PulseExploreJournal ClubDebatesTrendingResearchersJournals
Instagram
HomeExploreJournal ClubTrending
Synapse
⌘+K
Synapse
September 10, 2025The Astrophysical Journal0 citationsOpen Access

Characterizing the Solar High-Latitude Inertial Mode Observational Properties

Characterizing the Observational Properties of the Sun’s High-latitude m = 1 Inertial Mode

View Full Paper
Ask AI
Bookmark
Share

Authors

BDB. DingJZJunwei ZhaoRCRuizhu Chen

Discussion

Loading...

Member takes

Overview

Observational analysis reveals the m = 1 inertial mode exhibits significant power fluctuations in polar regions, indicating an intriguing link with solar activity.

Key Points

  • The power distribution of the m = 1 inertial mode is stronger in the northern polar region, highlighting a geographical influence on its properties.
  • Power of the m = 1 mode anticorrelates with solar activity, demonstrating persistence during solar minima and fragmentation during maxima.
  • Zonal and meridional phase velocities were computed, revealing less differential rotation in the mode compared to surrounding plasma.
  • Magnetic flux influences the mode's power and lifetime, enhancing its strength but reducing its persistence upon reaching high latitudes.

Cite This Study

Ding et al. (2025) studied this question.

synapsesocial.com/papers/68c1a91354b1d3bfb60e2681https://doi.org/10.3847/1538-4357/ade980
View Full Paper
Ask AI
Bookmark
Share

Also Consider

Synapse has enriched 2 closely related papers on similar clinical questions. Consider them for comparative context:

  1. 1Inertial Waves in a Nonlinear Simulation of the Sun's Convection Zone and Radiative Interior2024 · 13 citations
  2. 2The Sun’s differential rotation is controlled by high-latitude baroclinically unstable inertial modes2024 · 19 citations