难得一见、甚为壮观的太阳表面照片
<FONT size=4><FONT color=black><STRONG>1.逃离太阳的等离子体</STRONG> </FONT></FONT><P align=center><B><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171328311.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></B></P>
<P align=center><FONT color=black size=4>逃离太阳的等离子体</FONT></P><FONT color=black size=4> 在这张照片上,我们看到大量温度相对低、相对稠密的等离子体悬浮于日冕(太阳大气的最外层)表面。偶尔,这些猛烈的等离子体会突出重围,逃离太阳大气的魔掌。这条光谱线上的放射物是温度高达10万华氏度的色球高层(upper chromosphere)。照片中的每一个特征都追寻着磁场结构的足迹。温度最高的区域几乎全是白色,而颜色暗红的区域则表明温度相对较低。<BR><B> 2.太阳表面磁场结构的特写</B><BR></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171330770.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><FONT color=black size=4>太阳表面磁场结构的特写</FONT></P><FONT color=black size=4> 这是一张有关太阳表面磁场结构的特写照片,是口径为1 米的瑞典太阳望远镜(SST)于2003年8月22日以H-alpha光波拍摄到的。该望远镜由瑞典皇家科学院负责操作。<BR><B> 3.太阳黑子</B><BR></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171330235.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><FONT color=black size=4>太阳黑子</FONT></P><FONT color=black size=4> 这是一张2002年7月24日在太阳东侧边缘拍摄的太阳活跃区域的照片。它突出了这张照片的三维特点。照片上方中央区域的黑色太阳黑子结构表明,太阳黑子黑色“地板”上独特的立视面。据美国高空观测台天文学家布鲁斯·莱特斯(Bruce Lites)博士估计,这些结构的高度大概在200公里至450公里之间。照片中最小的可分解结构规模约在70公里左右。另外,我们可以从面向观测者的颗粒边缘看见无数明亮的光斑。<BR><B> 4.太阳上的“地震”</B><BR></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171330807.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><FONT color=black size=4>太阳上的“地震”</FONT></P>
<P><FONT color=black size=4> 太阳耀斑在太阳内部产生震波,与地球上地震产生的震波极为相似。1998年5月27日,研究人员观测到这次生成耀斑的太阳震动。据科学家估计,这次震动包含的能量大概是1906年旧金山大地震释放能量的4万倍,相当于11.3级地震。在一小时内,太阳波飞行的距离相当于十个地球的直径,之后活动强度越来越小,最终蜕变为太阳色球层的狂暴背景。与以等速度向外运行的水的波纹不同,太阳波在消失之前从最初每小时2.2万英里的速度向最高每小时25万英里的速度逐级递进。</FONT></P> <P><FONT size=4><FONT color=black><B>5.日全食的壮观日冕</B><BR></FONT></FONT></P>
<P align=center><B><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171330923.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></B></P>
<P align=center><FONT color=black size=4>日全食的壮观日冕</FONT></P><FONT color=black size=4> 这张日全食的照片是由美国国家大气研究中心高空观测台的研究小组于1980年2月16日在印度帕勒姆拍摄到的。日冕照片则是用戈登·纽科克(Gordon A. Newkirk)研制的一套新摄像机捕捉到的。这种专门的仪器可以通过放射过滤器,以红光拍摄到日冕。过滤器抑制明亮的内冕,以在同一张照片中显示光线更微弱的外冕。<BR><B> 6.金星穿越太阳盘面</B><BR><BR></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171330710.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><FONT color=black size=4>金星穿越太阳盘面</FONT></P><FONT color=black size=4> 美宇航局TRACE卫星在2004年6月8日金星开始穿越太阳盘面时捕捉到这张不同寻常的照片。<BR><B> 7.太阳黑子和光斑</B><BR></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171331907.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><FONT color=black size=4>太阳黑子和光斑</FONT></P><FONT color=black size=4> 2003年8月4日,瑞典太阳望远镜(SST)捕捉到的太阳表面太阳黑子和光斑的壮观照片。<BR><B> 8.剧烈的太阳耀斑</B><BR></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171331966.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><FONT color=black size=4>剧烈的太阳耀斑<BR></FONT></P>
<P><FONT color=black size=4> “日出”(前称太阳-B)太阳观测卫星在2006年12月13日成功捕捉到剧烈的太阳耀斑的照片。这是那次太阳活动强度处于低谷时期发生的最为剧烈的太阳耀斑之一。</FONT></P> <P><FONT size=4><FONT color=black><B><SPAN>9.太阳活动低谷时的日冕</SPAN></B><BR></FONT></FONT></P>
<P align=center><B><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171331559.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></B></P>
