我們不斷面臨氣候變化。觀察到這些變化發生在地球上的任何突發變化之前。在這裡，我們嘗試基於太陽食和地球大氣層和地球圈層的突然變化來模擬氣候變化。