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Jupiter radio emission probability tool
被引:1
|作者:
Cecconi, B.
[1
,2
]
Aicardi, S.
[3
]
Lamy, L.
[1
,2
,4
]
机构:
[1] Univ Paris Cite, Sorbonne Univ, Observ Paris PSL, LESIA,CNRS, Paris, France
[2] Univ Orleans, Observ Paris PSL, CNRS, ORN, Nancay, France
[3] Observ Paris PSL, CNRS, DIO, Paris, France
[4] Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
来源:
关键词:
jupiter;
radio emissions;
space physics;
online application;
observation planning;
!text type='python']python[!/text;
EUROPA;
D O I:
10.3389/fspas.2023.1091967
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Jupiter is a source of intense radio emissions in the decametric wavelength range observable from ground (above & SIM;10 MHz) and from space (down to a few kHz). The strong anisotropy of the Jovian radio sources results in characteristic shapes in the temporal-spectral domain, which can be used to identified the various types of Jovian radio components. The Jupiter Probability Tool provides users with Jovian radio emission observability predictions, depending on the observers location, and the radio emission class. The application can be used for observation planning or data analysis for ground or space observations.
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页数:7
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