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![Page 1: The Magnetosphere of Planet Mercury The planet Shape and structure of the magnetosphere Current systems Dynamics Energy sources Eigen oscillations.](https://reader035.fdocuments.net/reader035/viewer/2022062511/551c06765503469e4f8b4ec9/html5/thumbnails/1.jpg)
The Magnetosphere of Planet The Magnetosphere of Planet MercuryMercury
The planet
Shape and structure of the magnetosphere
Current systems
Dynamics
Energy sources
Eigen oscillations
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Planet und MagnetfeldPlanet und Magnetfeld
Planetenradius: 2439 kmKernradius: ~1829 kmMittl. Dichte: 5.42 g/cm3
Rotationsrate: 58.64 TageDipolmoment: 5·1019 Am2
Ober. Temp.: -173° - 429°Atmosphäre: NeinExosphäre: JaPlasmasphäre: NeinMagnetosphäre: Ja
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Das Magnetfeld des Planeten MerkurDas Magnetfeld des Planeten Merkur
Ness et al., 1978
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Planetary Magnetic FieldsPlanetary Magnetic Fields
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Magnetospheric Plasma SourcesMagnetospheric Plasma Sources
Mercury: solar wind and sputtering of surface material, e.g. sodium
Earth: solar wind and ionosphere
Jupiter: solar wind and volcanic activity of the moon Io
Saturn: solar wind, atmosphere of moon Titan, sputtering at surfaces of icy moons and rings
Uranus: polar ionosphere, minor solar wind contribution
Neptun: ionosphere, moon Triton
Mercury: solar wind and sputtering of surface material, e.g. sodium
Earth: solar wind and ionosphere
Jupiter: solar wind and volcanic activity of the moon Io
Saturn: solar wind, atmosphere of moon Titan, sputtering at surfaces of icy moons and rings
Uranus: polar ionosphere, minor solar wind contribution
Neptun: ionosphere, moon Triton
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The MagnetosphereMagnetosphere of Mercury
No atmosphere
thus no ionosphere
but exosphere
No plasmasphere
Weak magnetic field
Multi-ion plasma
Small magnetosphere
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Solar Wind: The Embedding MediumSolar Wind: The Embedding MediumSolar Wind: The Embedding MediumSolar Wind: The Embedding Medium
Magnetic field and plasma density
Mercury: 46 - 21 nT 73 - 33 cm-1
Earth: 8 nT 5 cm-1
Jupiter: 1 nT 0.2 cm-1
Saturn: 0.6 nT 0.06 cm-1
Uranus: 0.3 nT 0.01 cm-1
Neptun: 0.005 nT 0.005 cm-1
The velocity is almost constantin the inner part of the heliosphere
Magnetic field and plasma density
Mercury: 46 - 21 nT 73 - 33 cm-1
Earth: 8 nT 5 cm-1
Jupiter: 1 nT 0.2 cm-1
Saturn: 0.6 nT 0.06 cm-1
Uranus: 0.3 nT 0.01 cm-1
Neptun: 0.005 nT 0.005 cm-1
The velocity is almost constantin the inner part of the heliosphere
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Magnetopause FormationMagnetopause FormationMagnetopause FormationMagnetopause Formation
The magnetopause is a surface where the dynamic pressure of the solar wind
and the magnetic pressure of the magneto-spheric plasma are in equilibrium:
The dynamic pressure of solar wind particles istransferred to the magnetospheric plasma by
specular reflection of the particles at the boundary.
