<div class="figure-img" data-ke-type="image" data-ke-style="alignCenter" data-ke-mobilestyle="widthOrigin"><img src="https://t1.daumcdn.net/cafeattach/1ViNS/abbf80ff9fe4349bbf2a69106948cb741e64296a" class="txc-image" data-img-src="https://t1.daumcdn.net/cafeattach/1ViNS/abbf80ff9fe4349bbf2a69106948cb741e64296a" data-orgin-width="900" data-origin-height="600"></div><p style="text-align: center;"> </p><p style="text-align: center;"><b><span style="font-family: 'Noto Serif KR';" data-ke-size="size20">#태양광기사 #태양광뉴스 #태양광발전사업 #태양광에너지 #태양광모듈 #태양광인버터</span></b></p><p style="text-align: center;"> </p><p style="text-align: center;"><span style="color: #ee2323;"><b><span style="font-family: 'Noto Serif KR';" data-ke-size="size20">태양궤도 탐사선 솔라 오비터에 적용된 PI 팁 틸트 미러</span></b></span></p><p style="text-align: center;"> </p><p style="text-align: center;"><b><span style="font-family: 'Noto Serif KR';" data-ke-size="size20"><a href="http://www.solartodaymag.com/news/articleView.html?idxno=10119" target="_top" class="ke-link">http://www.solartodaymag.com/news/articleView.html?idxno=10119</a> </span></b></p><div class="figure-open" contenteditable="false" data-ke-type="opengraph" data-ke-align="alignCenter" data-og-type="website" data-og-title="태양궤도 탐사선 ‘솔라 오비터’에 적용된 PI 팁/틸트 미러" data-og-description="ESA와 NASA는 지난 2월 태양풍 형성 및 폭발 과정 등을 연구하기 위해 태양궤도 탐사선인 ‘솔라 오비터(Solar Orbiter)’를 발사했다. 여기에는 ‘PHI(Polarimetric and Helioseismic Imager)’의 보조 반사경(부��" data-og-host="www.solartodaymag.com" data-og-source-url="http://www.solartodaymag.com/news/articleView.html?idxno=10119" data-og-url="http://www.solartodaymag.com/news/articleView.html?idxno=10119" data-og-image="https://scrap.kakaocdn.net/dn/MzaoT/hyHyTkKMgd/iFcDguhV6fCHRRDYVr2pk0/img.jpg?width=600&height=424&face=0_0_600_424,https://scrap.kakaocdn.net/dn/b6MenG/hyHAI2XWVc/181JrKrHthgXMuM3h8j7F0/img.jpg?width=600&height=638&face=0_0_600_638,https://scrap.kakaocdn.net/dn/bwAnct/hyHy0KVjjd/hycSajK7dC8CKeJARRMhDK/img.jpg?width=600&height=424&face=0_0_600_424"><a href="http://www.solartodaymag.com/news/articleView.html?idxno=10119" target="_blank" data-source-url="http://www.solartodaymag.com/news/articleView.html?idxno=10119"><div class="og-image" style="background-image:url(https://scrap.kakaocdn.net/dn/MzaoT/hyHyTkKMgd/iFcDguhV6fCHRRDYVr2pk0/img.jpg?width=600&height=424&face=0_0_600_424,https://scrap.kakaocdn.net/dn/b6MenG/hyHAI2XWVc/181JrKrHthgXMuM3h8j7F0/img.jpg?width=600&height=638&face=0_0_600_638,https://scrap.kakaocdn.net/dn/bwAnct/hyHy0KVjjd/hycSajK7dC8CKeJARRMhDK/img.jpg?width=600&height=424&face=0_0_600_424)"></div><div class="og-text"><p class="og-title">태양궤도 탐사선 ‘솔라 오비터’에 적용된 PI 팁/틸트 미러</p><p class="og-desc">ESA와 NASA는 지난 2월 태양풍 형성 및 폭발 과정 등을 연구하기 위해 태양궤도 탐사선인 ‘솔라 오비터(Solar Orbiter)’를 발사했다. 여기에는 ‘PHI(Polarimetric and Helioseismic Imager)’의 보조 반사경(부��</p><p class="og-host">www.solartodaymag.com</p></div></a></div><p> </p>
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