star-line

Structure for accelerating line importance sampling
git clone git://git.meso-star.fr/star-line.git
Log | Files | Refs | README | LICENSE

commit b39671999e2ef3262b36a2cd26d2a648ff8e9ef6
parent 2f731318232214f5db6517480df548a4188a7117
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Tue, 10 Mar 2026 13:06:57 +0100

Correction of a typo in the sln-build manual page

Diffstat:
Mdoc/sln-build.1 | 4++--
1 file changed, 2 insertions(+), 2 deletions(-)

diff --git a/doc/sln-build.1 b/doc/sln-build.1 @@ -15,7 +15,7 @@ .\" .\" You should have received a copy of the GNU General Public License .\" along with this program. If not, see <http://www.gnu.org/licenses/>. -.Dd January 29, 2026 +.Dd March 10, 2026 .Dt SLN-BUILD 1 .Os .\"""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""" @@ -137,7 +137,7 @@ temperature of 292 K. Use the default options to mesh the spectrum, so that the resulting structure represents an upper bound on the spectral data: .Bd -literal -offset Ds -sln-build -P 1 -T 292 -o H2O_0-50_HITAMP2010_tree.bin \e +sln-build -P 1 -T 292 -o H2O_0-50_HITEMP2010_tree.bin \e -m /path/to/hitran/molparams.txt -x mixture.txt \e /path/to/hitran//H2O/01_0-50_HITEMP2010.par .Ed