0
22
22
B
vmnp swpswdyn
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Magnetoapause PositionMagnetoapause PositionMagnetoapause PositionMagnetoapause Position
The magnetopause stand-off distance along the
Sun-Earth line is given by
where k = 0.88 is a correction factor resulting from
gasdynamic approximations to the magnetosheath
flow: At Mercury RMP = 1.5 RP
The magnetopause stand-off distance along the
Sun-Earth line is given by
where k = 0.88 is a correction factor resulting from
gasdynamic approximations to the magnetosheath
flow: At Mercury RMP = 1.5 RP
6/12
0
2
)2
4(
swpsw
SurfaceMP vmnk
BR
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Electric Currents in the MagnetosphereElectric Currents in the MagnetosphereElectric Currents in the MagnetosphereElectric Currents in the Magnetosphere
Magnetopause currents
No ring current
Neutral sheet current
Tail current
Field-aligned currents
No polar electrojet currents
Magnetopause currents
No ring current
Neutral sheet current
Tail current
Field-aligned currents
No polar electrojet currents
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Magnetopause Current - Magnetopause Current - Chapman-Ferraro CurrentChapman-Ferraro CurrentMagnetopause Current - Magnetopause Current - Chapman-Ferraro CurrentChapman-Ferraro Current
At the mp jump in magneticfield by about 24 nT, a valuetypical also at the terrestrialmp.
From a current density of aboutjMP1.510-7 A/m2 results,assuming an mp thicknessof 125 km.
jB
0
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Magnetopause Current – Magnetopause Current – Ground Magnetic EffectGround Magnetic Effect
Magnetopause Current – Magnetopause Current – Ground Magnetic EffectGround Magnetic Effect
Chapman-Ferraro currents produce ground-magneticeffects, which at
Earth are of the order of 10 nT added to a 30,000 nT background field
and at
Mercury are of the order of 70 nT added to a 340 nT background field
The external field matters at the surface !!!!
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Field-Aligned CurrentsField-Aligned CurrentsField-Aligned CurrentsField-Aligned Currents
Slavin et al., 1997
Field-alignedcurrent density:
7x10-7 A/m2
Closure problem
as at Earth FACsclose in theionosphere butMercury has noionosphere
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Is there a substorm current wedgeIs there a substorm current wedge at Mercury ?at Mercury ?
Is there a substorm current wedgeIs there a substorm current wedge at Mercury ?at Mercury ?
jRjR
Enhanced westward electrojetin theIonosphere
or
closure viadiamagnetic currents in the plasma itself
Enhanced westward electrojetin theIonosphere
or
closure viadiamagnetic currents in the plasma itself
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Substorms and Flux Transport in the Open Magnetosphere
Substorms and Flux Transport in the Open Magnetosphere
Dayside reconnection transports plasma
and magnetic flux towards the nightside tail
where return flux is initiated by reconnection
again.
Dayside reconnection transports plasma
and magnetic flux towards the nightside tail
where return flux is initiated by reconnection
again.Dungey‘s model of the closed and open magnetosphereDungey‘s model of the closed and open magnetosphere
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Corotation, Reconnection Induced Convection, and the PlasmapauseCorotation, Reconnection Induced Convection, and the Plasmapause
Does Mercury have a plasmasphere ? Does Mercury have a plasmasphere ?
Plasmapause
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Magnetospheric Convection and Corotation
Magnetospheric Convection and Corotation
Corotation implies plasma motion and via the frozen-in theorem
electric fields, that is the corotational electric field is given as
and corotation driven plasma motion is ExB-drift convection
Corotation implies plasma motion and via the frozen-in theorem
electric fields, that is the corotational electric field is given as
and corotation driven plasma motion is ExB-drift convection
0 BvE
rEsurfaceEarth
cor er
RBE
2
3
2B
BEv corcor
Mercury hasnoplasmasphere
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External Forcing – Internal Reactions ?External Forcing – Internal Reactions ?
Siscoe and Christopher, 1975
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Bulk Modulus and CompressibilityBulk Modulus and Compressibility
V
pVK
Modulus
pd
Vd
V
1
Compressibility
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2
6/1
0
20 ; swpswMP vmnpp
BR
Magnetopause position
)(; MPMPMPMP
MP RrppdR
dpRK
Bulk modulus
MPpK /1/1 Compressibility
Mercury has a very stiff, but Jupiter a very fluffy magnetosphere; Mercury rings, Jupiter not !!!!!!
The Magnetospheric Bulk ModulusThe Magnetospheric Bulk Modulus
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Ringing the Magnetospheric Bell
Units: 1 nT; 0.1 mV/m
Magnetospheric eigen-oscillations are MHDwaves in the terretrialmagnetosphere.
Their periods are muchlonger than proton gyroperiods !!!
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This is the only published
evidence for ULF waves in
the Hermean magnetosphere.
