diff --git a/README.md b/README.md index b163c5f0..a6fd8840 100644 --- a/README.md +++ b/README.md @@ -395,7 +395,8 @@ terms differently: See the various enums and constants defined in `novas.h`, as well as the descriptions on the various NOVAS routines on how they are appropriate for the old and new methodologies respectively. Figure 1 also shows the relation of the -various old and new coordinate systems and the (Super)NOVAS functions for converting among them. +various old and new coordinate systems and the (Super)NOVAS functions for converting position / velocity vectors among +them. In NOVAS, the barycentric BCRS and the geocentric GCRS systems are effectively synonymous to ICRS, since the origin for positions and for velocities, in any reference system, is determined by the `observer` location, while aberration diff --git a/resources/SuperNOVAS-systems.dia b/resources/SuperNOVAS-systems.dia index d9215d51..67a531ed 100644 Binary files a/resources/SuperNOVAS-systems.dia and b/resources/SuperNOVAS-systems.dia differ diff --git a/resources/SuperNOVAS-systems.png b/resources/SuperNOVAS-systems.png index f28e9b5f..f708c90e 100644 Binary files a/resources/SuperNOVAS-systems.png and b/resources/SuperNOVAS-systems.png differ