Published November 28, 2023 | Version v1

ADAPT Global Solar Magnetic Maps - 2010 Sep 18-20 (w/ & w/o farside active region input)

  • 1. ROR icon United States Air Force Research Laboratory

Description

ADAPT (Air Force Data Assimilative Photospheric flux Transport) model global solar magnetic maps using HMI magnetograms with ("wfar") and without ("orig") estimated farside active region flux, for the 3  day period: September 18-20, 2010.  The farside emergence of NOAA AR11109 (approximately on 18sep2010, based on STEREO observations of farside) is estimated by modeling the HMI vector observation on the east-limb (i.e., at a CMD of approximately -61.5 degrees) back ~6 days. 

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Additional details

References

  • Arge, C.N., Henney, C.J., Koller, J., Compeau, C.R., Young, S., MacKenzie, D., Fay, A., Harvey, J.W. 2010, in Solar Wind 12, AIP Conf. Series, 1216, 343; https://doi.org/10.1063/1.3395870
  • Arge, C. N., Henney, C. J., Gonzales-Hernandez, I., Toussaint, W.A., Koller, J., and Godinez, H. C.: Modeling the corona and solar wind using ADAPT maps that include far side observations, in Solar Wind 13, AIP Conf. Series, 1539, 11-14, 2013; https://doi.org/10.1063/1.4810977.
  • Barnes, G., DeRosa, M. L., Jones, S. I., Arge, C. N., Henney, C. J., Cheung, M. C., Implications of Different Solar Photospheric Flux-Transport Models for Global Coronal and Heliospheric Modeling, ApJ, 946, 105, 2023; https://doi.org/10.3847/1538-4357/acba8e
  • Hickmann, K., S., Godinez, H. C., Henney, C. J., Arge, C. N., Data Assimilation in the ADAPT Photospheric Flux Transport Model, Solar Physics, 290, 1105-1118, 2015, https://doi.org/10.1007/s11207-015-0666-3.