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, 1992

Framhlið kápu
Jeffrey 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
22
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
Index of Keywords and Subjects
645
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