Hemispheric Geomagnetic Activity Dependence on IMF By: Evidence from the Satellite and Pre-Satellite Eras

Abstract The sign of the interplanetary magnetic field (IMF) \((B_y)\) is known toproduce hemispheric asymmetries in the coupled magnetosphere--ionospheresystem, but its long-term signature in hemispheric geomagnetic activityis less well established. We investigate whether IMF polarity organizesthe distribution of geomagnetic activity between the Northern andSouthern Hemispheres independently of the overall activity level.Homogeneous hemispheric \((aa)\) indices are analyzed using directlymeasured IMF \((B_y)\) during 1965--2010 and reconstructed IMF sectorpolarity extending back to 1868. Positive- and negative-\((B_y)\) days arefirst compared after matching them within 5-nT bins of overallgeomagnetic activity. As an independent control, the \((B_y)\) dependenceis estimated while accounting directly for southward IMF, solar-windspeed, and long-term variations. A systematic \((B_y)\)-dependent hemispheric asymmetry remains under bothcontrol approaches, with the most consistent positive differences between \((B_y>0)\) and \((B_y<0)\) conditions occurring in May, June, and October.The seasonal organization of this hemispheric effect differs markedlyfrom the corresponding \((B_y)\) dependence of overall geomagneticactivity. The latter is dominated by an annual component with aspring--autumn reversal, whereas the activity-matched hemisphericcontrast is dominated by a semiannual component with fitted maximanear May and November. Thus, the hemispheric dependence is not simplya scaled representation of the polarity-dependent seasonal modulationof total geomagnetic activity. Reconstructed IMF sector polarity shows that the principal seasonalfeatures of the activity-matched hemispheric contrast were alreadypresent during 1868--1964 and recur in the satellite-era reconstruction.The results suggest that IMF \((B_y)\) provides a persistent organizationof the hemispheric distribution of geomagnetic activity, superposed onthe better-known polarity-dependent modulation of overall geomagneticactivity.

Authors

Publication Details

Journal
Research Square
Published
2026-11-03
DOI
https://doi.org/10.21203/rs.3.rs-11360911/v1
Primary Topic
Ionosphere and magnetosphere dynamics
Type
preprint
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
preprint

Hemispheric Geomagnetic Activity Dependence on IMF By: Evidence from the Satellite and Pre-Satellite Eras

Jouni Takalo
Research Square
Ionosphere and magnetosphere dynamics
preprint

Hemispheric Geomagnetic Activity Dependence on IMF By: Evidence from the Satellite and Pre-Satellite Eras

Jouni Takalo
preprint en

Abstract

Abstract The sign of the interplanetary magnetic field (IMF) \((B_y)\) is known toproduce hemispheric asymmetries in the coupled magnetosphere--ionospheresystem, but its long-term signature in hemispheric geomagnetic activityis less well established. We investigate whether IMF polarity organizesthe distribution of geomagnetic activity between the Northern andSouthern Hemispheres independently of the overall activity level.Homogeneous hemispheric \((aa)\) indices are analyzed using directlymeasured IMF \((B_y)\) during 1965--2010 and reconstructed IMF sectorpolarity extending back to 1868. Positive- and negative-\((B_y)\) days arefirst compared after matching them within 5-nT bins of overallgeomagnetic activity. As an independent control, the \((B_y)\) dependenceis estimated while accounting directly for southward IMF, solar-windspeed, and long-term variations. A systematic \((B_y)\)-dependent hemispheric asymmetry remains under bothcontrol approaches, with the most consistent positive differences between \((B_y>0)\) and \((B_y<0)\) conditions occurring in May, June, and October.The seasonal organization of this hemispheric effect differs markedlyfrom the corresponding \((B_y)\) dependence of overall geomagneticactivity. The latter is dominated by an annual component with aspring--autumn reversal, whereas the activity-matched hemisphericcontrast is dominated by a semiannual component with fitted maximanear May and November. Thus, the hemispheric dependence is not simplya scaled representation of the polarity-dependent seasonal modulationof total geomagnetic activity. Reconstructed IMF sector polarity shows that the principal seasonalfeatures of the activity-matched hemispheric contrast were alreadypresent during 1868--1964 and recur in the satellite-era reconstruction.The results suggest that IMF \((B_y)\) provides a persistent organizationof the hemispheric distribution of geomagnetic activity, superposed onthe better-known polarity-dependent modulation of overall geomagneticactivity.

Research Square
Ionosphere and magnetosphere dynamics
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Laika access coming soon
Hemispheric Geomagnetic Activity Dependence on IMF By: Evidence from the Satellite and Pre-Satellite Eras — Jouni Takalo · Research Square (2026) | TGRS Research Map | TGRS