从十年JAXA和NASA日出天文台的亮点

国外航天 · 2016-10-20 10:46:00

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<p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="background: none; box-sizing: border-box;" data-dst="自推出以来，月22日，2006，日出，日本宇宙航空研究开发机构（JAXA）的联合任务，NASA一直看着太阳几乎不停，提供宝贵的洞察我们的明星–等人在整个宇宙。" data-src="Since its launch on Sept. 22, 2006, Hinode, a joint mission of the Japan Aerospace Exploration Agency (JAXA) and NASA, has been watching the sun nearly non-stop, providing valuable insight into our star – and others throughout the universe.">自推出以来，月22日，2006，日出，日本宇宙航空研究开发机构（JAXA）的联合任务，NASA一直看着太阳几乎不停，提供宝贵的洞察我们的明星–等人在整个宇宙。</trans></p><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"></p><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="background: none; box-sizing: border-box;" data-dst="“太阳是可怕的和华丽的，也是太阳系中最好的物理实验室，”Sabrina Savage说，在美国宇航局在亨茨维尔的马歇尔太空飞行中心的Hinode项目科学家，亚拉巴马州。“在过去的10年中，Hinode一直专注于了解我们的太阳是一个变量。”" data-src="“The sun is terrifying and gorgeous, and it’s also the best physics laboratory in our solar system,” said Sabrina Savage, project scientist for Hinode at NASA\'s Marshall Space Flight Center in Huntsville, Alabama. “In the past 10 years, Hinode has focused on understanding our sun as a variable star.”">“太阳是可怕的和华丽的，也是太阳系中最好的物理实验室，”Sabrina Savage说，在美国宇航局在亨茨维尔的马歇尔太空飞行中心的Hinode项目科学家，亚拉巴马州。“在过去的10年中，Hinode一直专注于了解我们的太阳是一个变量。”</trans></p><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"></p><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="background: none; box-sizing: border-box;" data-dst="Hinode已经被从太阳爆炸太阳能骨针的微妙运动的一切，让科学家们研究了这些现象。作为Hinode的大部分仪器仍处于良好的工作秩序，Hinode背后的团队希望更加深入到离我们最近的恒星。" data-src="Hinode has captured everything from solar explosions to the delicate motion of solar spicules, allowing scientists to study these phenomena in great detail. As most of Hinode’s instruments are still in good working order, the team behind Hinode hopes to delve even deeper into our nearest star.">Hinode已经被从太阳爆炸太阳能骨针的微妙运动的一切，让科学家们研究了这些现象。作为Hinode的大部分仪器仍处于良好的工作秩序，Hinode背后的团队希望更加深入到离我们最近的恒星。</trans></p><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"></p><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="background: none; box-sizing: border-box;" data-dst="“我们最近调整任务操作了几天的单目标跟踪，而不是跳跃在活跃的地区，”萨维奇说。“这种新的模式将使我们能够得到更为完整的活性区域进化的图片。”" data-src="“We recently adjusted mission operations to track a single target for several days, instead of jumping around among active regions,” said Savage. “This new paradigm will allow us to get a more complete picture of active region evolution.”">“我们最近调整任务操作了几天的单目标跟踪，而不是跳跃在活跃的地区，”萨维奇说。“这种新的模式将使我们能够得到更为完整的活性区域进化的图片。”</trans></p><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"></p><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="background: none; box-sizing: border-box;" data-dst="为了庆祝Hinode的第一个10年的轨道，这是从Hinode的科学成就，在过去的十年中10大亮点。" data-src="To celebrate Hinode’s first 10 years in orbit, here are 10 highlights from Hinode’s scientific accomplishments of the past decade.">为了庆祝Hinode的第一个10年的轨道，这是从Hinode的科学成就，在过去的十年中10大亮点。</trans></p><div class="dnd-atom-wrapper type-image context-full_width" style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px auto 2em; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; clear: both; word-spacing: 0px; display: table; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><div class="dnd-drop-wrapper" style="box-sizing: border-box;"><p><a href="data/attachment/portal/201610/20/110227p7wcvzw7ckqcncvy.jpg" target="_blank">

