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Explaining Solar Neutrinos with Heavy Higgs Masses in Partial Split Supersymmetry

is directly connected to a small solar neutrino mass differenceΔ​ms​o​l2\Delta m_{sol}^{2}. Therefore, the small observed value forΔ​ms​o​l2\Delta m_{sol}^{2}favors large values ofmAm_{A}up to 6 TeV. Such large values formAm_{A}would make PSS virtually indistinguishable from SS by using any observable other than neutrino masses....

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Spectral Characteristics of a Rotating Solar Prominence in Multiple Wavelengths

Korhonen, T. K., Lindberg, B., & Petterson, B. 2003, in Proc. SPIE, Vol. 4853, Innovative Telescopes and Instrumentation for Solar Astrophysics, ed. S. L. Keil & S. V. Avakya... 785, L2Su et al. (2012)Su, Y., Wang, T., Veronig, A., Temmer, M., & Gan, W. 2012, 756, L41Terradas et al. (2016)Terradas, J., Soler, R., Luna, M., et al. 2016, 820, 125Turk...

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[1608.01476] Radiation effects on the Gaia CCDs after 30 months at L2

as well as correlating these CTI diagnostic results with solar proton event data. We show that L2-directed solar activity has been relatively low since launch, and radiation damage (so far) is less than originally expected. Despite this, there are clear cases of correlation between earth-directed solar coronal mass ejection events and abrupt changes in...

Distributed autonomous relative navigation method for spacecraft formation near solar L2