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Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME Mythology: Do Global CMEs or Sympathetic CMEs Exist?
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Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

Dec 16, 2015

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Page 1: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

Rainer SchwennMax-Planck-Institut für Aeronomie

Katlenburg-Lindau

International Solar Cycle Studies 2001 (ISCS),

June 13-16, 2001Longmont, Colorado

CME Mythology: Do Global CMEs or Sympathetic CMEs Exist?

Page 2: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

A classical “halo” CME, observed by LASCO-

C2 on 4.11.1998

Towards or away from Earth? That knowledge would grantspace weather predictions a new quality

Halo CMEs: a new quality from SOHO

Page 3: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

A pressure wave (EIT Wave) in the solar

atmosphere, pushed by a flare on

7.4.1997.A halo CME was

launched towards Earth that caused a geomagnetic storm

on 10.4.97.

Front or backside: a new quality from SOHO

Page 4: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

This CME began as a “global” CME, i.e. in two parts

simultaneously on both limbs. Later, the envelope turned into

a full halo.

Note: the source “axis” was about parallel to the lobes’ axis

Page 5: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

Another apparent halo CME, also from two parts on

opposite limbs

This was the obvious source, on the front side.

The bright flash occurred at 05:58 UT, and the axes were parallel.However…

Page 6: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

…close inspection of C2 images proves: the east limb event started more than one hour ahead of time! An independent

backside source?

Morale: better look twice, in particular if you are about to create a myth…

Page 7: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

No: two lobes contained in one single halo CME, a “split halo”

The typical “global” CME?

Page 8: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

The same event: the source axis was

perpendicular to the lobes’ axis!

Page 9: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

No “global “ event, just two lobes contained in a halo CME, a backside event by the way

Page 10: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

Another split halo CME, “butterfly type”

Page 11: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

In this “butterfly type” halo CME,the axis was about 450 off

Page 12: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

2 lobes under a common halo envelope.The source was oriented almost parallel to the lobes’

axis.

Page 13: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

The source axis is perpendicular

to the lobes’ axis

Page 14: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

One more example: a “butterfly-type” halo CME, on the backside

Page 15: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

A perfect halo, originating close to to disc center

Page 16: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

A halo CME, “cannibalizing” a limb

CME

Close relatives of “global” CMEs: Cannibals!

Gopalswamy, 2000

Page 17: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

A halo CME, “cannibalizing” a limb

CME

Close relatives of “global” CMEs: Cannibals!

Note: the “light bulb” CME had occurred behind the limb

Gopalswamy, 2000

Page 18: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

2 succeeding halo CMEs, “cannibalizing” a

limb CME

Close relatives of “global” CMEs: Cannibals!

Gopalswamy, 2000

Page 19: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

Suggestion: “…the chains are visible manifestations of separators or quasi-separatrix layers formed between different interacting

large-scale magnetic flux systems in the evolving global magnetic solar atmosphere”

Chertok, 1997 ff

Other suspects in context with global CMEs: magnetic chains

Page 20: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

Bothmer and Schwenn, 1998

Sketch showing the possible large-scale topologyof a flux-rope magnetic cloud

Alternative explanation of “global” CMEs:

new perspective on flux ropes

Page 21: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

Erupting flux rope with its legs connected to the sun

Alternative explanation of “global” CMEs:

new perspective on flux ropes

Chen et al., 1993 ff

Page 22: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

This CME (on September 9th, 1997) was well observed by the Mark 3 and LASCO coronagraphs. It fits well to the erupting flux rope

model

Chen et al., 2000

Page 23: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

This is what the flux rope model would predict how this CME should look like

Chen et al., 2000

Page 24: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

1. A typical flux rope CME seen from the side, I.e. above one limb

Different perspectives of flux rope CMEs

Page 25: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

2. An extended flux rope CME seen from the front or

back side. Note the 2D rope structure and the engulfing 3D halo

CME structure.

“Global” CMEs:

a projection

effect!

Page 26: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

“Global” CMEs:

a projection

effect!

Page 27: Rainer Schwenn Max-Planck-Institut für Aeronomie Katlenburg-Lindau International Solar Cycle Studies 2001 (ISCS), June 13-16, 2001 Longmont, Colorado CME.

Rainer SchwennMax-Planck-Institut für Aeronomie

Katlenburg-Lindau

CME Mythology: Do Global CMEs or Sympathetic CMEs Exist?

My answer is: No.

They are probably just head-on (or head off…?) flux rope halo CMEs. Let’s see what they look like from

different perspectives, i.e., STEREO and Solar Orbiter.

STAY TUNED!