Does ACE IMF Polarity Come from Bz Data?

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SUMMARY

The discussion centers on the relationship between ACE IMF polarity and Bz data, specifically questioning whether ACE IMF polarity is derived from Bz measurements. The ACE IMF data, represented by a solid black line, shows a negative polarity despite Bz data indicating 8 out of 9 positive values. The Wang-Sheeley-Arge model predictions, based on data from Wilcox, Mount Wilson, and SOLIS solar observatories, are also referenced for comparison. The conclusion drawn is that discrepancies exist between ACE measurements and Bz data, warranting further investigation into the source of ACE IMF polarity.

PREREQUISITES
  • Understanding of ACE (Advanced Composition Explorer) satellite data
  • Familiarity with Bz (magnetic field component) measurements
  • Knowledge of the Wang-Sheeley-Arge model for solar wind predictions
  • Basic concepts of solar physics and interplanetary magnetic fields
NEXT STEPS
  • Research the methodology behind ACE IMF data collection and analysis
  • Explore the implications of Bz measurements on solar wind dynamics
  • Investigate the Wang-Sheeley-Arge model and its predictive capabilities
  • Examine case studies of ACE IMF polarity discrepancies with Bz data
USEFUL FOR

Astronomers, space weather researchers, and solar physicists interested in the dynamics of interplanetary magnetic fields and their implications for solar wind behavior.

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IMFQuestions_zpsa7a89988.jpg


IMF Polarity Predictions:
Comparison of real-time ACE IMF polarity data (solid black line) with Wang-Sheeley-Arge model predictions (colored dots). The three sets of predictions (i.e., red, green, and blue dots) are based on data from, respectively, Wilcox (WSO), Mount Wilson (MWO) and SOLIS (NSO) solar observatories. The solid black line is the real-time (9-hour-averaged) ACE IMF values normalized to equal unit value. A positive (negative) polarity indicates that the IMF is directed radially outward (inward) from the Sun to the Earth. Each 9-hour interval of real-time ACE data corresponds to 9 individual (hourly averaged) values when there are no gaps in coverage. If two-thirds of the 9 values have positive (negative) sign, they are assigned a polarity of +1 (-1). If less than two-thirds are of a particular sign, that time interval is assigned a polarity of zero, implying mixed or indeterminate polarity. Source : http://www.swpc.noaa.gov/ws/predimf_3d.html


Referring to above image, based on data from Bz, 8 out of 9 numbers are positive polarity, but ACE shows negative polarity, I would like to confirm whether ACE IMF polarity come from data of Bz or not.

Does anyone have any suggestions?

Thanks in advance for any suggestions :>
 
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