DOI: 10.5281/zenodo.7851765
title: Supplementary data for "BepiColombo mission confirms stagnation region of Venus and reveals its large extent"

description: Dataset of the data presented in the figures of Persson et al. (2022), Nature Communications, "BepiColombo mission confirms stagnation region of Venus and reveals its large extent". https://doi.org/10.1038/s41467-022-35061-3 Full author team: M. Persson<sup>1</sup>*, S. Aizawa<sup>1</sup>, N. André<sup>1</sup>, S. Barabash<sup>2</sup>, Y. Saito<sup>3</sup>, Y. Harada<sup>4</sup>, D. Heyner<sup>5</sup>, S. Orsini<sup>6</sup>, A. Fedorov<sup>1</sup>, C. Mazelle<sup>1</sup>, Y. Futaana<sup>2</sup>, L.Z. Hadid<sup>7</sup>, M. Volwerk<sup>8</sup>, G. Collinson<sup>9</sup>, B. Sanchez-Cano<sup>10</sup>, A. Barthe<sup>1</sup>, E. Penou<sup>1</sup>, S. Yokota<sup>11</sup>, V. Génot<sup>1</sup>, J.A. Sauvaud<sup>1</sup>, D. Delcourt<sup>7</sup>, M. Fraenz<sup>12</sup>, R. Modolo<sup>13</sup>, A. Milillo<sup>6</sup>, H.-U. Auster<sup>5</sup>, I. Richter<sup>5</sup>, J.Z.D. Mieth<sup>5</sup>, P. Louarn<sup>1</sup>, C.J. Owen<sup>14</sup>, T.S. Horbury<sup>15</sup>, K. Asamura<sup>3</sup>, S. Matsuda<sup>16</sup>, H. Nilsson<sup>2</sup> M. Wieser<sup>2</sup>, T. Alberti<sup>6</sup>, A. Varsani<sup>8</sup>, V. Mangano<sup>6</sup>, A. Mura<sup>6</sup>, H. Lichtenegger<sup>8</sup>, G. Laky<sup>8</sup>, H. Jeszenszky<sup>8</sup>, K. Masunaga<sup>3</sup>, C. Signoles<sup>1</sup>, M. Rojo<sup>1</sup>, G. Murakami<sup>3</sup> <sup>1</sup>Institut de Recherche en Astrophysique et Planétologie, Centre National de la Recherche Scientifique, Université Paul Sabatier - Toulouse III, Centre National d’Etudes Spatiales, Toulouse, France <sup>2</sup>Swedish Institute of Space Physics, Kiruna, Sweden <sup>3</sup>Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan <sup>4</sup>Department of Geophysics, Graduate School of Science, Kyoto University, Kyoto, Japan <sup>5</sup>Institute for Geophysics and Extraterrestrial Physics, Technische Universität Braunschweig, Braunschweig, Germany <sup>6</sup>Institute of Space Astrophysics and Planetology, Istituto Nazionale di Astrofisica, Rome, Italy <sup>7</sup>Laboratoire de Physique des Plasmas (LPP), Centre National de la Recherche Scientifique, Observatoire de Paris, Sorbonne Université, Université Paris Saclay, École Polytechnique, Institut Polytechnique de Paris <sup>8</sup>Space Research Institute, Austrian Academy of Sciences, Graz, Austria <sup>9</sup>National Aeronautic and Space Administration, Goddard Space Flight Center, Greenbelt, Maryland, USA <sup>10</sup>School of Physics and Astronomy, University of Leicester, Leicester, UK <sup>11</sup>Department of Earth and Space Science, Graduate School of Science, Osaka University, Japan <sup>12</sup>Max-Planck-Institute for Solar System Research, Göttingen, Germany <sup>13</sup>Laboratoire Atmosphères, Milieux, Observations Spatiales, Institut Pierre Simon Laplace, Université Versailles Saint Quentin en Yvelines, Université Paris-Saclay, Université Pierre Marie Curie, Centre National de la Recherche Scientifique, Guyancourt, France <sup>14</sup>Mullard Space Science Laboratory, University College London, Holmbury St. Mary, UK <sup>15</sup>Imperial College London, South Kensington Campus, London, UK <sup>16</sup>Graduate School of Natural Science and Technology, Kanazawa University, Kanazawa, Japan *Corresponding author. Email: moa.persson@irap.omp.eu