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J_rod7 · 04-29-2009, 01:01 AM

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Well for one, among some others here, I'm MAD-AS HELL that those so-called "elite" are using our Tax dollars on their extravagant survival "Arks."

Those of us left on the surface may be facing a scorched Earth from expected Solar Coronal Mass Ejections (CMEs), possible within the next 3-5 years.

Proceedings of the International Astronomical Union (2008), 4:475-477 Cambridge University Press
Copyright © International Astronomical Union 2009
doi:10.1017/S174392130902972X
Contributed Papers

SEPs and CMEs during cycle 23

Pertti Mäkeläa1, Nat Gopalswamya2, Seiji Yashiroa3, Sachiko Akiyamaa1, Hong Xiea1 and Eino Valtonena4

a1 Dept. of Physics, Catholic University of America, 200 Hannan Hall, Washington, DC 20064, USA email: pertti.makela@nasa.gov, sachiko.akiyama@nasa.gov, hong.xie@nasa.gov

a2 Nasa Goddard Space Flight Center, Code 695, Greenbelt, MD 20771, USA email: nat.gopalswamy@nasa.gov

a3 Interferometrics, Inc, 13454 Sunrise Valley Drive, Herndon, VA 20171, USA email: seiji.yashiro@nasa.gov

a4 Dept. of Physics & Astronomy, University of Turku, Vesilinnantie 5, FI-20014 Turku University, Finland email: eino.valtonen@utu.fi

Abstract

We present a study of solar energetic particles (SEPs) in association with coronal mass ejections (CMEs) and type II radio bursts. The particle and CME observations cover the years 1996–2007. We find that heavy-ion events in association with type II bursts and proton events are produced in more western and most energetic CMEs. In addition, the source distribution of type II associated proton events with heavy ions reminds the source distribution expected for events with flare particles. Therefore, the estimation of relative contributions by flares and shocks in SEP events and separation of suggested different particle acceleration models is complicated.

Keywords: Acceleration of particles; Sun: coronal mass ejections (CMEs); Sun: particle emission

I don't know HOW DEEP we would have to dig to escape immediate immolation, but there would not be much left to survive with upon re-emerging.

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04-29-2009, 01:01 AM	#11
J_rod7 Avalon Senior Member Join Date: Sep 2008 Location: Florida, USA Posts: 301	Re: huge underground base ***** * * Well for one, among some others here, I'm MAD-AS HELL that those so-called "elite" are using our Tax dollars on their extravagant survival "Arks." Those of us left on the surface may be facing a scorched Earth from expected Solar Coronal Mass Ejections (CMEs), possible within the next 3-5 years. Proceedings of the International Astronomical Union (2008), 4:475-477 Cambridge University Press Copyright © International Astronomical Union 2009 doi:10.1017/S174392130902972X Contributed Papers SEPs and CMEs during cycle 23 Pertti Mäkeläa1, Nat Gopalswamya2, Seiji Yashiroa3, Sachiko Akiyamaa1, Hong Xiea1 and Eino Valtonena4 a1 Dept. of Physics, Catholic University of America, 200 Hannan Hall, Washington, DC 20064, USA email: pertti.makela@nasa.gov, sachiko.akiyama@nasa.gov, hong.xie@nasa.gov a2 Nasa Goddard Space Flight Center, Code 695, Greenbelt, MD 20771, USA email: nat.gopalswamy@nasa.gov a3 Interferometrics, Inc, 13454 Sunrise Valley Drive, Herndon, VA 20171, USA email: seiji.yashiro@nasa.gov a4 Dept. of Physics & Astronomy, University of Turku, Vesilinnantie 5, FI-20014 Turku University, Finland email: eino.valtonen@utu.fi Abstract We present a study of solar energetic particles (SEPs) in association with coronal mass ejections (CMEs) and type II radio bursts. The particle and CME observations cover the years 1996–2007. We find that heavy-ion events in association with type II bursts and proton events are produced in more western and most energetic CMEs. In addition, the source distribution of type II associated proton events with heavy ions reminds the source distribution expected for events with flare particles. Therefore, the estimation of relative contributions by flares and shocks in SEP events and separation of suggested different particle acceleration models is complicated. Keywords: Acceleration of particles; Sun: coronal mass ejections (CMEs); Sun: particle emission I don't know HOW DEEP we would have to dig to escape immediate immolation, but there would not be much left to survive with upon re-emerging. * * ***** Last edited by J_rod7; 04-29-2009 at 01:04 AM.