The phrase "observing stations" is grammatically correct and can be used in written English.
It refers to specific locations or facilities where systematic observations are made. Example: The meteorological department has set up several observing stations along the coast to monitor weather patterns and provide real-time reports to the public.
In addition, observations from the National Weather Service NWSS) Cooperative Observing Stations were used.
The higher E × B vertical drift in the 90 100°E sector and the large geographic-geomagnetic offset in observing stations may have contributed to the observed differences.
Remote sensing approaches were selected to harness its capability to provide spatially explicit account of ecosystem parameters (Xiaoming et al. 2010; Li et al. 2014) especially in places like Guna-Tana watershed where there is acute shortage of in situ based hydro-meteorological observations and complete absence of flux tower observing stations for ecosystem health modeling.
Systematic time biases are estimated against the UTC time scale for a set of 22 observing stations in 2013, in the range of zero to a few μs.
All the observing stations are identical, operated in a fully robotic manner, and controlled by the headquarters located in Daejeon, Korea.
The society, the pre-eminent scientific organization in colonial America, also set up observing stations in the yard next to the Pennsylvania Statehouse — now Independence Hall — and along the shores of what is now Delaware.
By the end of 2007 a simply constructed telescope with a larger field of view at Xinglong Observing Station was employed to carry out trial observations.
A real-time correlation solar observing system (RCSOS) has been finished recently at Huairou Solar Observing Station (HSOS) in National Astronomical Observatories of China (NAOC).
The methods were applied to photospheric vector magnetic field data of active region NOAA 9077, observed by the Huairou Solar Observing Station (HSOS) of the National Astronomical Observatories of China before and after the 'Bastille Day' flare on July 13th and 14th, 2000.
In the current work, the three measures of the length of strong-shear neutral line, total unsigned current, and total unsigned current helicity are computed from 1353 vector magnetograms observed at Huairou Solar Observing Station.
The Solar Magnetic Field Telescope (SMFT) at the Huairou Solar Observing Station of the National Astronomical Observatory has been obtaining photospheric vector magnetograms on a daily basis for more than 20 years.
