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Supplementary data for "BepiColombo mission confirms stagnation region of Venus and reveals its large extent"

<p>Dataset of the data presented in the figures of Persson et al. (2022), Nature Communications, &quot;BepiColombo mission confirms stagnation region of Venus and reveals its large extent&quot;. https://doi.org/10.1038/s41467-022-35061-3</p> <p>Full author team:</p> <p>M. Persson<sup>1</sup>*, S. Aizawa<sup>1</sup>, N. Andr&eacute;<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. G&eacute;not<sup>1</sup>,&nbsp;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>,&nbsp;G. Murakami<sup>3</sup></p> <p><sup>1</sup>Institut de Recherche en Astrophysique et Plan&eacute;tologie, Centre National de la Recherche Scientifique, Universit&eacute; Paul Sabatier - Toulouse III, Centre National d&rsquo;Etudes Spatiales, Toulouse, France</p> <p><sup>2</sup>Swedish Institute of Space Physics, Kiruna, Sweden</p> <p><sup>3</sup>Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan</p> <p><sup>4</sup>Department of Geophysics, Graduate School of Science, Kyoto University, Kyoto, Japan</p> <p><sup>5</sup>Institute for Geophysics and Extraterrestrial Physics, Technische Universit&auml;t Braunschweig, Braunschweig, Germany</p> <p><sup>6</sup>Institute of Space Astrophysics and Planetology, Istituto Nazionale di Astrofisica, Rome, Italy</p> <p><sup>7</sup>Laboratoire de Physique des Plasmas (LPP), Centre National de la Recherche Scientifique, Observatoire de Paris, Sorbonne Universit&eacute;, Universit&eacute; Paris Saclay, &Eacute;cole Polytechnique, Institut Polytechnique de Paris</p> <p><sup>8</sup>Space Research Institute, Austrian Academy of Sciences, Graz, Austria</p> <p><sup>9</sup>National Aeronautic and Space Administration, Goddard Space Flight Center, Greenbelt, Maryland, USA</p> <p><sup>10</sup>School of Physics and Astronomy, University of Leicester, Leicester, UK</p> <p><sup>11</sup>Department of Earth and Space Science, Graduate School of Science, Osaka University, Japan</p> <p><sup>12</sup>Max-Planck-Institute for Solar System Research, G&ouml;ttingen, Germany</p> <p><sup>13</sup>Laboratoire Atmosph&egrave;res, Milieux, Observations Spatiales, Institut Pierre Simon Laplace, Universit&eacute; Versailles Saint Quentin en Yvelines, Universit&eacute; Paris-Saclay, Universit&eacute; Pierre Marie Curie, Centre National de la Recherche Scientifique, Guyancourt, France</p> <p><sup>14</sup>Mullard Space Science Laboratory, University College London, Holmbury St. Mary, UK&nbsp;</p> <p><sup>15</sup>Imperial College London, South Kensington Campus, London, UK&nbsp;</p> <p><sup>16</sup>Graduate School of Natural Science and Technology, Kanazawa University, Kanazawa, Japan</p> <p>&nbsp;&nbsp;&nbsp;&nbsp; *Corresponding author. Email: <a href="mailto:moa.persson@irap.omp.eu">moa.persson@irap.omp.eu</a></p>

ShareScore

32/100

Overall dataset sharing score

Score breakdown

These five areas show where the dataset supports — or may limit — practical reuse.

Stewardship
4
Harmonization
4
Access
16
Reuse readiness
8
Engagement
0