Reference:Reference-024924: Difference between revisions
From CSDMS
m Text replacement - " |CorpusID=" to " |CorpusID=" |
Tag: Undo |
||
| Line 16: | Line 16: | ||
|PublicationClusterID=0 | |PublicationClusterID=0 | ||
|MS_PublicationClusterID=0 | |MS_PublicationClusterID=0 | ||
|Semantic_ID=27b9b8b1a1aa6dea377bf78d8b41d61dc9a013de | |Semantic_ID=27b9b8b1a1aa6dea377bf78d8b41d61dc9a013de |CorpusID=251033565 | ||
|CorpusID=251033565 | |||
|PublicationWhatKindOf=a module application description | |PublicationWhatKindOf=a module application description | ||
|PublicationNrofModels=a single module | |PublicationNrofModels=a single module | ||
Revision as of 18:08, 6 October 2024
| Author(s) | Yang, Qike; Wu, Xiaoqing; Wang, Zhiyuan; Hu, Xiaodan; Guo, Yiming; Qing, Chun; |
| BibType | journalArticle |
| Title | Simulating the night-time astronomical seeing at Dome A using Polar WRF |
| Editors | |
| Year | 2022-07-26 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Booktitle | None |
| Volume | 515 |
| Pages | 1788–1794 |
| URL | https://academic.oup.com/mnras/article/515/2/1788/6648816 |
| DOI | 10.1093/mnras/stac1930 |
| ISBN | |
| Note | Auto downloaded ref at: 2024-09-04
|
| |
|
| Feature reference | No |
| PublicationClusterID | 0 |
| MS_PublicationClusterID | 0 |
| Semantic_ID | 27b9b8b1a1aa6dea377bf78d8b41d61dc9a013de |
| Nr of citations | 3 |
| Sort of publication | a module application description |
| Sort of model publication | a single module |
| Is the CSDMS HPC used | No |
| If HPC is used, for what project was it?: | |
| Associated simulation movie if any: |
|
| Model(s) discussed: | WRF
|
