Physics of Solar and Stellar Coronae: G.S. Vaiana Memorial Symposium: Proceedings of a Conference of the International Astronomical Union, Held in Palermo, Italy, 22–26 June, 1992Jeffrey L. Linsky, Salvatore Serio Springer Science & Business Media, 6. des. 2012 - 650 síður The original plans for a meeting to celebrate the second centenary of the As tronomical Observatory of Palermo were for a celebration with a double character. The gathering was to have both a historical character, appropriate for a bicenten nial, and a technical character, to note and chronicle the new phase of the history of the Observatory, which has prospered in parallel with the development of this fairly recent topic in astronomical research, the physics of stellar and solar coronae. After the untimely death of the Observatory's Director, Giuseppe S. Vaiana (Pippo to his many friends), a number of colleagues and friends insisted that the celebration should nevertheless be held and should be dedicated to this farsighted scientist who stimulated the development of coronal physics from the early x-ray observations of the solar corona to the recognition of coronae as an observable feature of nearly all stars. This memorial dedication did not change the character of the meeting, which was held in Palermo from 22 to 26 June 1992; as his contributions are very alive in the papers presented at the meeting and collected here, Pippo Vaiana has certainly achieved his place in the history of Astronomy. |
Efni
On the History of the Palermo Astronomical Observatory 21 | 20 |
Bodes Law and the Discovery of Ceres | 35 |
The NineteenthCentury Birth of Astrophysics | 47 |
NIXT High Resolution Observations | 70 |
High Resolution Thermally Differentiated Images of the Chromosphere | 83 |
New Aspects of Solar Coronal Physics Revealed by YOHKOH | 97 |
85 | 111 |
Dynamics of the Solar Corona Observed with the YOHKOH Soft Xray | 113 |
132 | 268 |
Results from an Optical | 279 |
Photometric and Spectroscopic Observations of Cool Stars Serendipitously | 295 |
Emission up to 18 keV in the Quiescent Xray Spectrum of II Peg | 311 |
ROSAT Observations of LateType Stars 327 | 325 |
ROSAT Observations of the Hyades | 345 |
41 | 346 |
163 | 372 |
103 | 118 |
86 | 129 |
Hard Xray Solar Flares Observed by YOHKOH and Particle Acceleration | 131 |
Properties of SMM Flares | 139 |
Analysis of Flare Evolution in the Emission MeasureTemperature Dia | 147 |
Soft Xray Line Shifts as Signature of the Flare Heating Process | 159 |
Siphon Flow Models of Coronal Loops | 163 |
NonThermal Line Profiles in Solar Flares | 179 |
83 | 184 |
Calibrated Solar EUV Spectrum from SERTS | 195 |
What We Have Learned from PreROSAT | 209 |
Stellar Coronal Xray Spectroscopy | 225 |
91 | 233 |
Xrays and Activity in PreMain Sequence Stars | 249 |
Coronal Stellar Emission in Galaxies | 267 |
57 | 385 |
31 | 459 |
Coronal Heating Mechanisms 515 | 513 |
Chromospheric Heating | 531 |
Mass Loss and Xray Emission from Giants and Supergiants | 549 |
Radiation Driven Winds and Xray Emission from O Stars 563 | 562 |
571 | |
Magnetic Fields and Coronae in LateType Stars 579 | 580 |
67 | 586 |
Thermal Transport in Static Stellar Coronal Loops | 595 |
ThreeDimensional Magnetic Reconnection in a Coronal Neutral Sheet | 611 |
MHD Equilibria in Uniform Gravity | 629 |
645 | |
Aðrar útgáfur - View all
Physics of solar and stellar coronae : G.S. Vaiana Memorial Symposium, held ... Engin sýnishorn í boði - 1993 |
Physics of Solar and Stellar Coronae: G.S. Vaiana Memorial Symposium ... Jeffrey L. Linsky,Salvatore Serio Engin sýnishorn í boði - 2012 |
Common terms and phrases
1993 Kluwer Academic active region active stars Ap.J Astron Astronomy Astrophys Astrophysics binaries chromospheric component convection zone coronal holes coronal loops correlation CVn systems dark channels density detected disk distribution dwarfs dynamo Einstein Observatory electrons emission measure energy evolution EXOSAT Figure flare stars flux Galactic Golub Haisch hard X-ray Harnden heating Hyades images J.F. Linsky Kluwer Academic Publishers late-type stars light curve luminosity functions magnetic field main sequence Micela microflares multilayer non-thermal observations obtained optical Palermo Pallavicini parameters phase photospheric Physics of Solar Piazzi plasma PSPC radio emission reconnection resolution ROSAT Rosner rotation sample scale Schmitt Sciortino Serio eds shows Skylab soft X-ray Solar and Stellar solar flares Solar Phys spatial spectral type spectrum Stellar Coronae structure surface Tauri stars temperature thermal Tsuneta Vaiana variability velocity wavelengths wind X-ray emission X-ray sources Yohkoh