</a></p></div><div class="dnd-legend-wrapper" style="font-size: 11px; box-sizing: border-box;"><div class="caption" style="box-sizing: border-box;"></div><div class="credits" style="font-style: italic; font-weight: 700; box-sizing: border-box;"><trans style="box-sizing: border-box;" data-dst="学分：美国宇航局/日本宇宙航空研究开发机构（Hinode" data-src="Credits: JAXA/NASA/Hinode">学分：美国宇航局/日本宇宙航空研究开发机构（Hinode</trans></div><div class="link" style="background: inherit; padding: 0px; box-sizing: border-box;"><a style="background: 0px 0px; color: rgb(66, 139, 202); box-sizing: border-box;" href="http://www.nasa.gov/feature/goddard/2016/highlights-from-a-decade-of-jaxa-and-nasa-s-hinode-solar-observatory"></a></div></div></div><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="box-sizing: border-box;" data-dst="这张金星是2012年6月5日的金星凌日期间，由日出的太阳光学望远镜。在这张图片中，金星刚刚开始它的旅程，穿过太阳表面。它的大气层是可见的薄的、发光的边境上的左上角。科学家使用的图像从金星凌日，Hinode和其他太阳观测卫星，研究金星的大气层。" data-src="This image of Venus was taken during the Venus transit of June 5, 2012, by Hinode’s Solar Optical Telescope. In this image, Venus is just beginning its journey across the face of the sun. Its atmosphere is visible as a thin, glowing border on the upper left of the planet. Scientists used images from the Venus transit, taken by Hinode and other sun-watching satellites, to study the atmosphere of Venus.">这张金星是2012年6月5日的金星凌日期间，由日出的太阳光学望远镜。在这张图片中，金星刚刚开始它的旅程，穿过太阳表面。它的大气层是可见的薄的、发光的边境上的左上角。科学家使用的图像从金星凌日，Hinode和其他太阳观测卫星，研究金星的大气层。</trans></p><hr style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; height: 0px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; margin-top: 20px; margin-bottom: 20px; word-spacing: 0px; border-top-color: rgb(238, 238, 238); border-right-width: 0px; border-bottom-width: 0px; border-left-width: 0px; border-top-style: solid; white-space: normal; box-sizing: content-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><div class="dnd-atom-wrapper type-image context-full_width" style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px auto 2em; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; clear: both; word-spacing: 0px; display: table; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><div class="dnd-drop-wrapper" style="box-sizing: border-box;"><p><a href="data/attachment/portal/201610/20/110310rcj5c060h68rjk2s.gif" target="_blank">

</a></p></div><div class="dnd-legend-wrapper" style="font-size: 11px; box-sizing: border-box;"><div class="caption" style="box-sizing: border-box;"></div><div class="credits" style="font-style: italic; font-weight: 700; box-sizing: border-box;"><trans style="box-sizing: border-box;" data-dst="美国宇航局/日本宇宙航空研究开发机构/学分：日出" data-src="Credits: NASA/JAXA/Hinode">美国宇航局/日本宇宙航空研究开发机构/学分：日出</trans></div><div class="link" style="background: inherit; padding: 0px; box-sizing: border-box;"><a style="background: 0px 0px; color: rgb(66, 139, 202); box-sizing: border-box;" href="http://www.nasa.gov/feature/goddard/2016/highlights-from-a-decade-of-jaxa-and-nasa-s-hinode-solar-observatory"></a></div></div></div><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="box-sizing: border-box;" data-dst="这些图像的月亮比太阳在2012年5月12日，与同时环食从美国西部和南洋的部分可见吻合。日环食发生时，月亮在太阳前面直接在其轨道上某一点，当它离地球比较远。这额外的距离使月亮看起来比天空中的太阳，所以它不会阻止太阳的整个脸，而留下一个薄的发光带–通常被称为一个火环–在它的边缘。" data-src="These images of the moon eclipsing the sun on May 12, 2012, coincided with a simultaneous annular eclipse visible from parts of the western United States and Southeast Asia. An annular eclipse happens when the moon passes directly in front of the sun at a point in its orbit when it is relatively far from Earth. This extra distance makes the moon appear smaller than the sun in the sky, so it doesn’t block the entire face of the sun, instead leaving a thin glowing band – often known as a ring of fire – around its edge.">这些图像的月亮比太阳在2012年5月12日，与同时环食从美国西部和南洋的部分可见吻合。日环食发生时，月亮在太阳前面直接在其轨道上某一点，当它离地球比较远。这额外的距离使月亮看起来比天空中的太阳，所以它不会阻止太阳的整个脸，而留下一个薄的发光带–通常被称为一个火环–在它的边缘。</trans></p><hr style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; height: 0px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; margin-top: 20px; margin-bottom: 20px; word-spacing: 0px; border-top-color: rgb(238, 238, 238); border-right-width: 0px; border-bottom-width: 0px; border-left-width: 0px; border-top-style: solid; white-space: normal; box-sizing: content-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><div class="dnd-atom-wrapper type-image context-full_width" style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px auto 2em; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; clear: both; word-spacing: 0px; display: table; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><div class="dnd-drop-wrapper" style="box-sizing: border-box;"><a style="background: 0px 0px; color: rgb(66, 139, 202); text-decoration: none; box-sizing: border-box;" href="http://www.nasa.gov/sites/default/files/thumbnails/image/hinode-chromosphere-layers-sun.png">