Amplitude: 2 nT
Period: 2 s, e.g.
about twice TG,Proton
this wave is not an
MHD wave !!!!
ULF ULF WavesWaves at at MercuryMercury
(from Russell, 1989)
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Global oscillations: Global oscillations: The Dungey ProblemThe Dungey Problem
Dipolemagnetosphere
MHD oscillations
Axisymmetric perturbations
Decoupled toroidal andpoloidal oscillations
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Decoupled toroidal
and poloidal eigen-
oscillations for axi-
symmetric ( m=0 )
perturbations
Voelker,1963
Global oscillations: EarthGlobal oscillations: Earth
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To treat this question we need Dungey‘s
equations for a non-MHD model of the
Hermean magnetosphere
as the anticipated eigenfrequencies are
less, but comparable to the gyrofrequency
Global oscillations: MercuryGlobal oscillations: Mercury
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3
12
21
00
0
0
i
iDielectric Tensor;
0<< < i
2
2
3
2
2
22
2
2
2
2
2
1 ;
pe
iAiAA v
c
v
c
v
c
Mercury: A Two Component Mercury: A Two Component Cold Plasma ApproachCold Plasma Approach
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11
2111 ggi
||eE
2
2
13
23
Avg
g
g
g
Mercury: Global OscillationsMercury: Global OscillationsAxisymmetric Perturbations m=0Axisymmetric Perturbations m=0
Scalar potentials
Toroidal operatorusing curvi-linearcoordinates
Toroidal oscillationcoupled to poloidalthough m=0, dueto 2
=> Dmitri Klimushkin and Pavel Mager
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a) Solar wind buffeting causes ringing of the magneto- sphere
b) The scale of the magnetosphere is about 10 x the ion gyroradius
c) Waves generated by buffeting are kinetic Alfvén waves with E|| 0.2 mV/m (Glassmeier, 2000)
d) Buffeting causes particle heating via kinetic Alfvén waves
Kinetic Alfvén Waves Kinetic Alfvén Waves in the Hermean Magnetospherein the Hermean Magnetosphere
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Electromagnetic Induction Electromagnetic Induction at Mercuryat Mercury
We have a small magnetosphere
Magnetopause currents are close to the planet
Temporal variations of magnetopause currents may cause strong induction effects
As the planet consists mainly out of a highly conducting core
How large are these induced fields ?
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Isototalen an der MerkuroberflächeIsototalen an der Merkuroberfläche
Länge
Bre
ite
Quadrupol-anteile
Nordpol
NordpolSüdpol
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BepiColombo am 28. April 2014BepiColombo am 28. April 2014
28. April 201417:00
Gesamtes Feld:HV-Magnetosphäremit 2-h periodischerMagnetopausenBewegung
Internes Feld
Externes FeldInduziertes Feld
Jan Grosser, Diplomathesis
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Das Humboldt Observatorium,Das Humboldt Observatorium,Merkuräquator, 28. April 2014, 18:00 LokalzeitMerkuräquator, 28. April 2014, 18:00 Lokalzeit
17:00
28. April 2014
Gesamtes Feld
Interner Anteil
Externer AnteilInduzierter Anteil
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SummarySummary
Mercury is a new point
in the magnetospheric
phase space !!!!!!
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Ein Dankeschön an...Ein Dankeschön an...
Jan Grosser Jan Grosser Diplomand am IGM, TUBSDiplomand am IGM, TUBS
Anja StadelmannAnja Stadelmann Doktorandin am IGM, TUBSDoktorandin am IGM, TUBS
Dr. Ulrich AusterDr. Ulrich Auster IGM, TU BraunschweigIGM, TU Braunschweig
Prof. Dr. D. Klimushkin,Prof. Dr. D. Klimushkin, Irkutsk, RussiaIrkutsk, Russia
Dr. P. Mager, Dr. P. Mager, Irkutsk, RussiaIrkutsk, Russia
Prof. Dr. J. VogtProf. Dr. J. Vogt IUB, BremenIUB, Bremen
Prof. Dr. G.-H. VoigtProf. Dr. G.-H. Voigt FH AachenFH Aachen