no code implementations • 5 Feb 2021 • L. L. Zhao, G. P. Zank, J. S. He, D. Telloni, Q. Hu, G. Li, M. Nakanotani, L. Adhikari, E. K. J. Kilpua, T. S. Horbury, H. O'Brien, V. Evans, V. Angelini
We focus on the transmission of the magnetic fluctuations across the shock and analyze the characteristic wave modes of solar wind turbulence near the shock observed by both spacecraft.
Space Physics Solar and Stellar Astrophysics
no code implementations • 26 Oct 2020 • L. L. Zhao, D. W. Hogg, M. Bedell, D. A. Fischer
It is designed with the needs of extreme-precision radial velocity (EPRV) in mind, which require that instruments be calibrated or stabilized to better than $10^{-4}$ pixels.
Instrumentation and Methods for Astrophysics Earth and Planetary Astrophysics
