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Possible problem with rotation equations in forces.c #86
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I'll let Matt comment on this, just one small thing: note that an inverse rotation is performed a few lines further down. |
I was just looking at this. You apparently are rotating x,y,z geocentric
equatorial coordinates to some
other coordinate frame. Davide told me that it should be the coordinates
defined by the moving position
of the polar axis of the earth with time so that the rotation should be
through very small angles in ra and dec
unless you;re integrating over thousands of years.
The accelerations are computed using the rotated x,y,z in that frame and
then the accelerations are
rotated back to equatorial coordinates. So I would expect that the
acceleration rotations should be through -a, -d
to get back to an equatorial coordinate frame if the first rotations for
x,y,z were through a, d. But the equations for
the accelerations clearly have a different structure than the rotations for
the coordinates. If this is not the case,
I'd really like an explanation of what is happening here.
Larry Wasserman
…On Sun, Jul 16, 2023 at 4:29 PM Hanno Rein ***@***.***> wrote:
I'll let Matt comment on this, just one small thing: note that an inverse
rotation is performed a few lines further down
<https://github.com/matthewholman/assist/blob/main/src/forces.c#L534C9-L534C14>
.
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Upon thinking about it, I'm not sure if my reply earlier this evening is
correct. So I will
retract that message until we sort out my original post which asks (1) Why
if the two
rotations ( a and d) are zero is the output x,y,z not identical to the
input x,y,z? and
(2) Why if you are correcting for the change in the obliquity of the axis
of the Earth
over time (a small amount) are you rotating through 90 degrees in Dec?
Larry
…On Sun, Jul 16, 2023 at 5:29 PM Hanno Rein ***@***.***> wrote:
I'll let Matt comment on this, just one small thing: note that an inverse
rotation is performed a few lines further down
<https://github.com/matthewholman/assist/blob/main/src/forces.c#L534C9-L534C14>
.
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I think I see a problem with the rotation equations in the J2,J3,J4 subroutine -- lines 492-495 in
forces.c.
For starters, assume the rotations were exactly zero in both ra and dec (ie no rotation at all).
I would think that you would expect that the rotation equations would yield:
dxp = dx
dyp = dy
dzp = dz
But if you set a=0 and d=0 with cosa=1, sina=0, cosd=1, sind=0 the equations give:
dxp = dy
dyp = dz
dzp = dx
which CAN'T be right and implies that the rotation equations are wrong.
Second, you're taking the value of a and d to be the actual RA and Dec of the Earth's pole (at J2000), ie 0
and 90 respectively and not the rotation angle of the pole from the J2000 position, both of which should both
be very small angles and are actually both zero if you want to fix things at J2000. But, you're effectively saying you want to
rotate the pole through 90 degrees in Dec and 0 degrees in RA.
And a very minor point, you calculate costheta2 = dz*dz/r2. But it's actually the sine of an angle, not
a cosine. And I think it's actually the sine of the "dec" of the object (but calculated from the non-light time corrected
positions).
Larry Wasserman
Lowell Observatory
[email protected]
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