全國中小學科展

地球科學

台灣的黯化現象與形成因素探討

本研究在探討台灣的黯化現象與形成因素,黯化現象為太陽輻射量到達地表的減少現象。我們藉由比較西元1961~ 2008年間,台北、台中、台南、大武、蘭嶼、花蓮六個測站的各項氣象因子進行分析處理並探討其變化情形與成因。 \r 研究結果顯示,台灣地區的都市測站(台北、台中、台南)日照時數、日照率、全天空輻射量均呈現先下降後上升的趨勢,顯示1961至2000年間確實存在黯化現象,而在鄉村測站(大武、蘭嶼)則有微幅改變但較不顯著。並藉由可能影響黯化現象各氣象因子的比對,發現最高溫的增加幅度遠小於最低溫,可能表示黯化現象部分削弱了暖化現象。另外,溫度均較差也逐年縮小,亦可以當成黯化現象的一個顯著的指摽。在造成黯化現象成因中,污染物和雲量最為明顯。在有雲量的影響下,台灣地區汙染物濃度對黯化現象的影響程度,依序為硝酸鹽類>PM10>二氧化硫,此外少量污染物也會使雲量大幅增加,故兩者對黯化現象會產生交互影響。由雲量改變量對應日照時數改變量/雲量改變量的分析圖中,可看出都市地區年平均雲量改變量大於15%時,其雲量每減少10%,日照時數約減少3~22%;若年平均雲量改變量小於15%時,則對黯化現象不具統計意義。取每年十月中雲量在1以下的天數來分析各污染物對全天空輻射量影響,可發現雲量極低時,單位污染物濃度對黯化現象影響,SO2最大,NOx次之,PM10最小。

The garnets of the schlich of the winter coast (the White Sea)

During an expedition to the White Sea Winter Coast, samples of schlich with numerous garnets were collected. The coast itself is primarily a set of high steeps of sandstones and mudstones with no garnets. On the beach, however, there are numerous pebbles of metamorphic rocks, and many of them contain garnets. They were brought there by the Quaternary glacier and the present day glacier activity. Their source could be the existing or fully eroded metamorphic rocks of the Kola Penninsila and Northern Karelia.\r Goal of the research: To discover the possible origin of the garnets.\r Tasks: 1) To analyze the structure and the chemical composition of the garnets. 2) To study the works on the garnets of the Kola Penninsila and Northern Karelia in order to compare the information to the results of the analysis.\r Methods: 1) Granulometric analysis; 2) Magnetic and electromagnetic separation; 3) Microscope study of the garnets; 4) X-ray diffraction analysis; 5) X-ray fluorescence analysis. \r RESULTS\r 1. The sample garnets could be divided into two types: the bright red and the pale pink.\r 2. Both types are almandines with spessartine components. The pale-pink one contains Arizona ruby components, and the bright red contains andradite ones. \r 3. Only a few samples from Khangaz Varaki, Malye Keivy, and Tersky Coast are similar to the garnets that we collected. It is possible that the glacier brought them from the Kola Penninsula, but it is also possible that the rocks, where the glacier brought our garnets from, have been totally eroded.

