Zobrazeno 1 - 8
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pro vyhledávání: '"Garton, Tadhg M."'
Autor:
Garton, Tadhg M., Jackman, Caitriona M., Smith, Andy W., Yeakel, Kiley L., Maloney, Shane A., Vandegriff, Jon
Publikováno v:
Frontiers in Astronomy and Space Science, 2021
The products of magnetic reconnection in Saturn's magnetotail are identified in magnetometer observations primarily through characteristic deviations in the north-south component of the magnetic field. These magnetic deflections are caused by travell
Externí odkaz:
http://arxiv.org/abs/2104.00496
Autor:
Reiss, Martin A., Muglach, Karin, Möstl, Christian, Arge, Charles N., Bailey, Rachel, Delouille, Veronique, Garton, Tadhg M., Hamada, Amr, Hofmeister, Stefan, Illarionov, Egor, Jarolim, Robert, Kirk, Michael S. F., Kosovichev, Alexander, Krista, Larisza, Lee, Sangwoo, Lowder, Chris, MacNeice, Peter J., Veronig, Astrid, Team, ISWAT Coronal Hole Boundary Working
Coronal holes are the observational manifestation of the solar magnetic field open to the heliosphere and are of pivotal importance for our understanding of the origin and acceleration of the solar wind. Observations from space missions such as the S
Externí odkaz:
http://arxiv.org/abs/2103.14403
Autor:
Azari, Abigail R., Biersteker, John B., Dewey, Ryan M., Doran, Gary, Forsberg, Emily J., Harris, Camilla D. K., Kerner, Hannah R., Skinner, Katherine A., Smith, Andy W., Amini, Rashied, Cambioni, Saverio, Da Poian, Victoria, Garton, Tadhg M., Himes, Michael D., Millholland, Sarah, Ruhunusiri, Suranga
Machine learning (ML) methods can expand our ability to construct, and draw insight from large datasets. Despite the increasing volume of planetary observations, our field has seen few applications of ML in comparison to other sciences. To support th
Externí odkaz:
http://arxiv.org/abs/2007.15129
Coronal holes (CHs) are regions of open magnetic flux which are the source of high speed solar wind (HSSW) streams. To date, it is not clear which aspects of CHs are of most influence on the properties of the solar wind as it expands through the Heli
Externí odkaz:
http://arxiv.org/abs/1811.11605
Publikováno v:
J. Space Weather Space Clim., 8 (2018) A02
Coronal holes (CH) are regions of open magnetic fields that appear as dark areas in the solar corona due to their low density and temperature compared to the surrounding quiet corona. To date, accurate identification and segmentation of CHs has been
Externí odkaz:
http://arxiv.org/abs/1711.11476
Akademický článek
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Publikováno v:
Journal of Space Weather and Space Climate, Vol 8, p A02 (2018)
Coronal holes (CH) are regions of open magnetic fields that appear as dark areas in the solar corona due to their low density and temperature compared to the surrounding quiet corona. To date, accurate identification and segmentation of CHs has been
Externí odkaz:
https://doaj.org/article/550ca82df14048dbbd30c34b3954c85c
Akademický článek
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