</a></div><div class="dnd-legend-wrapper" style="font-size: 11px; box-sizing: border-box;"><div class="caption" style="box-sizing: border-box;"></div><div class="credits" style="font-style: italic; font-weight: 700; box-sizing: border-box;"><trans style="box-sizing: border-box;" data-dst="美国宇航局/日本宇宙航空研究开发机构/学分：日出" data-src="Credits: NASA/JAXA/Hinode">美国宇航局/日本宇宙航空研究开发机构/学分：日出</trans></div><div class="link" style="background: inherit; padding: 0px; box-sizing: border-box;"><a style="background: 0px 0px; color: rgb(66, 139, 202); box-sizing: border-box;" href="http://www.nasa.gov/feature/goddard/2016/highlights-from-a-decade-of-jaxa-and-nasa-s-hinode-solar-observatory"></a></div></div></div><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="box-sizing: border-box;" data-dst="日出的太阳光学望远镜拍摄到太阳的色球–薄薄一层之间的太阳的表面和大气–2007年1月12日。这个图像展示了太阳能材料的纤维结构，是被太阳的复杂和不断变化的磁场力拉伸。" data-src="Hinode’s Solar Optical Telescope imaged the sun’s chromosphere – a thin layer between the sun’s surface and atmosphere – on Jan. 12, 2007. This image showcases the filament structure of solar material that is pulled and stretched by the sun’s complex and ever-changing magnetic forces."> </trans><a href="data/attachment/portal/201610/20/110315on5nhn3450ejyc9u.png" target="_blank" style="font-family: Tahoma, Arial, Helvetica, snas-serif; line-height: 1.8em;">

</a></p><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="box-sizing: border-box;" data-dst="日出的太阳光学望远镜拍摄到太阳的色球–薄薄一层之间的太阳的表面和大气–2007年1月12日。这个图像展示了太阳能材料的纤维结构，是被太阳的复杂和不断变化的磁场力拉伸。" data-src="Hinode’s Solar Optical Telescope imaged the sun’s chromosphere – a thin layer between the sun’s surface and atmosphere – on Jan. 12, 2007. This image showcases the filament structure of solar material that is pulled and stretched by the sun’s complex and ever-changing magnetic forces.">出的太阳光学望远镜拍摄到太阳的色球–薄薄一层之间的太阳的表面和大气–2007年1月12日。这个图像展示了太阳能材料的纤维结构，是被太阳的复杂和不断变化的磁场力拉伸。</trans></p><hr style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; height: 0px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; margin-top: 20px; margin-bottom: 20px; word-spacing: 0px; border-top-color: rgb(238, 238, 238); border-right-width: 0px; border-bottom-width: 0px; border-left-width: 0px; border-top-style: solid; white-space: normal; box-sizing: content-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><div class="dnd-atom-wrapper type-image context-full_width" style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px auto 2em; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; clear: both; word-spacing: 0px; display: table; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><div class="dnd-drop-wrapper" style="box-sizing: border-box;"><p><a href="data/attachment/portal/201610/20/110348gmutxeeuk5kx8mpm.gif" target="_blank">

