Trying to get an explicit function(ish)

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Pencilvester
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How would I go about solving for ##t_p## in the following equation:$$t_p - t + vy \cos {(2 \pi \omega t_p )} - vx \sin {(2 \pi \omega t_p )} = 0$$where our input is a point in ##ℝ^3## with coordinates ##t##, ##x##, and ##y##, and where ##v## and ##\omega## are constants. I’m pretty sure it can’t be a function exactly, as I’m pretty sure most, if not all input points will each yield 2 distinct outputs. If it matters to you, ##|v| < 1##, but I don’t think that it’s relevant to this problem. And this isn’t any kind of homework problem. I’m not in school, I’m just trying to analyze what a coordinate transformation might look like for going from coordinates of an inertial observer in flat spacetime to coordinates of an observer tracing out a helix in spacetime (or a circle in space), and I’m running into this limitation in my mathematical abilities, so any help would be much appreciated.
 
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In general there is no closed solution - you can only find approximations. It is possible to combine the cosine and sine term to a single sine (or cosine) with an additional phase, that makes the problem a bit easier to look at. tp cannot be too different from t as the other terms cannot get larger than vx or vy, respectively, this gives you a region to look for solutions. Once you found a tp that is not too far away from a solution tools like Newton's method will work.
 
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mfb said:
In general there is no closed solution - you can only find approximations. It is possible to combine the cosine and sine term to a single sine (or cosine) with an additional phase, that makes the problem a bit easier to look at. tp cannot be too different from t as the other terms cannot get larger than vx or vy, respectively, this gives you a region to look for solutions. Once you found a tp that is not too far away from a solution tools like Newton's method will work.
Dang. That’s dissatisfying for me. Well at least I didn’t spend much time trying to find a general solution before posting this. Thanks!