Analysing CME deflections

Sieyra1, Cecere1, Cremades2, Mierla3, Sahade1, Costa1 and PROBA-2team3

1. IATE (CONICET/UNC) - OAC (UNC) - Argentina2. FRM (UTN) - CONICET - Argentina

3. Royal Observatory of Belgium

IATE/Argentina ↔ ROB/Belgium – November 13, 2018

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Project Analysing CME deflections

Objectives

Objective of the project

Study the influence of the coronal environment in the early development ofCMEs to better understand the deviation between the source region(filament or active region) and the non-radial direction of propagation ofCME (i.e. deflection).

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Project Analysing CME deflections

Analyzed period of time

STEREO’s locations

2010/10/01 2011/10/01

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Project

Solar cycle

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Selection of Events

Deflection

CME deviation from the source region (filament)

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Methodology

Analysis: Triangulation

Prominence in SWAP & EUVI A

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Methodology

Analysis: Triangulation

Core of the CME in LASCO C2 & COR1 A

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Methodology

Analysis: Forward Modeling

CME in COR2 B & LASCO C2 & COR2 A

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Methodology

Analysis: Magnetic environment

Presence of CHs and ARs and PFSS

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Methodology

Analysis: Magnetic environment

Carrington map

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Results

CME deflection

Latitude vs time & Longitude vs time

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Results

Prominence

Latitude vs time & Longitude vs time

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Results

Preliminary results

The magnetic environment affects the dynamics of the CME:

CHsStreamers

The evolution of the prominence morphology may or may notaccompany deviation of the CME.

Work in Progress:

We are analyzing 10 more deflection events to understand relatedconditioning factors.

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Results

Preliminary results

The magnetic environment affects the dynamics of the CME:

CHsStreamers

The evolution of the prominence morphology may or may notaccompany deviation of the CME.

Work in Progress:

We are analyzing 10 more deflection events to understand relatedconditioning factors.

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Results

Thank you!

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