Update tmd_nodal.m

Updates in response to Issue #19.
chadagreene · Feb 6, 2024 · e51f393 · e51f393
1 parent 45b0f7b
commit e51f393
Showing 1 changed file with 3 additions and 2 deletions.
diff --git a/tmd_nodal.m b/tmd_nodal.m
@@ -14,8 +14,9 @@
 % [pu,pf] = tmd_nodal(constituents,p,N) takes input constituents 
 % as cell array (1xN constituents). Inputs p and N are the lunar perigee p 
 % and ascending lunar node N given by the tmd_astrol function, and are 
-% dimesnions Mx1, with one row per timestep. Nodal correction outputs pu,pf are MxN,
-% corresponding to M timesteps and N constituents. 
+% dimesnions Mx1, with one row per timestep. Nodal correction outputs pu,pf 
+% have units of radians and are are MxN dimensions, corresponding to M 
+% timesteps and N constituents. 
 % 
 %% Author Info
 % This function is part of the Tide Model Driver (TMD), which was written by Lana Erofeeva