<P align=center><SPAN><FONT color=black size=4>太阳活动低谷时的日冕</FONT></SPAN></P><SPAN><SPAN><SPAN><FONT color=black size=4> 这是太阳活动处于低谷时日冕的照片,两个半球中的红色代表温度高、较为</FONT><A id=vad_9 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,9,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,9)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_2.html&aid=10542&sid=6235007045041591&click=1&url=http%3A//www.vancl.com/WebSource/WebSource.aspx%3Fsource%3Dvogate%26SourceSunInfo%3D%26url%3Dhttp%3A//www.vancl.com/VanclZl/hjth.html&v=0&s=http%3A//qwgt.com/nature/universe/14052_3.html&rn=650000&k=%u6D3B%u8DC3" target=_blank name=9><FONT color=black size=4>活跃</FONT></A><FONT color=black size=4>的区域,周围则是安静日冕的温度低的等离子体(蓝色/</FONT></SPAN></SPAN><A id=vad_0 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,0,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,0)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_2.html&aid=10367&sid=6235007045041591&click=1&url=http%3A//www.qzwb.com&v=0&s=http%3A//qwgt.com/nature/universe/14052_3.html&rn=764986&k=%u7EFF%u8272" target=_blank name=0><FONT color=black size=4>绿色</FONT></A><FONT color=black size=4>)。同时还应注意北极皇冠状细丝、横跨赤道的光环、照片东南角的冕洞(日冕中一些辐射很弱、亮度比周围小得多的区域)和北极上方一个更小的日冕洞。这张照片以伪色、三层合成显示了日冕:蓝色、绿色和红色分别显示的是171、195和284的波长。</FONT></SPAN><BR><FONT size=4><FONT color=black><B><SPAN> 10.太阳表面不规则的黑子和光斑</SPAN></B><BR></FONT></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171331836.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><SPAN><FONT color=black size=4>太阳表面不规则的黑子和光斑</FONT></SPAN></P><FONT size=4><FONT color=black><SPAN> 2003年8月22日,瑞典太阳望远镜拍摄到的太阳表面不规则形状的太阳黑子和光斑的照片。</SPAN><BR> <B><SPAN><SPAN>11.水星<A id=vad_2 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,2,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,2)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_2.html&aid=10546&sid=6235007045041591&click=1&url=http%3A//www.vogate.com/bbs/viewthread.php%3Ftid%3D364%26page%3D1%26extra%3Dpage%253D1%20&v=0&s=http%3A//qwgt.com/nature/universe/14052_3.html&rn=799511&k=%u5F00%u59CB" target=_blank name=2>开始</A>经过太阳前方</SPAN></SPAN></B><BR></FONT></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171332235.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><SPAN><SPAN><FONT color=black size=4>水星开始经过太阳前方</FONT></SPAN></SPAN></P><FONT size=4><FONT color=black><SPAN><SPAN> 美宇航局TRACE卫星在2006年11月8日捕捉到的水星开始经过太阳前方的照片。</SPAN></SPAN><BR> <B><SPAN><SPAN>12.太阳东侧边缘朝向<A id=vad_5 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,5,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,5)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_2.html&aid=10698&sid=6235007045041591&click=1&url=http%3A//ag.weelaa.com/reg.php%3Fid%3Dcpc020&v=0&s=http%3A//qwgt.com/nature/universe/14052_3.html&rn=215724&k=%u5730%u7403" target=_blank name=5>地球</A></SPAN></SPAN></B><BR></FONT></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171332891.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><SPAN><SPAN><FONT color=black size=4>太阳东侧边缘朝向地球</FONT></SPAN></SPAN></P>
