Results 1 to 10 of about 6,029 (233)

Jovian Vortices and Jets [PDF]

Fluids, 2019
We explore the theory of isolated vortices in strongly sheared, deep zonal flows and the stability of these banded jets, as occur in Jupiter’s atmosphere This is done using the standard 2-layer quasigeostrophic model with the lower layer depth ...
Glenn R. Flierl, Philip J. Morrison, Rohith Vilasur Swaminathan   +2 more
doaj   +4 more sources

Modeling of the Jovian Magnetosphere [PDF]

Annales Geophysicae, 2005
This paper presents a global model of the Jovian magnetosphere which is valid not only in the equatorial plane and near the planet, as most of the existing models are, but also at high latitudes and in the outer regions of the magnetosphere. The model
I. I. Alexeev, E. S. Belenkaya
doaj   +5 more sources

Accessible viral metagenomics for public health and clinical domains with Jovian [PDF]

Scientific Reports
The integration of next-generation sequencing into clinical diagnostics and surveillance initiatives is impeded by the lack of data analysis pipelines that align with privacy legislation and laboratory certification protocols. To address these challenges,
Dennis Schmitz, Florian Zwagemaker, Sam Nooij, Thierry K. S. Janssens, Jeroen Cremer, Robert Verhagen, Harry Vennema, Annelies Kroneman, Marion P. G. Koopmans, Jeroen F. J. Laros, Miranda de Graaf   +10 more
doaj   +2 more sources

The Jovian Evection [PDF]

Monthly Notices of the Royal Astronomical Society, 1890
E. Nevill
openaire   +3 more sources

In situ evidence of the magnetospheric cusp of Jupiter from Juno spacecraft measurements [PDF]

Nature Communications
The magnetospheric cusp connects the planetary magnetic field to interplanetary space, offering opportunities for charged particles to precipitate to or escape from the planet.
Y. Xu, C. S. Arridge, Z. H. Yao, B. Zhang, L. C. Ray, S. V. Badman, W. R. Dunn, R. W. Ebert, J. J. Chen, F. Allegrini, W. S. Kurth, T. S. Qin, J. E. P. Connerney, D. J. McComas, S. J. Bolton, Y. Wei   +15 more
doaj   +2 more sources

Jupiter radio emission probability tool

Frontiers in Astronomy and Space Sciences, 2023
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).
B. Cecconi, B. Cecconi, S. Aicardi, L. Lamy, L. Lamy, L. Lamy   +5 more
doaj   +1 more source

Variation of the Jovian Magnetopause Under Constant Solar Wind Conditions: Significance of Magnetodisc Dynamics

Geophysical Research Letters, 2023
It is generally believed that variations in the upstream solar wind (SW) and interplanetary magnetic field (IMF) conditions are the main cause of changes of Jupiter's magnetopause (JM) location.
Enhao Feng, Binzheng Zhang, Zhonghua Yao, Peter A. Delamere, Zhiqi Zheng, William R. Dunn, Sheng‐Yi Ye   +6 more
doaj   +1 more source

Lightning at Jupiter pulsates with a similar rhythm as in-cloud lightning at Earth

Nature Communications, 2023
Our knowledge about the fine structure of lightning processes at Jupiter was substantially limited by the time resolution of previous measurements. Recent observations of the Juno mission revealed electromagnetic signals of Jovian rapid whistlers at a ...
Ivana Kolmašová, Ondřej Santolík, Masafumi Imai, William S. Kurth, George B. Hospodarsky, John E. P. Connerney, Scott J. Bolton, Radek Lán   +7 more
doaj   +1 more source

Jovian Periodicities (~10 h, ~40, 20, 15 min) at ACE, Upstream from the Earth’s Bow Shock, on 25–27 November 2003

Universe, 2023
It is known that Jovian radio and high energy electron emissions are observed near Earth. The question we address in this study is whether the quasi-periodic ~10 h and ~40/15–20 min (QP-10 h, QP-40/15–20 min) energetic particle and magnetic field ...
Georgios C. Anagnostopoulos, Panagiotis K. Marhavilas, Efthymios Vassiliadis, Emmanuel T. Sarris   +3 more
doaj   +1 more source

The Jovian ionosphere [PDF]

Geophysical Research Letters, 1974
Models for the Jovian ionosphere which incorporate the role of hydrocarbons in the production and loss of ionization, are presented. A new feature is the possible existence of a second peak in the electron density distribution. On comparing our model with the results of the Pioneer‐10 measurements of the Jovian ionospheric electron density‐distribution,
S. S. Prasad, Arjun Tan
openaire   +1 more source