Alec Daly
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View article: Statistical Survey of Interchange Events in the Jovian Magnetosphere Using Juno Observations
Statistical Survey of Interchange Events in the Jovian Magnetosphere Using Juno Observations Open
Interchange instability is known to drive fast radial transport of electrons and ions in Jupiter's inner and middle magnetosphere. In this study, we conduct a statistical survey to evaluate the properties of energetic particles and plasma …
View article: Generation and Impacts of Whistler‐Mode Waves During Energetic Electron Injections in Jupiter's Outer Radiation Belt
Generation and Impacts of Whistler‐Mode Waves During Energetic Electron Injections in Jupiter's Outer Radiation Belt Open
Energetic particle injections are commonly observed in Jupiter's magnetosphere and have important impacts on the radiation belts. We evaluate the roles of electron injections in the dynamics of whistler‐mode waves and relativistic electron…
View article: Plasma Wave and Particle Dynamics During Interchange Events in the Jovian Magnetosphere Using Juno Observations
Plasma Wave and Particle Dynamics During Interchange Events in the Jovian Magnetosphere Using Juno Observations Open
Interchange instability is known to drive fast radial transport of particles in Jupiter's inner magnetosphere. Magnetic flux tubes associated with the interchange instability often coincide with changes in particle distributions and plasma…
View article: Figure 3
Figure 3 Open
The data provided is the electron phase space density in s^3/m^6 as a function of pitch angle from 33.31 keV to 972.3 keV inside and outside of the event. This data is used to create an energy distribution, which is used to estimate the gr…
View article: Plasma Wave and Particle Dynamics During Interchange Events in the Jovian Magnetosphere Using Juno Observations
Plasma Wave and Particle Dynamics During Interchange Events in the Jovian Magnetosphere Using Juno Observations Open
Dataset used to produce figures for the paper and supporting information submitted to Geophysical Research Letters with the title "Plasma Wave and Particle Dynamics During Interchange Events in the Jovian Magnetosphere Using Juno Observati…
View article: Figure S5
Figure S5 Open
Same as figure 2 with panel b's data being replaced by an energy spectrogram of proton fluxes from 3 to 1000 keV, and panels c-e's data being replaced by pitch angle distributions of proton fluxes at 302 keV, 39 keV, and 9 keV.
View article: Figure 1
Figure 1 Open
Juno observations of energetic electrons and plasma waves on 17 February 2020. (a) Magnetic field strength and rate of change (dB/dt); (b) Energy spectrogram of electron fluxes from 30 keV to 1 MeV observed by JEDI; (c) Energy spectrogram …
View article: Figure S4
Figure S4 Open
Same as figure 2 with panel b's data being replaced by an energy spectrogram of proton fluxes from 3 to 1000 keV, and panels c-e's data being replaced by pitch angle distributions of proton fluxes at 302 keV, 39 keV, and 9 keV.
View article: Figure S5
Figure S5 Open
Same as figure 2S with data panel 2b data being replaced by an energy spectrogram of proton fluxes from 3 to 1000 keV, and panels 2c-e data being replaced by pitch angle distributions of proton fluxes at 302 keV, 39 keV, and 9 keV.
View article: Plasma Wave and Particle Dynamics During Interchange Events in the Jovian Magnetosphere Using Juno Observations
Plasma Wave and Particle Dynamics During Interchange Events in the Jovian Magnetosphere Using Juno Observations Open
Dataset used to produce figures for the paper and supporting information submitted to Geophysical Research Letters with the title "Plasma Wave and Particle Dynamics During Interchange Events in the Jovian Magnetosphere Using Juno Observati…
View article: Figure S6
Figure S6 Open
Same as figure S5 with data panel 2b data being replaced by an energy spectrogram of proton fluxes from 3 to 1000 keV, and panels 2c-e data being replaced by pitch angle distributions of proton fluxes at 302 keV, 39 keV, and 9 keV.