</a></p></div><div class="dnd-legend-wrapper" style="font-size: 11px; box-sizing: border-box;"><div class="caption" style="box-sizing: border-box;"></div><div class="credits" style="font-style: italic; font-weight: 700; box-sizing: border-box;"><trans style="box-sizing: border-box;" data-dst="美国宇航局/日本宇宙航空研究开发机构/学分：日出" data-src="Credits: NASA/JAXA/Hinode">美国宇航局/日本宇宙航空研究开发机构/学分：日出</trans></div><div class="link" style="background: inherit; padding: 0px; box-sizing: border-box;"><a style="background: 0px 0px; color: rgb(66, 139, 202); box-sizing: border-box;" href="http://www.nasa.gov/feature/goddard/2016/highlights-from-a-decade-of-jaxa-and-nasa-s-hinode-solar-observatory"></a></div></div></div><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="box-sizing: border-box;" data-dst="这段视频从日出的X射线望远镜是一个近两个月的意象，复合从2013年8月17日到2013年10月4日。中心附近的磁盘的亮点是活跃的地区，集中的磁场区域，很容易爆发像太阳耀斑和日冕物质抛射。这些图像被捕获在太阳的11年周期的最大活动阶段，其间活跃的地区主要集中在太阳赤道的一段。" data-src="This footage from Hinode’s X-ray Telescope is a composite of nearly two months of images, from Aug. 17, 2013, to Oct. 4, 2013. The bright spots near the center of the disk are active regions, areas of concentrated magnetic field that are prone to eruptions like solar flares and coronal mass ejections. These images were captured near the maximum activity phase of the sun’s 11-year cycle, a period during which active regions are concentrated near the sun’s equator.">这段视频从日出的X射线望远镜是一个近两个月的意象，复合从2013年8月17日到2013年10月4日。中心附近的磁盘的亮点是活跃的地区，集中的磁场区域，很容易爆发像太阳耀斑和日冕物质抛射。这些图像被捕获在太阳的11年周期的最大活动阶段，其间活跃的地区主要集中在太阳赤道的一段。</trans></p><hr style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; height: 0px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; margin-top: 20px; margin-bottom: 20px; word-spacing: 0px; border-top-color: rgb(238, 238, 238); border-right-width: 0px; border-bottom-width: 0px; border-left-width: 0px; border-top-style: solid; white-space: normal; box-sizing: content-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="box-sizing: border-box;" data-dst="Hinode拍摄了这张照片–Lovejoy彗星在这里看到，在2011年12月16日的太阳光学望远镜的架–左下橙色条纹。彗星Lovejoy彗星是Kreutz家族的一大成员，一组经常通过非常接近太阳的彗星。Lovejoy彗星在它存活下来的绕太阳是罕见的，新兴的完整的另一面。" data-src="Hinode captured this image of Comet Lovejoy – seen here as an orange streak in the lower left of the frame – with its Solar Optical Telescope on Dec. 16, 2011. Comet Lovejoy is a large member of the Kreutz family of comets, a group of comets that often pass extremely close to the sun. Comet Lovejoy is rare in that it survived its trip around the sun, emerging intact on the other side."><a href="data/attachment/portal/201610/20/110349kzr32ngwgw433tlp.jpg" target="_blank" style="font-family: Tahoma, Arial, Helvetica, snas-serif; line-height: 1.8em;">

</a>Hinode拍摄了这张照片–Lovejoy彗星在这里看到，在2011年12月16日的太阳光学望远镜的架–左下橙色条纹。彗星Lovejoy彗星是Kreutz家族的一大成员，一组经常通过非常接近太阳的彗星。Lovejoy彗星在它存活下来的绕太阳是罕见的，新兴的完整的另一面。</trans></p><hr style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; height: 0px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; margin-top: 20px; margin-bottom: 20px; word-spacing: 0px; border-top-color: rgb(238, 238, 238); border-right-width: 0px; border-bottom-width: 0px; border-left-width: 0px; border-top-style: solid; white-space: normal; box-sizing: content-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><div class="dnd-atom-wrapper type-image context-full_width" style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px auto 2em; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; clear: both; word-spacing: 0px; display: table; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><div class="dnd-drop-wrapper" style="box-sizing: border-box;"><p><a href="data/attachment/portal/201610/20/110432wan54qdqnihqg3aj.gif" target="_blank">

