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| 1 | Setting up of a probabilistie neural network for sensor fault detection including operation with compo- nent faults 显示文摘 | Romesis C Mathioudakis K | 2003 | J Eng Gas Turbines Power2003，125，3： | 1 |
| 2 | Nanomechanical properties of multilayered amorphous carbon structures显示文摘 | Mathioudakis C Kelires P C Panagiotatos Y | 2002 | Physical Review B2002，65，205203： | 1 |
| 3 | Fist record of the apple stem pitting virus(ASPV)in quince in Greece显示文摘 | Mathioudakis M M Maliogka V I Dovas C I | 2006 | Journal of Plant Pathology2006，88，2： | 1 |
| 4 | “Glandular intoxication' following emergenttracheotomy during transsphenoidal surgery for acromegaly:Cushing's 1910unrefx-oized case of thyroid storm?显示文摘 | Pendleton C Mathioudakis N | 2012 | Pituitary2012，23，5： | 1 |
| 5 | Nanomechanical properties of muhilayered amorphous carbon structures显示文摘 | MATHIOUDAKIS C KELIRES P C PANAGIOTATOS Y | 2002 | Physical Review B2002，65，20： | 1 |
| 6 | Fist record of the apple stem pitting virus(ASPV)in quince in Greece显示文摘 | Mathioudakis M M Maliogka V I Dovas C I | 2006 | Journal of Plant Pathology2006，88，2： | 1 |
| 7 | Bayesian Network Approach for Gas Path Fault Diagnosis显示文摘 | Romessis C Mathioudakis K | 2006 | Journal of Engineering for Gas Turbines and Power2006，128，1： | 1 |
| 8 | Structure, stability, and stress properties of amorphous and nano- structured carbon films 显示文摘 | Fyta M G Mathioudakis C Kopidakis G Kelires P C | 2005 | Thin Solid Films2005，482，12： | 1 |
| 9 | Pepino mosaic virus capsid protein interacts with a tomato heat shock protein cognate 70显示文摘 | Mathioudakis M M Veiga R Ghita M Tsikou D Medina V Canto T Makris A M Livieratos I C | | Virus Research0，163，1： | 1 |
| 10 | First record of the apple stem pitting virus(ASPV) in quince in Greece显示文摘 | Mathioudakis M M Maliogka V I Dovas C I | 2006 | Journal of Plant Pathology2006，88，2： | 1 |
| 11 | Can active late-type stars contribute to the Galactic lithium abundance?显示文摘Lithium abundances in our Galaxy and especially 6 Li abundances provide important constraints on our understanding of Big Bang Nucleosynthesis(BBNS),stellar evolution and the creation of light elements by cosmic rays in the ISM.~6 Li has been detected in energetic solar events,one chromospherically active binary and several dwarf halo stars.Continuing our work on active late-type stars with high lithium abundances,we expand our study to consider if the flare origin of lithium created by spallation can contribute significantly to the Galactic abundance of lithium.We previously derived ~6 Li/~7 Li=0.030 ± 0.010 for active K dwarf GJ 117 using VLT UVES observations.We find^6 Li/~7 Li ratios of 0.02 and 0.10 for two other stars in our sample,GJ 182 and EUVE J1145-55.3 A,respectively.Considering that these later type,active stars have significant flare rates and stellar winds,we have estimated the contribution of these stars to the Galactic lithium abundance.Given that K and M stars comprise over 84% of our Galaxy and that many of these can have significant stellar winds,we conclude that spallation in stellar flares can contribute 1% and up to 5% of the Galactic lithium abundance. | Darnell E.Kelly Damian J.Christian Mihalis Mathioudakis Darko Jevremovi′c | 2020 | Research in Astronomy and Astrophysics2020，20，7： | 0 |
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