EGU23-17162, updated on 26 Feb 2023
https://doi.org/10.5194/egusphere-egu23-17162
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

The first light from the joint total solar irradiance measurement experiment onboard the FY3-E meteorological satellite

Xin Ye1, Ping Zhu2, Jean-Philippe Montillet5, Xiuqing Hu3, Jinhua Wang4, Dongjun Yang1, Jin Qi3, Wolfgang Finsterle5, Peng Zhang3, Wei Fang1, Silvio Koller5, Daniel Pfiffner5, Baoqi Song1, Zhitao Luo1, Kai Wang1, Margit Haberreiter5, Duo Wu1, and Werner Schmutz5
Xin Ye et al.
  • 1Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Dongnan Hu Road 3888, Changchun, 130033, Jilin, China
  • 2Institute for Advanced Study, Shenzhen University, Shenzhen, China.
  • 3National Satellite Meteorological Center, China Meteorological Administration, Beijing, China
  • 4Shanghai Academy of Spaceflight Technology, Shanghai, China
  • 5Physikalisch-Meteorologisches Observatorium Davos and World Radiation Center, Davos Switzerland

The Fengyun 3E (FY3E) spacecraft was launched on the 4th of July 2021 at 23h 28min UTC according to CASC (China Aerospace Science and Technology Corp.) on a Long March 4C vehicle from JSLC (Jiuquan Space Launch Center) in China. The orbit is a sun-synchronous near-circular with an altitude of 800 km, and an inclination of 98.7 degrees. The nominal lifetime of the satellite is eight years. The JTSIM experiments belong to the solar activities monitoring package. The solar radiation is absorbed by the black-coated cavity and the induced different heat-flux between the primary and reference cavity is measured, and the electrically calibrated differential heat-flux is used to compute the solar irradiance. SIAR has three identical channels A, B, and C, and each channel has a different solar exposure time to study the instrument’s nonlinear drift due to degradation. DARA also has three cavity radiometers and electrical substitution radiometers (Channel A, Channel B, and Channel C). The difference is that they are aligned in a triangle. Compared to VIRGO/PMO6, DARA inverts the aperture geometry to eliminate stray light. DARA and SIAR absolute radiometers are not operating at the same time due to the different designs and measurement sequences. On August 18, 2021, both instruments successfully passed the first commission phase, and they started to observe the total solar irradiance since then.

How to cite: Ye, X., Zhu, P., Montillet, J.-P., Hu, X., Wang, J., Yang, D., Qi, J., Finsterle, W., Zhang, P., Fang, W., Koller, S., Pfiffner, D., Song, B., Luo, Z., Wang, K., Haberreiter, M., Wu, D., and Schmutz, W.: The first light from the joint total solar irradiance measurement experiment onboard the FY3-E meteorological satellite, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-17162, https://doi.org/10.5194/egusphere-egu23-17162, 2023.