RAM‐SCB Runs on Request at CCMC
Abstract The Ring current–Atmosphere interactions Model (RAM) with Self‐Consistent magnetic (B) field (SCB) combines a large‐scale kinetic model of ring current plasma with a three‐dimensional (3‐D) force‐balanced model of the terrestrial magnetic field. RAM‐SCB simulates the evolution of major ion...
Saved in:
| Main Authors: | , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Wiley
2023-12-01
|
| Series: | Space Weather |
| Online Access: | https://doi.org/10.1029/2023SW003771 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1841536450305196032 |
|---|---|
| author | Steven K. Morley Vania K. Jordanova Yihua Zheng Maksym Petrenko |
| author_facet | Steven K. Morley Vania K. Jordanova Yihua Zheng Maksym Petrenko |
| author_sort | Steven K. Morley |
| collection | DOAJ |
| description | Abstract The Ring current–Atmosphere interactions Model (RAM) with Self‐Consistent magnetic (B) field (SCB) combines a large‐scale kinetic model of ring current plasma with a three‐dimensional (3‐D) force‐balanced model of the terrestrial magnetic field. RAM‐SCB simulates the evolution of major ion species (H+, O+, and He+ by default) and electrons as a function of azimuth, radial distance, energy, and pitch angle. Simulation outputs include the Dst index, and pressure and differential flux of the modeled species, thus providing benefit as a science code and to inform surface charging hazard within the model domain. Version 2.2 of this open‐source simulation code has now—as of 8 August 2023—been made available for Runs‐On‐Request via the Community Coordinated Modeling Center. |
| format | Article |
| id | doaj-art-ef5ff2b6143e41f0b9e54214f3b6e39f |
| institution | Kabale University |
| issn | 1542-7390 |
| language | English |
| publishDate | 2023-12-01 |
| publisher | Wiley |
| record_format | Article |
| series | Space Weather |
| spelling | doaj-art-ef5ff2b6143e41f0b9e54214f3b6e39f2025-01-14T16:30:45ZengWileySpace Weather1542-73902023-12-012112n/an/a10.1029/2023SW003771RAM‐SCB Runs on Request at CCMCSteven K. Morley0Vania K. Jordanova1Yihua Zheng2Maksym Petrenko3Space Science and Applications Los Alamos National Laboratory Los Alamos NM USASpace Science and Applications Los Alamos National Laboratory Los Alamos NM USACommunity Coordinated Modeling Center NASA Goddard Space Flight Center Greenbelt MD USACommunity Coordinated Modeling Center NASA Goddard Space Flight Center Greenbelt MD USAAbstract The Ring current–Atmosphere interactions Model (RAM) with Self‐Consistent magnetic (B) field (SCB) combines a large‐scale kinetic model of ring current plasma with a three‐dimensional (3‐D) force‐balanced model of the terrestrial magnetic field. RAM‐SCB simulates the evolution of major ion species (H+, O+, and He+ by default) and electrons as a function of azimuth, radial distance, energy, and pitch angle. Simulation outputs include the Dst index, and pressure and differential flux of the modeled species, thus providing benefit as a science code and to inform surface charging hazard within the model domain. Version 2.2 of this open‐source simulation code has now—as of 8 August 2023—been made available for Runs‐On‐Request via the Community Coordinated Modeling Center.https://doi.org/10.1029/2023SW003771 |
| spellingShingle | Steven K. Morley Vania K. Jordanova Yihua Zheng Maksym Petrenko RAM‐SCB Runs on Request at CCMC Space Weather |
| title | RAM‐SCB Runs on Request at CCMC |
| title_full | RAM‐SCB Runs on Request at CCMC |
| title_fullStr | RAM‐SCB Runs on Request at CCMC |
| title_full_unstemmed | RAM‐SCB Runs on Request at CCMC |
| title_short | RAM‐SCB Runs on Request at CCMC |
| title_sort | ram scb runs on request at ccmc |
| url | https://doi.org/10.1029/2023SW003771 |
| work_keys_str_mv | AT stevenkmorley ramscbrunsonrequestatccmc AT vaniakjordanova ramscbrunsonrequestatccmc AT yihuazheng ramscbrunsonrequestatccmc AT maksympetrenko ramscbrunsonrequestatccmc |