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Temporal Offsets between Maximum CME Speed Index and Solar, Geomagnetic, and Interplanetary Indicators during Solar Cycle 23 and the Ascending Phase of Cycle 24 View all abstracts by submitter

Ali Kilcik   Submitted: 2016-04-20 23:52

On the basis of morphological analysis of yearly values of the maximum CME (coronal mass ejection) speed index, the sunspot number and total sunspot area, sunspot magnetic field, and solar flare index, the solar wind speed and interplanetary magnetic field strength, and the geomagnetic Ap and Dst indices, we point out the particularities of solar and geomagnetic activity during the last cycle 23, the long minimum which followed it and the ascending branch of cycle 24. We also analyze temporal offset between the maximum CME speed index and the above-mentioned solar, geomagnetic, and interplanetary indices. It is found that this solar activity index, analyzed jointly with other solar activity, interplanetary parameters, and geomagnetic activity indices, shows a hysteresis phenomenon. It is observed that these parameters follow different paths for the ascending and the descending phases of solar cycle 23. It is noticed that the hysteresis phenomenon represents a clue in the search for physical processes responsible for linking the solar activity to the near-Earth and geomagnetic responses.

Authors: A. Özgüç, A. Kilcik, K. Georgieva, B. Kirov
Projects: None

Publication Status: Accepted for publication by Solar Physics
Last Modified: 2016-04-26 07:40
Go to main E-Print page  The apparent critical decay index at the onset of solar prominence eruptions  Constraints on energy release in solar flares from RHESSI and GOES X-ray observations I. Physical parameters and scalings  Edit Entry  Download Preprint  Delete Entry 

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