鑽石石墨化及氧化速率之研究

Pleistocene mammals of a river basin of Adycha

The paper represents the results of study of remains of mammalians which inhabited the Adycha-River basin (Verkhoyansky Region) during the Pleistocene Epoch. All studied materials belong to the Museum of Paleontology and Ethnography of the Adychinskaya Secondary School. For a long time, People have been finding ancient animal bones on the Adycha-River banks, and since 1955, the teacher, Bozhedonov Nikolai Gerasimovich, has been organizing exploring local lore expeditions for school children purposed for mammoth fauna investigation and material collection for the school museum. In this research collected material was classified, measurements of the Pleistocene Period animal bones were made. On the basis of it we came to conclusion that during the Pleistocene Epoch, very rare species of animals inhabited the Adycha-River basin. To our opinion, the Adycha-River basin is a unique site for research activity. Comparative measurements of the Pleistocene Periods animal bones were made. Of flu work we know measurements of the Early and Middle Pleistocene Period elephant’s bones which inhabited the Adycha-River basin. Elephants inhabited with mammoth. To our opinion, they didn’t yield to size to mammoth. In that time the Adycha-River basin, was been inhabited by camelopard, bison and Soergelia.\r Museum has 2 skull’s fragments and ovibos fronts part of horny stream. Geological age which is Early Pleistocene or late Pleistocene. These bones concern to Praeovibos. Distance between horns is more 100 mm. If we compare with ovibos skull of the Late Pleistocene we see that distance between horns is longer for the 10 time. We couldn’t found such comparisons at scientist’s works. It results that the more distance between horns is longer the more ancient, and skull’s sizes are much less.\r 7-8 km lower of Betenkes, in disclosing “?????? ???????” and sand bank “??????”, was been founded 3 crag’s part of skull of Soergelia, metacarpal bone and 2 skull’s fragments with horns part. On the Adycha-River basin was bun founded above all quantity of soergelias remains.\r In the Pleistocene Period inhabited a lot of horses. Which remains he have now. Our horse’s height in crest is from 142 to 156 sm. And what about of horses of the Early Pleistocene, it is more than 230 sm.\r Molar teeth of the Early Pleistocene Epoch horse are more for the 2.5 times than of contemporaneous analog.

星星相映-以理論與觀測探究雙星形成機制

由於在銀河系中的多數恆星是以雙星系統存在,因此雙星的形成機制在恆星演化理論中扮演極重要的角色。但目前其形成的機制未有定論,而爭論的焦點主要為兩個假說:一個假說為當分子雲在裂解為雲核時,同一雲核會形成兩顆恆星互繞;另一假說為不同雲核會分別塌縮為不同的恆星。這份研究中,我們以金斯最小質量與半徑為理論依據,找尋上萬筆的觀測數據,並對其資料來源做觀測限制上的確認,進而分析雙星間距的分布,且以雙星的星團與光譜型為分類作圖。分析後的結果中,我們發現前主序雙星間距分布圖出現了一個小於金斯最小半徑的峰值,得出了分裂說必定存在,然無法排除捕獲說的存在;並且發現不同星團、光譜型對間距的關係有顯著的差別。

大屯火山群磁場分布測量與分析

近年來許多研究顯示台北的大屯山底下可能存在岩漿庫,而最近一次的噴發可能約在5000年前,於是我們決定利用地球物理方法對大屯山做更進一步的了解。由於磁力測勘是了解火成岩區的重要工具,而且前人對大屯山的磁力探勘似乎著墨較少,所以我們決定使用磁力對大屯山進行測勘。測區包含了公路以及步道的部分,量取資料後,我們經過一些標準的程序得到磁力異常值,再利用極化修正將資料修正得更直觀,並用修正前後的資料繪出的圖與溫泉露頭、地表岩性等做比對。最後我們利用物理方法得到相對的居里點深度,希望能進一步了解大屯火山群的地熱活動。我們研究後認為:大屯山下方的居禮點深度較深,地熱活動較不活躍,而七星山到大油坑間的居禮點深度較淺,地熱活動則較旺盛,可能有岩漿庫存在。

Microregion Belusske Vrata

宜蘭外海條狀雨帶成因探討

觀察逐時雷達迴波圖之後,我們發現冬末春初時節,從傍晚到凌晨這段時間,在宜蘭外海是一條狀雨帶的「好發期」,這條狀雨帶並非由鋒面或其他已知的天氣系統引起,故我們想研究這條狀雨帶強度與其氣候環境間的關係。前人的研究中,並沒有研究宜蘭外海的條狀雨帶,不過,從其他研究類似的條狀雨帶的參考資料中,我們發現大部分的研究認定條狀雨帶的成因,都是由風場輻合所引起,因此,我們想研究是否還有其他促使條狀雨帶形成的原因。先定義出條狀雨帶常出現的範圍,挑出有出現條狀雨帶的時數,並利用軟體Extract Color擷取每ㄧ張圖片中條狀雨帶的像素,藉此將範圍中的回波訊號量化。整理向中央氣象局收集來的氣象資料(風向、風速、氣溫、海溫),與回波訊號的量化數據做對照。結果我們發現,以風的輻合輻散來看,當風的輻合量愈大時,此雨帶也愈明顯;以溫差來看,海溫與氣溫的溫差愈大,此雨帶愈明顯。