</a></p></div><div class="dnd-legend-wrapper" style="font-size: 11px; box-sizing: border-box;"><div class="caption" style="box-sizing: border-box;"></div><div class="credits" style="font-style: italic; font-weight: 700; box-sizing: border-box;"><trans style="box-sizing: border-box;" data-dst="美国宇航局/日本宇宙航空研究开发机构/学分：日出" data-src="Credits: NASA/JAXA/Hinode">美国宇航局/日本宇宙航空研究开发机构/学分：日出</trans></div><div class="link" style="background: inherit; padding: 0px; box-sizing: border-box;"><a style="background: 0px 0px; color: rgb(66, 139, 202); box-sizing: border-box;" href="http://www.nasa.gov/feature/goddard/2016/highlights-from-a-decade-of-jaxa-and-nasa-s-hinode-solar-observatory"></a></div></div></div><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="box-sizing: border-box;" data-dst="Hinode抓住了这1太阳爆炸视图，2014。这次爆炸是由不稳定的磁场在太阳表面掀起。这个镜头是由Hinode X射线望远镜拍摄的。虽然X射线通常是肉眼看不见的，它们是彩色在橙色方便查看。" data-src="Hinode caught this view of a solar explosion on Aug.1, 2014. This explosion was set off by unstable magnetic fields on the sun’s surface. The footage was captured by Hinode’s X-ray Telescope. Though X-rays are typically invisible to our eyes, they are colorized here in orange for easy viewing.">Hinode抓住了这1太阳爆炸视图，2014。这次爆炸是由不稳定的磁场在太阳表面掀起。这个镜头是由Hinode X射线望远镜拍摄的。虽然X射线通常是肉眼看不见的，它们是彩色在橙色方便查看。</trans></p><hr style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; height: 0px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; margin-top: 20px; margin-bottom: 20px; word-spacing: 0px; border-top-color: rgb(238, 238, 238); border-right-width: 0px; border-bottom-width: 0px; border-left-width: 0px; border-top-style: solid; white-space: normal; box-sizing: content-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="box-sizing: border-box;" data-dst="日出的太阳光学望远镜拍下了这张2013年10月19日的太阳暗条。长丝是巨大的丝带相对凉爽的材料，通过太阳大气的螺纹，称为科罗娜啤酒。科学家们用这个形象和其他人从Hinode学习到更多关于太阳能材料在科罗娜啤酒加热。" data-src="Hinode’s Solar Optical Telescope took this close-up of a solar filament on Oct. 19, 2013. Filaments are huge ribbons of relatively cool material that thread through the sun’s atmosphere, called the corona. Scientists used this image and others from Hinode to learn more about how solar material is heated in the corona."><a href="data/attachment/portal/201610/20/110440rxivvkxvoqz7mnxx.png" target="_blank" style="font-family: Tahoma, Arial, Helvetica, snas-serif; line-height: 1.8em;">

