• 因为保密等原因,不能提供更多获得数据的仪器等方面的描述,数据更新时间为不定时更新,此数据为DUT1=UT1-UTC 值的公告,以+/-0.1s 精度的时间信号传输。
  • 2D spectral observation data of solar towers from 1999 to 2015.
  • 由于这种图像显示方式对画面生成及显示有极高的要求,现在,360度×180度的全景画幅只应用在了极少数的科技娱乐场馆当中。
  • We present a three-dimensional (3D) extinction map of the southern sky.
    with the distances calculated from the Gaia data release 2 (DR2) parallaxes, we have constructed a 3D ...
    By combining our 3D extinction map with those from the literature, we present an all-sky 3D extinction ...
    map, and use it to explore the 3D distribution of the Galactic dust grains.
    We use two different models, one consisting of a single disk and another of two disks, to fit the 3D ...
  • We present a three-dimensional (3D) extinction map of the southern sky.
    with the distances calculated from the Gaia data release 2 (DR2) parallaxes, we have constructed a 3D ...
    By combining our 3D extinction map with those from the literature, we present an all-sky 3D extinction ...
    map, and use it to explore the 3D distribution of the Galactic dust grains.
    We use two different models, one consisting of a single disk and another of two disks, to fit the 3D ...
  • We present a three-dimensional (3D) extinction map of the southern sky.
    with the distances calculated from the Gaia data release 2 (DR2) parallaxes, we have constructed a 3D ...
    By combining our 3D extinction map with those from the literature, we present an all-sky 3D extinction ...
    map, and use it to explore the 3D distribution of the Galactic dust grains.
    We use two different models, one consisting of a single disk and another of two disks, to fit the 3D ...
  • We present a three-dimensional (3D) extinction map of the southern sky.
    with the distances calculated from the Gaia data release 2 (DR2) parallaxes, we have constructed a 3D ...
    By combining our 3D extinction map with those from the literature, we present an all-sky 3D extinction ...
    map, and use it to explore the 3D distribution of the Galactic dust grains.
    We use two different models, one consisting of a single disk and another of two disks, to fit the 3D ...
  • 图1:漫游截图 3D模型怎么选? 万维望远镜能够导入3DS和OBJ两种格式的3D模型。
    图2:OBJ格式(左)与3DS格式(右)对比 如果你不知道去哪里找3D模型,这里为大家提供了一些网址可供参考: NASA 3D资源网:https://nasa3d.arc.nasa.gov/models ...
    图3:3D模型的导入 如果你暂时没有找到适合的3D模型,其实万维望远镜本身就自带了一个3D模型——国际空间站。
    图4:国际空间站3D模型 让你的3D模型动起来!
    假设我们要模拟ISS的运行情况,首先在网络上搜索它的TLE(参考网址:https://celestrak.com/)。
  • Xu, D. Liang, and L.
    Xu, D. Liang, and L. Shao, Static spherical vacuum solutions in the bumblebee gravity model, Phys.
    D 107, 024011 (2023) Units: Geometrized (G=c=1) and the radius of the horizon taken as the unit length ...
  • Xu, D. Liang, and L.
    Xu, D. Liang, and L. Shao, Static spherical vacuum solutions in the bumblebee gravity model, Phys.
    D 107, 024011 (2023) Units: Geometrized (G=c=1) and the radius of the horizon taken as the unit length ...
  • Xu, D. Liang, and L.
    Xu, D. Liang, and L. Shao, Static spherical vacuum solutions in the bumblebee gravity model, Phys.
    D 107, 024011 (2023) Units: Geometrized (G=c=1) and the radius of the horizon taken as the unit length ...
  • Xu, D. Liang, and L.
    Xu, D. Liang, and L. Shao, Static spherical vacuum solutions in the bumblebee gravity model, Phys.
    D 107, 024011 (2023) Units: Geometrized (G=c=1) and the radius of the horizon taken as the unit length ...
  • 为了庆祝新朋友加入,同时鼓励大家创作出更优秀的作品,国家天文科学数据中心联合航天文创CASCI联合推出3D模型大礼包,一次性为你奉上7个制作精美的3D模型,并提前制作成便于漫游使用的图层文件。
    图1 系列3D模型由双方联合发布 3D模型列表 1、SOHO (Solar and Heliospheric Ocservatory) 中文译名:太阳和日球层探测器 SOHO是太阳探测卫星。
    大赛网站的万维望远镜科普资源栏目可以下载这些图层文件 使用方法:(观看教学视频请点击这里) 如果需要模拟天问一号向火星出发的场景,可首先在地球图层上点击右键—添加—选择图层文件即可将天问一号3D模型导入万维望远镜 ...
  • 本文将介绍M31N 2017-01e两次再爆发——M31N 2022-03d和M31N 2019-09d的发现和证认过程。
    图1 M31N 2022-03d发现图像 编号:M31N 2022-03d(=PNV J00441072+4154224=AT 2022fcy=PSP22P) 发现时间:2022年3月5日22 ...
    图4 M31N 2019-09d发现图像 编号:M31N 2019-09d(=PNV J00441073+4154220=PSP19C) 发现时间:2019年9月22日23时28分11秒 ...
    但可惜的是,M31N 2019-09d变暗非常迅速,根本不给人拍摄光谱的机会;而M31N 2022-03d上报时距离爆发已过去二十余天,也早已暗下去。
    Shafter教授表示他正在确认一些再发新星,应其要求,赵经远先后向他提供了M31N 2022-03d和M31N 2019-09d接近峰值亮度的图像,以及一系列测光数据。
  • Properties of host galaxies of type II AGNs derived from 2D decomposition to their HST images using galfit ...
  • numbers of stars in the SP-sample, columns 4–5 are the spectroscopy types classified by the LAMOST 1D ...
  • stars in the duplicate SP-sample, columns 4-5 are the spectroscopy types classified by the LAMOST 1D ...
  • stars in the duplicate SP-sample, columns 4-5 are the spectroscopy types classified by the LAMOST 1D ...
  • Properties of host galaxies of type 1 AGNs derived from 2D decomposition to their HST images using galfit ...
  • Supported by the National Key R&D Program “Cosmological High performance heterogeneous simulation system ...
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