Titlebook: Solar Gamma-, X-, and EUV Radiation; Sharad R. Kane Book 1975 International Astronomical Union 1975 Corona.Solar flare.Variation.gamma-ray

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G. E. BruecknerLichtmikroskopes heranreicht. Da außerdem das Cytoplasma der Bakterien ungewöhnlich reich an Nukleinsäure ist, kann innerhalb der Innenstruktur von Bakterien mit konventionellen Färbemethoden unter Benutzung basischer Farbstoffe nicht weiter differenziert werden. Mit der Entwicklung des Elektronenmi

Creditee

Kenneth G. Widingrch Nachweis spezifischer Antikörper des Patienten gegen Erregerantigene. Trotz großer Fortschritte bei der Zurückdrängung oder Ausrottung einstmals verheerender Infektionen, z. B. Pocken, sind Infektionserreger nach wie vor häufige Erkrankungs- und Todesursachen, z. B. Tuberkulose, Malaria, Hepatit

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Solar Activity Observed in X-Rays and the EUV from OSO 7therefore must be maintained by a more or less continuous injection of energy..A nested arch structure is also indicated for XUV flares of the two-component type, which likewise may require continuous energy input since conduction cooling should otherwise be very rapid. Multiple spikes during the im

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CEDE

Flare-Like Ultraviolet Spectra of Active Regionsare are reproduced in Figure 2. One recognizes that the transition zone instability started intermittently prior to the flare and could be seen during short time intervals long after the flare had ceased.

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Fe , Emission in Solar Flares Observed with the NRL/ATM XUV Slitless Spectrographated electron density is 5×10. cm...The Fe . emission was visible 8 to 10 min as compared with a calculated cooling time by conduction of only 5 min. The lengthened life of the emission may be associated with the observed ‘turbulence’, which inhibits the heat conduction, or alternatively, with a slo

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D. H. Brabban,E. B. Dorling,W. M. Glencross,J. R. H. Herring

Buttress

Spatially Resolved X-Ray Spectra of Coronal Active Regionstions allowed the spot corresponding to the X-ray collimator axis to be identified and so the collimator pointing direction on the solar disc was controlled from the ground by means of commands sent to the rocket.

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