"observation range" is a correct and usable phrase in written English.
It refers to the distance or area in which something can be observed or seen. You can use it in a sentence like: "The ranger pointed out the wildlife within our observation range." A definition for this phrase can be found in a dictionary or online, such as in the Merriam-Webster dictionary: https://www.merriam-webster.com/dictionary/observation%20range.
Additionally, the involved network congestion and contention dynamics are presented, while the effects of observation range, speed, time intervals between observations, and odometry readings on the SLAM accuracy are shown based on an extensive set of simulation studies.
All foot and ankle examinations should include a thorough inspection, gait observation, range of motion and neurovascular examination.
In the case of the ground-based DITF, with an observation range of around a hundred and several tens of kilometers, the dynamic range is given more importance than the gain.
On the other hand, in case of Peg-in-Hole manipulation, the number of positive and negative responses varied for the same statement regarding to the observation range: 40% negative, 30% neutral and 30% positive.
Since the tiltmeter was designed to measure tiny tilt changes such as from earth tides (approximately 10−7 radians), the observation range was not sufficient to measure such a huge ground tilt near the fault.
The neutral atmospheric effect in InSAR is a difference of two acquisition time (phi_{text{NA}} = phi_{text{NA}}^{text{slave}} - phi_{text{NA}}^{text{master}}), and (phi_{text{NA}}) primarily reflects water vapor heterogeneity in the troposphere because the effect of dry air is spatially homogeneous in a typical InSAR observation range (Zebker et al. 1997).
The pH during the observation ranged 6 7.8.
The GPS rovers (Promark3) in the field were set at the inundation limit and measured up to the observation ranges from the location of the base site of the Proflex500.
After eight months of observation ranging from May 2009 to January 2010, the Kepler team established Kepler-10b as the first rocky exoplanet discovered by the Kepler satellite.
Quarterly HH compliance rates by direct observation ranged from 92 to 99%.
The period of observation ranged from 0.5 to 41 years with a mean of 17 years.
