bump version to 3.9.4

japhir · May 29, 2024 · 3217c35 · 3217c35
1 parent 699aea4
commit 3217c35
Show file tree

Hide file tree

Showing 5 changed files with 6 additions and 6 deletions.
diff --git a/CITATION.cff b/CITATION.cff
@@ -44,8 +44,8 @@ keywords:
   - earth sciences
   - marine sciences
 license: GPL-3.0-or-later
-version: 3.9.3
-date-released: '2024-04-24'
+version: 3.9.4
+date-released: '2024-05-28'
 references:
 - authors:
   - family-names: Zeebe

diff --git a/DESCRIPTION b/DESCRIPTION
@@ -1,6 +1,6 @@
 Package: snvecR
 Title: Calculate Earth’s Obliquity and Precession in the Past
-Version: 3.9.3.9000
+Version: 3.9.4
 Authors@R:
     c(person("Ilja", "Kocken", , "ikocken@hawaii.edu", role = c("aut", "cre", "trl", "cph"),
              comment = c(ORCID = "0000-0003-2196-8718")),

diff --git a/NEWS.md b/NEWS.md
@@ -1,4 +1,4 @@
-# snvecR (development version)
+# snvecR 3.9.4
 
 # snvecR 3.9.3
 * Added a package option for the cache directory.

diff --git a/inst/CITATION b/inst/CITATION
@@ -11,7 +11,7 @@ bibentry(
   ## journal = "CRAN / JOSS??",
   year = "2023",
   abstract = "Easily calculate precession and obliquity from an astronomical solution (defaults to ZB18a from Zeebe and Lourens (2019)) and assumed or reconstructed values for tidal dissipation (Td) and dynamical ellipticity (Ed). This is a translation and adaptation of the 'C'-code in the supplementary material to Zeebe and Lourens (2022), with further details on the methodology described in Zeebe (2022). The name of the 'C'-routine is 'snvec', which refers to the key units of computation: spin vector s and orbit normal vector n.",
-  version = "3.9.3",
+  version = "3.9.4",
   ## volume = {n/a},
   ## number = {n/a},
   ## pages = {},

diff --git a/tests/testthat/test-get_solution.R b/tests/testthat/test-get_solution.R
@@ -1,6 +1,6 @@
 test_that("get_solution() inputs are checked", {
   pth <- withr::local_tempdir(pattern = "snvecR")
-  withr::local_options(list(snvecR.cachedir = pth, width = 150))
+  withr::local_options(list(snvecR.cachedir = pth))
   expect_error(get_solution(astronomical_solution = "hoi"))
   expect_error(get_solution(astronomical_solution = "full-La11"))
   expect_error(get_solution(astronomical_solution = data.frame(x = 1, y = 5))) # this runs via prepare_solution