Air Force Data Assimilative Photospheric Flux Transport (ADAPT) Model
Abstract
As the primary input to coronal and solar wind models, global estimates of the solar photospheric magnetic field distribution are critical to space weather forecasting. These global magnetic maps are essential for accurate modeling of the corona and solar wind, which is vital for gaining the basic understanding necessary to improve forecasting models needed for Air Force operations. In this paper, we describe our efforts and progress toward developing the Air Force Data Assimilative Photospheric flux Transport (ADAPT) model. ADAPT incorporates the ensemble Kalman filter data assimilation technique with a photospheric magnetic flux transport model. The flux transport model evolves the magnetic flux on the Sun using relatively well understood transport processes when observations are not available and then updates the modeled flux with new observations using the ensemble Kalman filter. The data assimilation with the ensemble Kalman filter rigorously takes into account model and observational uncertainties, as well as accounting for regional correlations. Anticipated outcomes of the ADAPT model include improvement in: 1) the estimation of solar corona and polar fields. 2) understanding the nature and behavior of solar super granular diffusion and meridional flows over the solar cycle, and 3) modeling and forecasting the solar wind near Earth.
Document Details
- Document Type
- Technical Report
- Publication Date
- Mar 01, 2010
- Accession Number
- ADA515973
Entities
People
- Alex Fay
- C.r. Compeau
- Carl Henney
- Charles Arge
- David Mackenzie
- John W. Harvey
- Josef Koller
- Shawn Young
Organizations
- Air Force Research Laboratory