机译:未解决的精细结构得以解决:IRIS对太阳过渡区的观测
Univ Oslo, Inst Theoret Astrophys, NO-0315 Oslo, Norway;
Univ Oslo, Inst Theoret Astrophys, NO-0315 Oslo, Norway|Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA;
Univ Oslo, Inst Theoret Astrophys, NO-0315 Oslo, Norway;
Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA;
Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA;
Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA;
Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA;
Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA;
Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA;
Univ Oslo, Inst Theoret Astrophys, NO-0315 Oslo, Norway;
Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA;
Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA;
Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA;
Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA;
Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA;
Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA;
Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA;
Montana State Univ, Dept Phys, Bozeman, MT 59717 USA;
Montana State Univ, Dept Phys, Bozeman, MT 59717 USA;
Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA|Bay Area Environm Res Inst, Sonoma, CA 95476 USA;
Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA|Bay Area Environm Res Inst, Sonoma, CA 95476 USA;
机译:IRIS在太阳过渡区观察到的未解析精细结构环的性质和建模
机译:太阳过渡区的大气层对应物未解析的精细结构环
机译:太阳能过渡区域精细结构模型的研究
机译:重建粗糙分辨卫星观察的细尺空气污染结构
机译:太阳过渡区:高分辨率FUV-EUV成像和未解析的日冕漏斗建模,这是通过多光谱太阳望远镜阵列II:MSSTA II进行的第二次飞行。
机译:安静和背景噪声中分辨出的和未分辨出的谐波区域对脑干语音诱发反应的贡献
机译:未解决的精细结构已解决 - IRIs对太阳能的观测 过渡地区