Zobrazeno 1 - 10
of 22
pro vyhledávání: '"planetary ionosphere"'
Autor:
Pietro Franceschi, Daniele Catone, Daniela Ascenzi, Kevin C. Prince, Paolo Tosi, Stefano Turchini
Publikováno v:
Chemical physics
398 (2012): 269–277. doi:10.1016/j.chemphys.2011.06.009
info:cnr-pdr/source/autori:Daniela Ascenzi, Paolo Tosi, Pietro Franceschi, Daniele Catone, Stefano Turchini, Kevin C. Prince,/titolo:Chemical synthesis in acetonitrile containing discharges. Insights from photoionization experiments with synchrotron radiation/doi:10.1016%2Fj.chemphys.2011.06.009/rivista:Chemical physics (Print)/anno:2012/pagina_da:269/pagina_a:277/intervallo_pagine:269–277/volume:398
398 (2012): 269–277. doi:10.1016/j.chemphys.2011.06.009
info:cnr-pdr/source/autori:Daniela Ascenzi, Paolo Tosi, Pietro Franceschi, Daniele Catone, Stefano Turchini, Kevin C. Prince,/titolo:Chemical synthesis in acetonitrile containing discharges. Insights from photoionization experiments with synchrotron radiation/doi:10.1016%2Fj.chemphys.2011.06.009/rivista:Chemical physics (Print)/anno:2012/pagina_da:269/pagina_a:277/intervallo_pagine:269–277/volume:398
The photoinduced ion chemistry of acetonitrile is investigated by using tuneable VUV synchrotron radiation in an octupolar ion guide with mass spectrometric detection. The appearance energies and yields of primary photoions and secondary ionic produc
Publikováno v:
第40回月・惑星シンポジウム = Proceedings of the 40th ISAS Lunar and Planetary Symposium. :147-150
We have compared time history of integrated flux of Jupiter's H3(+) aurora, acquired in 1998-2000, with the sola-wind database. The solar wind at Jupiter is simulated based on the MHD (MagnetoHydroDynamic) tomography analysis of InterPlanetary Scinti
Autor:
Miroslav Polášek, Christian Alcaraz, Ján Žabka, Véronique Vuitton, Barbara Cunha de Miranda, Simon Chefdeville, Claire Romanzin
Publikováno v:
Journal of Physical Chemistry A
Journal of Physical Chemistry A, American Chemical Society, 2015, 119 (23), pp.6082-6098. ⟨10.1021/jp512846v⟩
Journal of Physical Chemistry A, American Chemical Society, 2015, 119 (23), pp.6082-6098. ⟨10.1021/jp512846v⟩
An experimental study has been carried out on the reactions of state selected O(+)((4)S, (2)D, (2)P) ions with methane with the aims of characterizing the effects of both the parent ion internal energy and collision energy on the reaction dynamics an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::febdb9071f9ac7265bf058d6ef00d5d8
https://hal.archives-ouvertes.fr/hal-02319338/document
https://hal.archives-ouvertes.fr/hal-02319338/document
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :25-28
For the purpose of confirming the plasma condition of the topside ionosphere, we have investigated spectra of Jupiter's radio emissions observed with the Cassini spacecraft to derive the Faraday rotation for the period of Cassini's Jupiter swing-by a
Autor:
Terada, Naoki, Martian Aeronomy Group
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :132-135
資料番号: AA0063505034
Autor:
Takahashi, Yukihiro, Sakanoi, Takeshi, Yamazaki, Atsushi, Yoshida, Jun, Yoshida, Kazuya, Nakanishi, Hiroki, Shoji, Yasuhiro, Kawasaki, Kohei, Taguchi, Makoto
Publikováno v:
第6回宇宙科学シンポジウム = Proceedings of the 6th Space Science Symposium. :407-450
資料番号: AA0063353044
Autor:
Sakanoi, Takeshi, Takahashi, Yukihiro, Yoshida, Kazuya, Taguchi, Makoto, Yamazaki, Atsushi, Yoshida, Jun, Nakanishi, Hiroki, Shoji, Yasuhiro, Kawasaki, Kohei
Publikováno v:
第5回宇宙科学シンポジウム = Proceedings of the 5th Space Science Symposium. :392-395
惑星観測は、これまで探査機による直接探査と地上望遠鏡による遠隔計測を主な手段としてきたが、どちらも一長一短がある。惑星の大気・プラズマ現象の解明のためには、連続的な時
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