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Contribution Poster
Observations of the December 2006 particle events at high latitudes with the KET aboard Ulysses
Speakers
- Prof. A. STRUMINSKY
Primary authors
- Prof. Bernd HEBER (CAU Kiel)
Co-authors
- Prof. A. STRUMINSKY (Institute of Space Research, Russian Academy of Sciences, Profsoyuznaya Street, 84/32, Moscow 117997, Russia)
- Mr. R. MUELLER-MELLIN (CAU Kiel)
- Dr. R. GOMEZ-HERRERO (CAU Kiel)
- Dr. A. KLASSEN (CAU Kiel)
- Prof. R. WIMMER-SCHWEINGRUBER (CAU Kiel)
- Dr. C. STEIGIES (CAU Kiel)
- Prof. W. DRÖGE (Institut für Theoretische Physik und Astrophysik, Universität Würzburg, 97074 Würzburg)
- Dr. O. MALANDRAKI (Research and Scientific Support Department of ESA, ESTEC, Noordwijk, The Netherlands)
- Dr. R. MARSDEN (Research and Scientific Support Department of ESA, ESTEC, Noordwijk, The Netherlands)
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Abstract content
An unexpected rise of solar activity close to its minimum in December 2006 resulted in four X-class flares and four energetic particle events. These events were observed close to Earth and above 70 degree South by the Ulysses spacecraft, which was at a heliocentric distance of 2.8 AU at that time. Three out of these four events produced significant intensity increases up to several hundred MeV/nucleon for protons and alpha-particles and several 10 MeV for electrons at high southern latitudes. They were associated with X9.0, X6.5, and X3.4 flares from the AR 10930, coronal type II bursts and strong microwave emission on 5-th, 6-th, and 13-th December, respectively. Although these flares have similar X-ray and microwave time profiles, the particle event on December 13 is the weakest among the three at Ulysses, but it is the largest near Earth. It produced a ground level event leading to an intensity increase of about 34 % in the Kiel neutron monitor. In contrast the December 6 particle event was the largest at Ulysses. We will discuss these events in context of previous Ulysses observations and its consequences for particle propagation to solar Polar Regions.
If this papers is presented for a collaboration, please specify the collaboration
KET
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 1 (SH), pages 217-220