Jupiter radio emission probability tool

Frontiers in Astronomy and Space Sciences

Astronomy and Space Sciences

S. Aicardi¹  B. Cecconi²  L. Lamy³ 

[1] DIO, Observatoire de Paris-PSL, CNRS, Paris, France;LESIA, Observatoire de Paris-PSL, CNRS, Sorbonne Université, Université Paris Cité, Paris, France;ORN, Observatoire de Paris-PSL, Université d'Orléans, CNRS, Nançay, France;LESIA, Observatoire de Paris-PSL, CNRS, Sorbonne Université, Université Paris Cité, Paris, France;ORN, Observatoire de Paris-PSL, Université d'Orléans, CNRS, Nançay, France;Aix Marseille Université, CNRS, CNES, LAM, Marseille, France;

关键词: jupiter;    radio emissions;    space physics;    online application;    observation planning;    python;   

DOI  :  10.3389/fspas.2023.1091967

 received in 2022-11-07, accepted in 2023-01-09,  发布年份 2023

来源: Frontiers

【 摘 要 】

Jupiter is a source of intense radio emissions in the decametric wavelength range observable from ground (above ∼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.

【 授权许可】

Unknown   
Copyright © 2023 Cecconi, Aicardi and Lamy.