View article: Figure S5
Figure S5 Open
Observations of energetic electrons and plasma waves at 05:05-05:10 on 6 April 2019. fig_S2_a) Magnetic field strength and rate of change observed by MAG. fig_S2_b) Energy spectrogram of electron fluxes from 30 keV to 1 MeV observed by JED…
View article: Figure 2
Figure 2 Open
Juno observations from 06:07-06:12 on 6 April 2019. fig_2_a) Magnetic field strength and rate of change observed by MAG. fig_2_b) Energy spectrogram of electron fluxes from 30 keV to 1 MeV observed by JEDI; fig_2_c) Energy spectrogram of e…
View article: Figure S2
Figure S2 Open
Juno observations of energetic electrons and plasma waves on 16 July 2018. (a) Magnetic field strength and rate of change (dB/dt); (b) Energy spectrogram of electron fluxes from 30 keV to 1 MeV observed by JEDI; (c) Energy spectrogram of e…
View article: Figure S3
Figure S3 Open
Same as figure S2 with panel b's data being replaced by an energy spectrogram of proton fluxes from 3 to 1000 keV, and panels c-e's data being replaced by pitch angle distributions of proton fluxes at 302 keV, 55 keV, and 9 keV.
View article: Figure S2
Figure S2 Open
Juno data during event on 16 July 2018. fig_S1_a) Magnetic field strength and rate of change observed by MAG. fig_S1_b) Energy spectrogram of electron fluxes from 30 keV to 1 MeV observed by JEDI; fig_S1_c) Energy spectrogram of electron f…
View article: Figure S1
Figure S1 Open
Same as figure 1 with panels b,c's data being replaced by an Energy spectrogram of proton fluxes from 3 to 1000 keV, and panels d-f's data being replaced by Pitch angle distributions of proton fluxes at 200 keV and 10 keV.
View article: Figure S3
Figure S3 Open
Same as figure 1 with panels b,c's data being replaced by an Energy spectrogram of proton fluxes from 3 to 1000 keV, and panels d-f's data being replaced by Pitch angle distributions of proton fluxes at 200 keV and 10 keV.
View article: Figure S6
Figure S6 Open
Same as figure 2S with data panel 2b data being replaced by an energy spectrogram of proton fluxes from 3 to 1000 keV, and panels 2c-e data being replaced by pitch angle distributions of proton fluxes at 302 keV, 39 keV, and 9 keV.
View article: Figure 4
Figure 4 Open
The data provided is the electron phase space density in s^3/m^6 as a function of pitch angle from 32.77 keV to 974.2 keV inside and outside of the event. This data is used to create an energy distribution, which is used to estimate the gr…
View article: Figure S1
Figure S1 Open
Same as figure 1S with panel b's data being replaced by an energy spectrogram of proton fluxes from 3 to 1000 keV, and panels c-e's data being replaced by pitch angle distributions of proton fluxes at 302 keV, 55 keV, and 9 keV.
View article: Figure 2
Figure 2 Open
Juno observations from 06:07-06:12 on 6 April 2019. fig_2_a) Magnetic field strength and rate of change observed by MAG. fig_2_b) Energy spectrogram of electron fluxes from 30 keV to 1 MeV observed by JEDI; fig_2_c) Energy spectrogram of e…
View article: Figure S1
Figure S1 Open
Same as figure 1 with panels b,c's data being replaced by an Energy spectrogram of proton fluxes from 3 to 1000 keV, and panels d-f's data being replaced by Pitch angle distributions of proton fluxes at 200 keV and 10 keV.
View article: Figure S3
Figure S3 Open
Same as figure 1S with panel b's data being replaced by an energy spectrogram of proton fluxes from 3 to 1000 keV, and panels c-e's data being replaced by pitch angle distributions of proton fluxes at 302 keV, 55 keV, and 9 keV.
View article: Figure S4
Figure S4 Open
Observations of energetic electrons and plasma waves at 05:05-05:10 on 6 April 2019. fig_S2_a) Magnetic field strength and rate of change observed by MAG. fig_S2_b) Energy spectrogram of electron fluxes from 30 keV to 1 MeV observed by JED…
View article: Energetic Proton Distributions in the Inner and Middle Magnetosphere of Jupiter Using Juno Observations
Energetic Proton Distributions in the Inner and Middle Magnetosphere of Jupiter Using Juno Observations Open
Jupiter is known to have a complex magnetosphere containing energetic (above 10s of keV) electrons, protons, and heavy ions. However, a global distribution of these energetic particles is not fully understood before the era of the polar‐or…