in geomagnetic activity Lauri Holappa and Kalevi Mursula ReSoLVE - - PowerPoint PPT Presentation

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in geomagnetic activity Lauri Holappa and Kalevi Mursula ReSoLVE - - PowerPoint PPT Presentation

Explicit IMF By-effect in geomagnetic activity Lauri Holappa and Kalevi Mursula ReSoLVE Centre of Excellence University of Oulu, Finland Solar wind-magnetosphere coupling IMF B z -component is the main driver of magnetic reconnection at


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SLIDE 1

Explicit IMF By-effect in geomagnetic activity

Lauri Holappa and Kalevi Mursula

ReSoLVE Centre of Excellence University of Oulu, Finland

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SLIDE 2
  • IMF Bz-component is the main

driver of magnetic reconnection at the magnetopause

  • IMF By is included in coupling

functions, but its effect does not depend on its sign

𝑒Φ𝑁𝑄 𝑒𝑒

= 𝑀4/3πΆπ‘ˆ

2/3sin πœ„ 2 8/3

,

πΆπ‘ˆ = 𝐢𝑨

2 + 𝐢𝑧 2

πœ„ = arctan 𝐢𝑧 𝐢𝑨

  • Does the sign of By matter?
  • Stronger auroral electrojets

for By>0 than for By < 0 in winter! [Friis-Christensen et al., 2017; Smith et al., 2017]

Solar wind-magnetosphere coupling

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SLIDE 3

Russell-McPherron effect

  • Negative IMF Bz in GSM coordinate system for IMF By > 0

in fall and for By < 0 in spring.

[Zhao et al., 2012] Spring Fall

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SLIDE 4

Russell-McPherron effect

=> Solar wind driving of the magnetosphere is enhanced for IMF By > 0 in fall, and for By < 0 in spring.

Superposed monthly means and standard errors of the Newell function dΦMP/dt in 1966-2015

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SLIDE 5
  • Deep minimum in AL index during winter for By < 0
  • Cannot be explained by the Russell-McPherron effect.

=> Explicit By-effect

Seasonal variation of AL index

All data in 1966-2015

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SLIDE 6

Explicit By-effect in AL index

  • In NH winter, for the same value of

dΦMP/dt, By > 0 produces a stronger AL-index than By < 0.

  • Opposite By-dependence

in NH summer

|AL|, winter solstice Β± 15 days |AL|, summer solstice Β± 15 days

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SLIDE 7

Explicit By-effect in AL index

  • Explicit By-dependence is

very weak around spring and fall equinoxes.

|AL|, spring equinox Β± 15 days |AL|, fall equinox Β± 15 days

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SLIDE 8

a) We calculate measured and predicted polarity ratios includes the RMP-effect b) The ratio of these two ratios quantifies the explicit By-effect AL index is about 40-50% stronger for By>0 than for By<0 around the winter solstice.

Removing Russell-McPherron effect

[Holappa and Mursula, JGR, 2018]

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SLIDE 9

Latitudinal dependence

  • For strong driving (Bz < -5 nT), the By-effectis about 40% at subauroral latitudes

(55Β°-60Β°) even when averaging over all seasons. => Substorms are stronger and latitudinally more extensive for By > 0 than for By < 0.

  • Ratio R+/- for local

geomagnetic indices (Ah-indices) at different latitudes for all seasons in 1995-2017 [Holappa et al., JGR, 2019]

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SLIDE 10

Latitudinal dependence

  • For strong driving (Bz < -5 nT), the By-effectis about 40% at subauroral latitudes

(55Β°-60Β°) even when averaging over all seasons. => Substorms are stronger and latitudinally more extensive for By > 0 than for By < 0.

  • Ratio R+/- for local

geomagnetic indices (Ah-indices) at different latitudes for all seasons in 1995-2017 [Holappa et al., JGR, 2019]

YOU ARE HERE

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SLIDE 11
  • IMF By is an explicit driver of high-latitude

geomagnetic activity

  • Geomagnetic activity is significantly stronger for

By > 0 than for By < 0 in winter

  • The By-effect is strongest at subauroral latitudes

at about 55Β°-60Β° geomagnetic latitude

  • IMF By is important for space weather

predictions

  • No physical explanation yet!

References:

  • L. Holappa and K. Mursula, J. Geophys. Res. (Space), 123, 2018.
  • L. Holappa, N. Gopalswamy and K. Mursula, J. Geophys. Res.

(Space), 124, 2019.

Summary

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SLIDE 12

By-effect in Southern Hemisphere

  • K-index of Syowa station

in Antarctica

  • During SH winter, for the

same value of dΦMP/dt, By < 0 produces stronger K-index than By > 0.

  • By-dependence in SH is
  • pposite to that in NH
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SLIDE 13

By-effect in Southern Hemisphere

  • During SH summer, for

the same value of dΦMP/dt, By > 0 produces stronger K-index than By < 0.

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SLIDE 14
  • By-dependence in the AU

index (eastward electrojet) is solely due to Russell- McPherron effect

No explicit By-effect in AU index

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  • The explicit By-effect (in

NH) maximizes around 5 UT, i.e., when the Earth’s dipole axis points away from the Sun οƒž The explicit By-effect maximizes when the auroral region is maximally in darkness οƒž By-effect is efficient under low ionospheric conductivity?

UT-variation

Left: Ratio π‘†π‘“π‘¦π‘žπ‘š

+/βˆ’(AL) for different UT hours and

months. Right: π‘†π‘“π‘¦π‘žπ‘š

+/βˆ’(AL) averaged over months.

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SLIDE 16
  • There is a correlation

between By and Bx. Which of the two components is the driver?

  • Limiting the amplitude
  • f Bx has almost no

effect to the results => Bx has only little, if any, explicit effect on high latitude geomagnetic activity

No explicit Bx effect