• Aucun résultat trouvé

Spatial Distribution of the Pedersen Conductance in the Jovian Aurora From Juno‐UVS Spectral Images

N/A
N/A
Protected

Academic year: 2021

Partager "Spatial Distribution of the Pedersen Conductance in the Jovian Aurora From Juno‐UVS Spectral Images"

Copied!
11
0
0

Texte intégral

Loading

Références

Documents relatifs

The main properties of this inner magnetospheric region are briefly recalled. The dynamical response of the plasma s phere to enhancements of geomagnetic activity

These systems are compared for the competition and complementarities between crops in terms of grain yield of rice and maize, and biomass production.. During the wet season of

tems can be related to the spin wave properties of the ferromagnet, and we evaluate contributions arising from surface spin waves as well as from the bulk spin waves.. The first

Mukherjee, Hilbert+ et al in prep (solid line) Henriques 2014 (dash line) Lagos+ 2012 COSMICLENS: gamma= 0.2. Effect of baryonic

Maintenant que nous disposons de plusieurs années d’observations de l’ozone troposphérique au-dessus de l’Europe pendant la période estivale, plusieurs axes de recherche sont

In this study, in order to determine Tks5 interactome in situ and therefore invadopodia molecular compo- sition, we engineered MDA-MB-231 breast cancer cell lines expressing

The results (Table 1) reveal that (1) the population activity of the D1down neurons is signif- icantly higher than that of the D1up neurons in the epoch pre- ceding TC ( p ⬍⬍ 0.001

Figure 4: Total porosity versus the surface area of the image of (a) a quarried tuffeau, (b) a quarried sebastopol stone, (c) the strongly weathered zone of a weathered