Titlebook: Mass Supply and Flows in the Solar Corona; The 2nd SOHO Worksho B. Fleck,G. Noci,G. Poletto Book 1994 Springer Science+Business Media Dordr

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Observed Redshifts of Transition Region/Corona Linesainty in the available laboratory wavelength of the intercombination line at 1218 Å (2S. .S.-2s2p .P.)..The observed shift in 0 V is compared with corresponding measurements of lines formed at other temperatures (Si IV, C IV, N IV, 0 IV, and Fe XII). Large variations in the shift are found along the

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Book 1994 solving open problems. Oral pa­ pers and poster presentations were followed by Working Group sessions. On the last day of the Workshop the Group Leaders reported on the activities of their Working Group. These proceedings include most of the papers presented at the Work­ shop, including the poster

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ht help in solving open problems. Oral pa­ pers and poster presentations were followed by Working Group sessions. On the last day of the Workshop the Group Leaders reported on the activities of their Working Group. These proceedings include most of the papers presented at the Work­ shop, including the poster 978-94-010-4401-1978-94-011-0930-7

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The Scientific Payload of the Space-Based Solar and Heliospheric Observatory (SOHO)me (STSP), the first “Cornerstone” of ESA’s long-term programme “Space Science-Horizon 2000”. The principal scientific objectives of the SOHO mission are: a) a better understanding of the structure and dynamics of the solar interior using techniques of helioseismology, and b) a better insight into t

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Magnetic Fine Structures in Coronal Loopsn of field-aligned electric currents into the lower atmosphere is discussed. It is argued that currents strong enough to heat the corona can persist only for short periods of time. The formation of thin current sheets is discussed. It is argued that photospheric magnetic structures (flux tubes) play

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