• Aucun résultat trouvé

Saturn's aurorae

N/A
N/A
Protected

Academic year: 2021

Partager "Saturn's aurorae"

Copied!
49
0
0

Texte intégral

(1)

Tom Stallard

Saturn’s

aurorae

University of

L

e

i

c

e

s

t

e

r

Sarah Badman, University of Lancaster

Ulyana Dyudina, Caltech

Denis Grodent, University of Liege

(2)

Jupiter

Earth

(3)

Bunce et al [2003] Persoon et al [2013]

(4)

Lamy et al., 2009

Radio aurora

(5)
(6)

Energetic particle

precipitation

(7)

H, H

2

H*, H

2

*

Energetic particle

precipitation

(8)

H, H

2

H*, H

2

*

H

2

= H

2

+

H

2

+

+

H

2

=

H

3

+

… … …

H

3

+

1 2 3

Energetic particle

precipitation

(9)

Lamy et al., 2013

Lyα

H

2

(10)

Visible aurora

Baβ

Based on Dyudina et al., submitted

H

2

Dyudina et al.

(11)

H

3

+

CH

4

Infrared aurora

(12)

Altitudinal extent

(13)

Morphology of the aurora

(14)

Badman et al., 2011

N>S

S>N

70

˚

60

˚

80

˚

Lamy et al., 2009

(15)

Badman et al., 2006; 2012; Nichols et al., submitted

(16)

Talboys et al., 2011

(17)

UVIS

VIMS

ISS

Melin et al., 2011; submitted – see also Lamy et al., 2013

(18)

FUV EUV FUV+EUV

H

2

color ratio

(19)

Small scale structures

Spatial resolution ~200 km

0800

1000

1200

Dyudina et al., submitted; Grodent et al., WIP

(20)

Solar wind

interaction

(21)
(22)
(23)
(24)

(a)

Dayside reconnection

(a)

Tail reconnection

(a)

Unbalanced tail and dayside

reconnection e.g. large

compression-induced tail

reconnection

(b)

Rotating diffuse blob produced

by tail reconnection

After Badman et al. (2005), Cowley et al. (2005)

(25)

Stallard et al., 2012

(26)

Origin of these

small scale

auroral

features?

Complex Field-Aligned Current (FAC) structures

Bunce et al. [2010], Talboys et al. [2009,2011]

1-2° (lat) wide

FAC structures

(27)

Badman et al., 2012 Pryor, priv. comm.

(28)
(29)

Dusk spots non-conjugate

(30)

Origin of these

small scale

auroral

features?

Vortices triggered by K-H instabilities

Masters et al. [2010], Fukazawa et al. [2009],Walker et al. [2011], Delamere et al. [2011]

FAC associated

with dΩ

//

/ dt

> 0.55 R

S

Wilson et al. [2012]:

(31)

Meredith et al., 2013

(32)

Dyudina et al., submitted

Stallard et al., 2008

(33)

Magnetospheric

plasma

(34)

Mitchell et al., 2009

(35)

Radioti et al., 2012

Cassini/UVIS

UV aurora related to electrons injections 1) pitch angle diffusion + electron scattering and 2) FACs driven by ∇p along boundaries of hot plasma cloud (ENA)

Cassini/INCA

variable color scale

(36)

Cassini/UVIS 2008_240_05_46 South Pole

Schippers et al., 2012 Grodent et al. WIP

(37)

Enceladus footprint

Pryor et al., 2011

(38)
(39)

O’Donoghue et al., 2013

(40)

Periodic

(41)

One-hour period oscillations

(42)
(43)

Nichols et al., submitted Nichols et al., 2010

(44)

Badman et al., 2012 Stallard

(45)

Auroral currents in PPO phase

(46)

Opposite sum and difference profiles

(47)
(48)
(49)

Summary

Drivers of aurora

Solar wind interactions (Earth-like)

Internal plasma interactions (Jupiter-like)

Neutral atmosphere interactions(?)

Highlights the need for multi-instrument observations

Ongoing research

2013 Campaign Icarus Special Issue

Continued simultaneous observations in 2014-2015

Proximal orbit campaign

Need to observe mesosphere-ionosphere-aurora interactions

Seasonal variability

Références

Documents relatifs

[2011] dem- onstrated the role of the obliqueness of wave propagation for pitch-angle diffusion, thus far the overwhelming majority of calculations for diffusion coefficients have

Although many of the waves have been observed from the Voyager epoch to the Cassini epoch and their structures appear very similar to density and bending waves, most do not appear

We compare the effects of resonant wave–particle scattering by lower band chorus waves and the adiabaticity violation of electron motion due to the strong curvature of field lines

Systems are developed with this framework by defining concrete events, global state variables and invariants over them, and event handlers and filters.. Becaues

Since reducing the burden of rehospitalisations during the vulnerable phase is of critical clinical importance, we analyse here the effect of chronic exposure to ivabradine versus

Among the candidate genes that might play a role in regulating IKBKAP mRNA alternative splicing, NOVA1, a gene encoding the neuron-specific splicing factor, was found to be

Enfin, le développement d’un outil assurant le forçage du modèle d’agitation par le modèle de propagation permet d’obtenir un outil performant simulant la houle depuis le

Considering the dilution rate D as the control, we are able to build a closed loop feedback depending on the measurements of bacterial concentration (through e.g. the optical