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pro vyhledávání: '"A, Takoudi"'
Autor:
E., Kardasis, J., Peralta, G., Maravelias, M., Imai, A., Wesley, T., Olivetti, Y., Naryzhniy, L., Morrone, A., Gallardo, G., Calapai, J., Camarena, P., Casquinha, D., Kananovich, N., MacNeill, C., Viladrich, A, Takoudi
Publikováno v:
Atmosphere 2022, 13(2), 348
Firstly identified in images from JAXA's orbiter Akatsuki, the cloud discontinuity of Venus is a planetary-scale phenomenon known to be recurrent since, at least, the 1980s. Interpreted as a new type of Kelvin wave, this disruption is associated to d
Externí odkaz:
http://arxiv.org/abs/2202.12601
Autor:
Emmanuel (Manos) Kardasis, Javier Peralta, Grigoris Maravelias, Masataka Imai, Anthony Wesley, Tiziano Olivetti, Yaroslav Naryzhniy, Luigi Morrone, Antonio Gallardo, Giovanni Calapai, Joaquin Camarena, Paulo Casquinha, Dzmitry Kananovich, Niall MacNeill, Christian Viladrich, Alexia Takoudi
Publikováno v:
Atmosphere, Vol 13, Iss 2, p 348 (2022)
Firstly identified in images from JAXA’s orbiter Akatsuki, the cloud discontinuity of Venus is a planetary-scale phenomenon known to be recurrent since, at least, the 1980s. Interpreted as a new type of Kelvin wave, this disruption is associated to
Externí odkaz:
https://doaj.org/article/66136f7d0e7f48ea89f5e55762c52f62
Autor:
Emmanouil Kardasis, Javier Peralta, Grigoris Maravelias, Masataka Imai, Anthony Wesley, Tiziano Olivetti, Yaroslav Naryzhniy, Luigi Morrone, Antonio Gallardo, Giovanni Calapai, Joaquin Camarena, Paulo Casquinha, Dzmitry Kananovich, Niall MacNeill, Christian Viladrich, Alexia Takoudi
The cloud discontinuity of Venus is a planetary-scale phenomenon known to be recurrent since, at least, the 1980s. It was initially identified in images from JAXA’s orbiter Akatsuki. This disruption is associated to dramatic changes in the clouds
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::92c6c3793563a44092c5aa08087f41f7
https://doi.org/10.5194/epsc2022-208
https://doi.org/10.5194/epsc2022-208
Akademický článek
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