<P><SPAN><SPAN><SPAN><SPAN><FONT color=black size=4> 这是美宇航局TRACE卫星2006年11月11日在171波长下拍摄到的照片,显示的是一个位于太阳东侧边缘的相当大的活跃区域转向朝地球的半球时的情景。请注意该区域前缘细丝的低浅、</FONT></SPAN><A id=vad_6 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,6,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,6)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_2.html&aid=10499&sid=6235007045041591&click=1&url=http%3A//www.vancl.com/websource/websource.aspx%3Furl%3Dhttp%3A//www.vancl.com/%26source%3Dvogate&v=0&s=http%3A//qwgt.com/nature/universe/14052_3.html&rn=656468&k=%u9ED1%u8272" target=_blank name=6><FONT color=black size=4>黑色</FONT></A><SPAN><A id=vad_8 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,8,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,8)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_2.html&aid=10501&sid=6235007045041591&click=1&url=http%3A//www.vancl.com/websource/websource.aspx%3Furl%3Dhttp%3A//www.vancl.com/%26source%3Dvogate&v=0&s=http%3A//qwgt.com/nature/universe/14052_3.html&rn=747063&k=%u7ED3%u6784" target=_blank name=8><FONT color=black size=4>结构</FONT></A><FONT color=black size=4>,以及该区域右侧一些“飘浮”黑色物质和朝向右方下面的瞬间显现的小区域。</FONT></SPAN></SPAN></SPAN></SPAN></P> <P><B><SPAN><SPAN><FONT color=black size=4>13.太阳保持强度极低</FONT><A id=vad_3 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,3,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,3)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_3.html&aid=10150&sid=6235007045041591&click=1&url=http%3A//www.vogate.com/bbs&v=0&s=http%3A//qwgt.com/nature/universe/14052_4.html&rn=589073&k=%u6D3B%u52A8" target=_blank name=3><FONT color=black size=4>活动</FONT></A><FONT color=black size=4>水平</FONT></SPAN></SPAN></B><BR></P>
<P align=center><B><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171332296.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></B></P>
<P align=center><SPAN><SPAN><FONT color=black size=4>太阳保持强度极低活动水平</FONT></SPAN></SPAN></P><SPAN><SPAN><SPAN><FONT color=black size=4> 美宇航局TRACE卫星于2008年5月22日拍摄到的太阳照片。由于太阳始终保持在强度极低的活动水平,在盘面上只有很小一部分区域</FONT><A id=vad_5 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,5,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,5)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_3.html&aid=10360&sid=6235007045041591&click=1&url=http%3A//www.vogate.com/bbs&v=0&s=http%3A//qwgt.com/nature/universe/14052_4.html&rn=181310&k=%u53EF%u4EE5" target=_blank name=5><FONT color=black size=4>可以</FONT></A><FONT color=black size=4>看到。细胞状外形是由一束束磁流形成的,磁流是在充斥着对流活动的超光斑网络的下冲区域中收集到的。</FONT></SPAN></SPAN></SPAN><BR><FONT color=black size=4> <B><SPAN>14.光环在太阳活跃区上方如拱门</SPAN></B><BR></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171333643.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><SPAN><FONT color=black size=4>光环在太阳活跃区上方如拱门</FONT></SPAN></P><FONT size=4><FONT color=black><SPAN> 2001年1月1日,薄薄的光环在太阳活跃区上面如拱门一般出现的壮观景象。</SPAN><BR> <B>15.日冕物质喷发快速扩散</B><BR></FONT></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171333235.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><FONT color=black size=4>日冕物质喷发快速扩散</FONT></P><FONT size=4><FONT color=black><SPAN> 在LASCO卫星2002年1月8日拍摄的这张照片显示的是日冕物质喷发(CME)快速扩散的情景,当时,日冕以每小时数百万公里的速度向太空喷射了十亿吨物质。这张C2照片旋转了90度,如此一来,看上去好像是日冕向下喷射物质。研究人员将美宇航局远紫外线成像望远镜在另外一天拍摄的太阳照片放大,与这张C2照片重叠,这样,它完全覆盖于剩余的盘面,增强了视觉效果。