This dataset is the digitised version of Table 1 of Leblanc et al. (1983) paper. This version has been curated by B. Cecconi and L. Debisschop. They used an online OCR (Optical Character Recognition) tool (available at: https://www.onlineocr.net) for the initial conversion of the ADS provided scanned pages of the paper. They reformatted the table and validated the content.

This dataset provides public access to polar projections of the Juno spacecraft magnetic footprint during perijoves (PJ) ±5h computed with 3 different magnetic field models, from mid 2016 (PJ1) to mid 2018 (PJ14).

This collection is composed of Cassini/RPWS/NHFR (Radio and Plasma Waves Science / High Frequency Receiver) hourly N2 (Level 2) files.

This collection contains a series of published Jovian radio emission probability and occurrence maps.

This collection is composed of the Southern and Northern SKR phase systems derived from Cassini/RPWS/HFR (Radio and Plasma Waves Science / High Frequency Receiver) measurements, as described in Lamy (2011).

Le guide du DMP à l’Observatoire de Paris complète le modèle de DMP proposé par le Groupe de Travail Science ouverte. Il donne davantage de détails, renvoie vers des liens utiles pour celles et ceux qui n’auraient pas eu toutes les réponses à leurs questions avec le seul modèle de DMP.

Abstract: The European Radiation Dosimetry Group, EURADOS focuses, among other issues, on the harmonization of dose assessment within Europe and conformance with international practices. Along these lines, this EURADOS report compares route doses and dose rates at flight altitudes due to solar cosmic radiation (SCR) associated with ground level enhancements (GLEs) as calculated by means of nine available computer codes. Some of these codes are routinely used for the assessment of radiation exposure of aircraft...

This collection is contains all the Cassini/RPWS/HFR data products (from raw data to added-value products).

This paper describes what is available in BASS2000 database and how to use it the best possible way. It details access to all kinds of observations, in various ways, as well as use of specific tools, and use of Heliophysics Feature Catalogue (HFC) from HELIO

Decametric radio observation from Nançay Decameter Array (NDA). The NDA at the Station de Radioastronomie de Nancay (SRN) is a phased array of 144 "Teepee" helicoidal antenna, half of which being Right Handed (RH) polarized and the other half being Left Handed (LH) polarized. Four receivers are currently connected to the NDA, sampling data in spectral ranges within 5 to 80 MHz. This collection contains the Solar observation data products, in raw and CDF formats.

This collection is composed of Cassini/RPWS/HFR (Radio and Plasma Waves Science / High Frequency Receiver) hourly N3d (Level 3d) files.

This document describes the on-boarding process for new data providers in VESPA.

This dataset contains the natural planetary low frequency radio emission spectra for the Sun, the Earth, Jupiter, Saturn, Uranus and Neptune

This dataset contains calibrated Cassini-RPWS-HFR Jupiter fly-by data from 6 months of Jupiter encounter: 2000-275 (Oct 1st) 00:00 to 2001-090 (Mar 31st) 24:00. The spectral range covers 3.5 kHz to 16 MHz.

This dataset is the digitised version of Table 1 of Leblanc et al. A&A 1981 paper. This version has been curated by B. Cecconi and L. Debisschop. They used an online OCR (Optical Character Recognition) tool (available at: https://www.onlineocr.net) for the initial conversion of the ADS provided scanned pages of the paper. They reformatted the table and validated the content.

This collection contains figures and movies showing the ExPRES radio source occultations during the Galileo spacecraft Jovian icy moon flybys. This collection supplements: Cecconi, B, C K Louis, C Muñoz Crego, and C Vallat. 2021. “Jovian Auroral Radio Source Occultation Modelling and Application to the JUICE Science Mission Planning.” Planetary and Space Science 209 (105344): 1–34. doi:10.1016/j.pss.2021.105344.

This document presents the process to prepare the individual VESPA resource descriptor repository.

L’attribution d’un identifiant pérenne – c’est-à-dire d’un DOI – à un jeu de données nécessite quelques prérequis. La fiche intitulée « Les bonnes pratiques en matière de DOI à l’Observatoire de Paris » explique ce qu’est un DOI, à quoi il ressemble et présente les différentes métadonnées qu’il faudra renseigner pour attribuer un DOI à des données.

This collection is composed of Cassini RPWS Quasi Thermal Noise (QTN) data set contains thermal plasma parameters derived by QTN spectroscopy analysis applied on data acquired with the High Frequency Receiver (HFR) during the perikrones of the entire mission.

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...