Phizicist said:
I'm not sure how to post in the correct forum. Please advise.
Welcome to PF.
You will get the hang of it.
I think the idea in this thread is to actually measure the Earth's tide, at a fixed base station, over a long period of time. That is certainly a challenge, but it is possible. When we measure gravity at a fixed station, we are effectively measuring the changing distance from the centre of the Earth underfoot, and so to detect the changing elliptical equatorial profile, which is the Earth tide.
The Earth's orbital plane about the Sun is not parallel with the Earth's Equatorial plane, which is different again to the Moon's orbital plane about the Earth. So the Earth tide is the sum of Solar and Lunar terms, with asynchronous periods, and varying magnitudes. It is certainly easier to compute the Earth tide than it is to measure it. At least we can predict the pattern to look for in the data.
I don't think there is a budget to buy or rent a gravimeter, so it is a case of trying to identify a gravimeter that can be built on a budget by a practical person. By automating and logging data continuously at a fixed station it should be possible extract the Earth Tide from the recorded data.
As technology changes, different possibilities will rise and fall.
There is an article here from 2012 on the historical advances in gravimeters.
https://www.hindawi.com/journals/ijge/2012/687813/
I believe the three options, in order of complexity, are a pendulum, a spring balance, or a thrown mass. I don't think superconductive or atomic rubidium sensors are realistic for skilled amateurs on a budget, but I am open to suggestions.
Typical MEMS accelerometers do not have anywhere near the resolution needed to measure tides. But there is this article
small-and-inexpensive-mems-gravimeter. See the comments: “The Nature abstract and the summary here neglect to mention that the accelerometer, to function to the precision needed, must be in high vacuum and temperature controlled to within 1 milliKelvin. Do-able, but it’s not quite as simple as just a thin slab of silicon.”
The slope of the Earth's surface changes due to Earth tide, but by how much? Around the Earth's equator, there are two Earth tide highs, and two Earth tide lows. Those points at 90°, are about 10,000 km apart. The peak to peak change due to Earth Tide is about half a metre, which makes the amplitude of the elliptical deformation ±0.25 m. The slope is then 0.25 in 20e6/2Pi = 7.85e-8 radian = 0.016 arc sec. But the best theodolites and levels can only measure 0.2 arc sec.
Astronomical VLBI with 15 m precision dishes is only now being used to establish the base lines of continent-wide geodetic networks to a resolution of about 2 mm. That is now being used to correct GPS networks.
So, what other practical possibilities are there?