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Orbital, Latitudinal, and Diurnal Variations in Meteoroid Influx, Atmospheric Ablation and Ionization, and Micrometeorite Accretion at Venus

  • Authors: Juan Diego Carrillo-Sánchez, Diego Janches, John M. C. Plane, Petr Pokorný

Juan Diego Carrillo-Sánchez et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure A4.

Orbital and latitudinally averaged total injection rates of ablated Na (Figure A4(a)) and Fe (Figure A4(b)) for different relative mass contributions of the HTCs and the OCCs: 26.7% HTC and 73.3% OCC (in blue); 50% HTC and 50% OCC (in orange); 75% HTC and 25% OCC (in black); and 86.1% HTC and 13.9% OCC (in red). The panels also show the fraction of Na and Fe ablated above 125 km altitude for different relative contributions of HTCs and OCCs.

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