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	A CLOCK SCANNING SYNTHETIC APERTURE RADIOMETER AS A POTENTIAL PAYLOAD OF SPORT 会议论文 OAI收割 IEEE International Geoscience and Remote Sensing Symposium (IGARSS), Quebec, CANADA, JUL 13-18, 2014 作者: Zhang, Cheng; Liu, Hao; Wu, Ji; Sun, Weiying; Niu, Lijie 收藏 \| 浏览/下载：29/0 \| 提交时间：2015/09/18 Solar polar orbit radiometer synthetic aperture clock scan
	The Lyman-alpha Imager onboard Solar Polar Orbit Telescope 会议论文 OAI收割 International Conference on Optical Instruments and Technology - Optical Systems and Modern Optoelectronic Instruments, Beijing, PEOPLES R CHINA, NOV 17-19, 2013 作者: Li, Baoquan; Li, Haitao; Zhou, Sizhong; Jiang, Bo 收藏 \| 浏览/下载：38/0 \| 提交时间：2014/04/30 LMI Lyman-alpha Imager corona mass ejections Solar Polar Orbit Telescope
	Imaging interplanetary CMEs at radio frequency from solar polar orbit 期刊论文 OAI收割 ADVANCES IN SPACE RESEARCH, 2011, 卷号: 48, 期号: 5, 页码: 943-954 作者: Wu Ji; Sun Weiying 收藏 \| 浏览/下载：22/0 \| 提交时间：2014/12/15 Interplanetary CMEs Interferometric imaging Solar polar orbit Radio telescope
	The Simulation measurement experiment and calibration for Solar Total Irradiance Monitor on board (EI CONFERENCE) 会议论文 OAI收割 ICO20: Remote Sensing and Infrared Devices and Systems, August 21, 2005 - August 26, 2005, Changchun, China Yupeng W.; Wei F.; Bingxi Y. 收藏 \| 浏览/下载：37/0 \| 提交时间：2013/03/25 STIM (Solar Total Irradiance Monitor) can be used on sun-synchronous polar orbit weather satellites to measure the total solar irradiance. It contains three independent and identical wide view absolute radiometers. They are mounted on the satellite in an angle which ensure the sun scan over the field of view of the absolute radiometers. This measurement method doesn't need the instrument tracking the sun but the sun scan over the field of view of the absolute radiometers in each orbit cycle. The paper presents the measurement method of simulation for solar irradiance measurement and calibration by mounting the instrument on a two-axis rotation table. By controlling the rotation angle velocity of the instrument in the meridian direction being the same as that of the weather satellite's on orbit we can measure the solar irradiance when the sun scan over the field of view of the absolute radiometers to simulate the onboard state. And we have operated the measurement with the prototype of STIM. The SIAR-1 is traceable to WRR and serves as a transfer standard. So simultaneous comparison measurements between SIAR-1 and each of the three wide view absolute radiometers are measured to provide calibration corrections to the instrument. And we have a further study at the influence of stray light to the measurement results. This paper presents the method of simulation experiment and calibration for solar irradiance measurement with Solar Total Irradiance Monitor on board.
	The full hemisphere integrating measurement of the reflectance of black cavity (EI CONFERENCE) 会议论文 OAI收割 ICO20: Illumination, Radiation, and Color Technologies, August 21, 2005 - August 26, 2005, Changchun, China 作者: Wang Y.; Yu B.; Wang Y.; Wang Y.; Wang Y. 收藏 \| 浏览/下载：18/0 \| 提交时间：2013/03/25 The conical black cavities are used in the Solar Irradiance Absolute Radiometers (SIARs) of the solar constant monitor aboard on the SZ spaceship and of the Solar Total Irradiance Monitor (STIM) aboard on sun-synchronous polar orbit weather satellites. A low reflectance measurement instrument which is used for making the integrating measurement on the reflectance of the conical black cavity in a high precision within the full hemisphere (include the entrance of the Ulbrichtsphere) has been constructed. The characteristic of the instrument is the employment of a semi-transparent mirror which is mounted in an inclination angle of 45 degrees in front of the entrance of the Ulbrichtsphere. The incident beam is reflected to the black cavity or white board by the semi-transparent mirror. A portion of those which is made diffused reflection through the black cavity or white board is measured by the detector located in the side face of the Ulbrichtsphere and the other portion which is reflected to the entrance is measured by the other detector after passing through the semi-transparent mirror and then being focused on by an ellipsoidal mirror. The two measurement data are added up to get the integrating reflectance within full hemisphere. The presentation and verification on the measurement result of the reflectance of the black cavity and its precision are described in this article. The absolute accuracy can reach 0.012%.