Overlooked astrophysical signatures of axion(-like) particles

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2ndPower-law index n of L x ~ B n =ƒ(time) YOHKOH / XRTThe relation between the solar soft X-ray flux (below ~4.4keV) …and B canbe approximated by a power law with an averaged index close to 2.Benevolenskaya, Kosovichev, Lemen, Scherrer, Slater ApJ. 571 (2002) L181Note: axion-to-photon oscillation ∝ B 2 e.g., in CASTDHH Hoffmann, K. Z., Nucl. Phys. B Suppl. 151 (2006) 35911 years solar cycle?
FLARES origin?L x↑3rdThe Electron “Problem”e - flux~10 5 × hard X-raysfrom Bremsstrahlung! B maxRebinned peak flare X-ray intensity vs. B maxD. Mason et al., ApJ. 645 (10.7.2006)1543 B 2 correlationG. Emslie (2005 2005)http://www.astro.auth.gr/%7Evlahos/ascona/memberstalks/energeticsEmslie.ppt#366,8
Page 1: Overlooked astrophysical signatures
Page 4: How can ~axions show-up in celestia
Page 7 and 8: On solving the Coronal Heating Prob
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Page 11 and 12: 2 nd component
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Page 15 and 16: Quiet-Sun X-ray observationsRHESSIT
Page 17 and 18: FLARESThe Electron “Problem”G.
Page 19 and 20: Flares T flare ≈ T core199 flares
Page 21 and 22: 1 st component ~B 2 4 cases ~ consi
Page 23: The long-term evolution of AR 7978
Page 27 and 28: Magnetic field computed from the Ze
Page 29 and 30: Solar metalicity
Page 31 and 32: Serious disagreement between the pr
Page 33 and 34: The Ne abundance has been inferred
Page 35 and 36: Solar ν’s & X-raysoscillations /
Page 37 and 38: X-raysYohkohSXT S60 o N60 oSXT equa
Page 41 and 42: Solar Corona proxy Fe green line19
Page 43 and 44: By general agreement: the energy of
Page 45 and 46: Gamma rays from the neutralino dark
Page 47: Are these astrophysical ~axion sign
Page 50: X-ray mysteries:• Class 0 protost

Overlooked astrophysical signatures of axion(-like) particles

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