From e70d0ddf83609c41064ef81ea33dcbb01e34e0df Mon Sep 17 00:00:00 2001 From: anand43 Date: Fri, 1 Mar 2024 14:54:39 -0500 Subject: [PATCH] Minor restructuring --- docs/user-guide/gravitational-harmonics/index.rst | 6 +++--- 1 file changed, 3 insertions(+), 3 deletions(-) diff --git a/docs/user-guide/gravitational-harmonics/index.rst b/docs/user-guide/gravitational-harmonics/index.rst index 5f1505677..abc739a48 100644 --- a/docs/user-guide/gravitational-harmonics/index.rst +++ b/docs/user-guide/gravitational-harmonics/index.rst @@ -59,13 +59,13 @@ manner. Here we use Chariklo as an example body and refer to Jacobi Ellipsoid mo cb_T_rotation/= 24.0 # converting to julian days (TU) cb_rot = [[0, 0, 360.0 / cb_T_rotation]] # degrees/TU -Once the central body parameters are defined, we can compute the gravitational harmonics coefficients (:math:`C_{lm}`). Here we set the -reference radius flag to `True` and ask the function to return the reference radius. More in the additional capabilities section below. +Once the central body parameters are defined, we can compute the gravitational harmonics coefficients (:math:`C_{lm}`). The output coefficients are already correctly normalized. :: c_lm, cb_radius = swiftest.clm_from_ellipsoid(mass = cb_mass, density = cb_density, a = cb_a, b = cb_b, c = cb_c, lref_radius = True) -*Note: The maximum degree is set to 6 by default to ensure computational efficiency.* +*Note: Here we set the reference radius flag to `True` and ask the function to return the reference radius. More in the +additional capabilities section below. The maximum degree is set to 6 by default to ensure computational efficiency.* Add the central body to the simulation along with the coefficients. ::