Venusian bow shock crossings manually identified from measurements by the ASPERA-4 and MAG instruments onboard Venus Express
Authors/Creators
- 1. IRAP, CNRS-UPS-CNES, Toulouse, France; GSFS, The University of Tokyo, Kashiwa, Japan
- 2. Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo, Tokyo, Japan
- 3. IRAP, CNRS-UPS-CNES, Toulouse, France; Institut Supérieur de l'Aéronautique et de l'Espace, Supaero, Université de Toulouse, Toulouse Cedex, France
- 4. Luleå University of Technology, Kiruna, Sweden
- 5. Swedish Institute of Space Physics, Kiruna, Sweden
Description
Bow shock crossings at Venus identified manually from the ASPERA-4 and MAG instruments onboard Venus Express for the full mission from 2006 to 2014.
A detailed description of the dataset can be found in the paper "Influence of solar wind variations on the shapes of Venus’ plasma boundaries based on Venus Express observations" by Signoles et al.
The boundary crossings by Venus Express are determined from combining the measurements of both ion, electron and magnetic field measurements. The bow shock is identified from the sharp increase in the magnetic field magnitude, and the increase in electron and ion temperature. The ion composition boundary is identified from the decrease in magnetosheath protons and electrons, and the appearance of planetary heavy ions.
The dataset contains 5193 identified bow shock crossings and 2679 identified ion composition boundary crossings.
For more information on the dataset contact: M. Persson, moaperssonphd at gmail.com