</a></trans></p><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="box-sizing: border-box;" data-dst="日出的太阳光学望远镜拍下了这张2013年10月19日的太阳暗条。长丝是巨大的丝带相对凉爽的材料，通过太阳大气的螺纹，称为科罗娜啤酒。科学家们用这个形象和其他人从Hinode学习到更多关于太阳能材料在科罗娜啤酒加热。" data-src="Hinode’s Solar Optical Telescope took this close-up of a solar filament on Oct. 19, 2013. Filaments are huge ribbons of relatively cool material that thread through the sun’s atmosphere, called the corona. Scientists used this image and others from Hinode to learn more about how solar material is heated in the corona.">日出的太阳光学望远镜拍下了这张2013年10月19日的太阳暗条。长丝是巨大的丝带相对凉爽的材料，通过太阳大气的螺纹，称为科罗娜啤酒。科学家们用这个形象和其他人从Hinode学习到更多关于太阳能材料在科罗娜啤酒加热。</trans></p><hr style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; height: 0px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; margin-top: 20px; margin-bottom: 20px; word-spacing: 0px; border-top-color: rgb(238, 238, 238); border-right-width: 0px; border-bottom-width: 0px; border-left-width: 0px; border-top-style: solid; white-space: normal; box-sizing: content-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="background: none; box-sizing: border-box;" data-dst="太阳耀斑在太阳黑子会发生什么？Hinode帮助回答这个由2006年12月13日太阳光学望远镜拍摄的耀斑的观点，问题，推出后短短几个月。太阳能材料的可见光在太阳黑子的亮线帮助科学家推断有黑子和耀斑联系在一起。" data-src="What happens to a sunspot during a solar flare? Hinode helped answer that question with this view of a flare taken by its Solar Optical Telescope on Dec. 13, 2006, just a few months after launch. The bright threads of solar materials visible over the sunspots helped scientists deduce how sunspots and solar flares are linked."><a href="data/attachment/portal/201610/20/110523y5z075x1k59v115o.gif" target="_blank" style="font-family: Tahoma, Arial, Helvetica, snas-serif; line-height: 1.8em;">

</a>太阳耀斑在太阳黑子会发生什么？Hinode帮助回答这个由2006年12月13日太阳光学望远镜拍摄的耀斑的观点，问题，推出后短短几个月。太阳能材料的可见光在太阳黑子的亮线帮助科学家推断有黑子和耀斑联系在一起。</trans></p><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="box-sizing: border-box;" data-dst="日出的太阳光学望远镜捕捉到的这镜头，太阳的边缘。螺纹状的结构，有点像–草在风中挥舞–骨针，气体通过太阳的各个区域的能量转移巨大的羽毛。" data-src="Hinode’s Solar Optical Telescope captured this footage of the sun’s limb. The thread-like structures – which somewhat resemble grass waving in the wind – are spicules, giant plumes of gas that transfer energy through the sun’s various regions."><a href="data/attachment/portal/201610/20/110612bbtzkgurtrjnbtit.gif" target="_blank" style="font-family: Tahoma, Arial, Helvetica, snas-serif; line-height: 1.8em;">

</a>日出的太阳光学望远镜捕捉到的这镜头，太阳的边缘。螺纹状的结构，有点像–草在风中挥舞–骨针，气体通过太阳的各个区域的能量转移巨大的羽毛。</trans></p><hr style="font: 14px/20px "Helvetica Neue", Helvetica, Arial, sans-serif; height: 0px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; margin-top: 20px; margin-bottom: 20px; word-spacing: 0px; border-top-color: rgb(238, 238, 238); border-right-width: 0px; border-bottom-width: 0px; border-left-width: 0px; border-top-style: solid; white-space: normal; box-sizing: content-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-text-stroke-width: 0px;"><p style="font: 14px/1.4em "Helvetica Neue", Helvetica, Arial, sans-serif; margin: 0px 0px 15px; color: rgb(0, 0, 0); text-transform: none; text-indent: 0px; letter-spacing: normal; word-spacing: 0px; white-space: normal; box-sizing: border-box; widows: 1; background-color: rgb(255, 255, 255); -webkit-font-smoothing: inherit; -webkit-text-stroke-width: 0px;"><trans style="background: none; box-sizing: border-box;" data-dst="这个特写镜头从日出的太阳光学望远镜显示对流细胞在太阳表面。对流是太阳将能量从深处到表面的一种方式，它发出的光和热。" data-src="This close-up from Hinode’s Solar Optical Telescope shows convection cells on the surface of the sun. Convection is one way that the sun transports energy from its depths up to the surface, where it’s emitted as light and heat."><a href="data/attachment/portal/201610/20/110645fhhip8ntmqh2m9kd.gif" target="_blank" style="font-family: Tahoma, Arial, Helvetica, snas-serif; line-height: 1.8em;">

</a>这个特写镜头从日出的太阳光学望远镜显示对流细胞在太阳表面。对流是太阳将能量从深处到表面的一种方式，它发出的光和热。</trans></p><br class="Apple-interchange-newline">

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