Prediction of coronal and heliospheric magnetic fields: the promise of SOI-MDI on SOHO.

Details Prediction of coronal and heliospheric magnetic fields: the promise of SOI-MDI on SOHO. Prediction of coronal and heliospheric magnetic fields: the promise of SOI-MDI on SOHO.

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382...76h&link_type=abstract

AIP Conf. Proc., No. 382, p. 76 - 79

Computer Science

Solar Corona: Magnetic Fields, Solar Corona: Structure

Scientific paper

Coronal magnetic field models reproduce the static characteristics of coronal and heliospheric structures fairly well; however, limitations of spatial and temporal resolution and nonuniform quality of the input data are important factors limiting investigations of the response of the corona to rapidly changing photospheric conditions. The Solar Oscillations Investigation (SOI) Michelson Doppler Imager (MDI) experiment on SOHO produces a series of full-disk photospheric magnetic field observations with 4″resolution about every 96 minutes for the next several years. To suggest the potential of the MDI photospheric magnetic field data, the authors show calculations of the steady coronal magnetic field using low spatial resolution data and compare results with various observations.

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