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Monday afternoon heliospheric properties of CMEs DL: Alexis Rouillard (GMU/NRL/NASA): CME classification as a discussion starter. Slow CMEs: blobs, in-out pairs, blow-out, 3-part CMEs. All from flux ropes - Nobody actually disagreed officially. Fast CMEs: a more complicated mess. Lots of discussion: Is it really possible to classify CMEs using their speed since they form a Gaussian or Gaussian-like distribution? Ok for the classification about impulsive vs. gradual events (Jie Zhang). All CMEs, even using this impulsive/gradual classification are similar, just depends how high the reconnection happens (Angelos). Or is there still some fundamental differences between AR CMEs and “quiet Sun” CMEs (Tibor)?

Monday afternoon heliospheric properties of CMEs

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Monday afternoon heliospheric properties of CMEs. DL: Alexis Rouillard (GMU/NRL/NASA): CME classification as a discussion starter. Slow CMEs: blobs, in-out pairs, blow-out, 3-part CMEs. All from flux ropes - Nobody actually disagreed officially. Fast CMEs: a more complicated mess. - PowerPoint PPT Presentation

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Page 1: Monday afternoon heliospheric properties of CMEs

Monday afternoon heliospheric properties of CMEs

• DL: Alexis Rouillard (GMU/NRL/NASA): CME classification as a discussion starter.– Slow CMEs: blobs, in-out pairs, blow-out, 3-part

CMEs. All from flux ropes - Nobody actually disagreed officially.

– Fast CMEs: a more complicated mess.• Lots of discussion: Is it really possible to classify CMEs

using their speed since they form a Gaussian or Gaussian-like distribution? Ok for the classification about impulsive vs. gradual events (Jie Zhang).

• All CMEs, even using this impulsive/gradual classification are similar, just depends how high the reconnection happens (Angelos). Or is there still some fundamental differences between AR CMEs and “quiet Sun” CMEs (Tibor)?

Page 2: Monday afternoon heliospheric properties of CMEs

CME = flux rope?• Do CMEs or flares come first?• Are all CMEs flux rope?

– Brian Wood showed one example of a CME with a clear axis BUT 1 AU reconstruction don’t necessarily give the same axis direction.

Page 3: Monday afternoon heliospheric properties of CMEs

CME = flux rope?• What proofs do we have?

– Does the axis have to be what appear as the axis in the white-light images?

– Can we really infer orientation from density measurements?

– We need remote-sensing of the magnetic field, maybe Faraday rotation.

• Mario Bisi showed the CME events from August 2010.– 6+ CMEs probably contributed– At 1 AU, VEX and ST-B see a RH flux rope but ACE

sees a LH flux rope. Different CMEs?– Alexis mentioned a case from 2008 when STEREO

separation was small and 2 events with different helicity arrived at the same time at Earth...

Page 4: Monday afternoon heliospheric properties of CMEs

Life without STEREO nor HIs• Brian’s example: clear case when not-halo

CMEs are Earth-directed. Clear contribution from the HIs. In theory, only need one continuous monitoring of the heliosphere away from the Sun-Earth line.

• Do CMEs rotate?– Evidence from coronagraphs?– What mechanism would cause rotation

to start farther away in the heliosphere?– One example of 45+ degree rotation

shown by Robin Colaninno.

• Jason Byrne showed kinematics from December 2008 CME: different peak speed from Ying Liu’s model. Also discussed problem of determining CME kinematics.