</SPAN><BR> <B><SPAN><SPAN>16.太阳表面磁场<A id=vad_7 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,7,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,7)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_3.html&aid=10501&sid=6235007045041591&click=1&url=http%3A//www.vancl.com/websource/websource.aspx%3Furl%3Dhttp%3A//www.vancl.com/%26source%3Dvogate&v=0&s=http%3A//qwgt.com/nature/universe/14052_4.html&rn=343407&k=%u7ED3%u6784" target=_blank name=7>结构</A></SPAN></SPAN></B><BR></FONT></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171334103.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><SPAN><SPAN><FONT color=black size=4>太阳表面磁场结构</FONT></SPAN></SPAN></P>
<P><SPAN><SPAN><FONT color=black size=4> 瑞典太阳望远镜在2003年8月22日以H-alpha光波拍摄的太阳表面磁场结构近距离特写照片。</FONT></SPAN></SPAN></P> <P><B><SPAN><FONT color=black size=4>17.</FONT><A id=vad_1 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,1,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,1)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_4.html&aid=10528&sid=6235007045041591&click=1&url=&v=0&s=http%3A//qwgt.com/nature/universe/14052_5.html&rn=382480&k=%u7A81%u51FA" target=_blank name=1><FONT color=black size=4>突出</FONT></A><FONT color=black size=4>物喷发</FONT></SPAN></B><BR></P>
<P align=center><B><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171334282.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></B></P>
<P align=center><SPAN><FONT color=black size=4>突出物喷发</FONT></SPAN></P><FONT size=4><FONT color=black><SPAN><SPAN> 美宇航局卫星2008年9月29日观测到这次给人视角冲击的突出物喷发事件。这些突出物在数小时里先是升起,后如瀑布般落下,此情此景就像冉冉升起的一面大旗,然后分离涌向太空。照片中可以看到的物质其实是温度高达6万度的电离氦。突出物则是温度相对较低的气云,悬浮于太阳表面,受到磁力的控制。</SPAN></SPAN><BR> <B><SPAN>18.月球从太阳盘面缓缓经过</SPAN></B><BR></FONT></FONT>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171334642.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><SPAN><FONT color=black size=4>月球从太阳盘面缓缓经过</FONT></SPAN></P><SPAN><SPAN><FONT color=black size=4> 月球在2007年2月25日从太阳盘面缓缓经过的镜头,遗憾的是,这一幕在</FONT><A id=vad_4 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,4,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,4)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_4.html&aid=10698&sid=6235007045041591&click=1&url=http%3A//ag.weelaa.com/reg.php%3Fid%3Dcpc020&v=0&s=http%3A//qwgt.com/nature/universe/14052_5.html&rn=619839&k=%u5730%u7403" target=_blank name=4><FONT color=black size=4>地球</FONT></A><SPAN><FONT color=black size=4>上看不到。STEREO-B卫星在绕太阳轨道飞行时拍摄到这张照片。美宇航局STEREO任务由发生于2006年10月、用以研究太阳风暴的两颗卫星组成。STEREO-B卫星目前距离地球约100万英里,同月球的距离是它同地球距离的4.4倍,结果,照片中出现的月球相当于</FONT><A id=vad_7 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,7,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,7)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_4.html&aid=10669&sid=6235007045041591&click=1&url=http%3A//www.szinfo.com&v=0&s=http%3A//qwgt.com/nature/universe/14052_5.html&rn=899219&k=%u6211%u4EEC" target=_blank name=7><FONT color=black size=4>我们</FONT></A><FONT color=black size=4>通常看到的月球大小的1/4.4。</FONT></SPAN></SPAN></SPAN><BR><B><SPAN><SPAN><FONT color=black size=4> 19.