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. 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)?

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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.