太阳边缘</FONT><A id=vad_8 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,8,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,8)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_4.html&aid=10542&sid=6235007045041591&click=1&url=http%3A//www.vancl.com/WebSource/WebSource.aspx%3Fsource%3Dvogate%26SourceSunInfo%3D%26url%3Dhttp%3A//www.vancl.com/VanclZl/hjth.html&v=0&s=http%3A//qwgt.com/nature/universe/14052_5.html&rn=854882&k=%u6D3B%u8DC3" target=_blank name=8><FONT color=black size=4>活跃</FONT></A><FONT color=black size=4>地区的耀斑</FONT></SPAN></SPAN></B><BR>
<P align=center><FONT color=black size=4><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171335577.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0></FONT></P>
<P align=center><SPAN><SPAN><FONT color=black size=4>太阳边缘活跃地区的耀斑</FONT></SPAN></SPAN></P><SPAN><SPAN><SPAN><SPAN><FONT color=black size=4> 2001年9月30日,美宇航局STEREO卫星在靠近太阳边缘的活跃地区观测到一次强度不大的耀斑。突出物的细丝飘浮在上面,丝般的</FONT></SPAN><A id=vad_6 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,6,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,6)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_4.html&aid=10499&sid=6235007045041591&click=1&url=http%3A//www.vancl.com/websource/websource.aspx%3Furl%3Dhttp%3A//www.vancl.com/%26source%3Dvogate&v=0&s=http%3A//qwgt.com/nature/universe/14052_5.html&rn=332189&k=%u9ED1%u8272" target=_blank name=6><FONT color=black size=4>黑色</FONT></A><SPAN><FONT color=black size=4>(温度相对低)物质沿着场力线</FONT><A id=vad_9 onmouseover="this.style.borderBottom='2px #FF3366 solid';var fxEvent=arguments;kwmouseover(this,9,fxEvent);" style="FONT-SIZE: 1em; CURSOR: pointer; COLOR: #ff3366; BORDER-BOTTOM: #ff3366 1px dotted; TEXT-DECORATION: underline" onmouseout="this.style.borderBottom='1px #FF3366 dotted'; kwmouseout(this,9)" href="http://action.vogate.com/c/c.php?r=http%3A//qwgt.com/nature/universe/14052_4.html&aid=6374&sid=6235007045041591&click=1&url=http%3A//www.fisheyes.cn/category.php%3Fid%3D4&v=0&s=http%3A//qwgt.com/nature/universe/14052_5.html&rn=473868&k=%u79FB%u52A8" target=_blank name=9><FONT color=black size=4>移动</FONT></A><FONT color=black size=4>,接着扩展形成这种舞龙般的明亮轮廓。(孝文)</FONT></SPAN></SPAN></SPAN></SPAN> 太美了 精彩 好看 壮观,见识了,谢谢。
回复 1樓 dianyinke 的帖子
没钱,赚钱去,再来看 太美呢! 一个字,太美了! 精美壮观。 太美了 真是太漂亮了! 精美绝伦,蔚为壮观。 至阳至刚。 <P><IMG onmousewheel="return imgzoom(this);" onmouseover="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.style.cursor='hand'; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" onclick="if(!this.resized) {return true;} else {window.open(this.src);}" alt="" src="http://qwgt.com/nature/UploadFiles_2588/200810/20081020171333235.jpg" onload="if(this.width>screen.width*0.7) {this.resized=true; this.width=screen.width*0.7; this.alt='Click here to open new window\nCTRL+Mouse wheel to zoom in/out';}" border=0> </P><P> </P>
<P><FONT color=red size=6><STRONG>壮哉,太阳! </STRONG></FONT></P> <DIV class=t_msgfont id=postmessage_210573>壮观,见识了,谢谢。</DIV> 太美了 太美了 美丽,但也可怕。人类何其渺小。 不错!!!!!!!!!!! <FONT color=blue size=4>不应该叫“地震”,应该叫作:“阳震”。</FONT> 太美极了! 壮观,见识了,谢谢 美,壮观,难得一见。 这 才 认 清 太 阳 了 <P>哇,</P>
<P> </P>
<P>真美,</P>
<P> </P>
<P>看了后非常非常的震撼啊 </P>
<P> </P>
<P> </P> 有这么多图片和文字的介绍,很生动啊
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