MPAe T1ex127-.45ex51275atigkeitsbericht 2002/2003 - Max-Planck ...

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II INHALT/CONTENTS Plasma outflow and mass flux in an equatorial coronal hole . . . . . . . . . . . . . . . . . . . . . . . . 28 Network structures and Doppler shifts in solar equatorial coronal holes . . . . . . . . . . . . . . . . . . 29 Spatial mapping of scattering polarisation at the solar limb . . . . . . . . . . . . . . . . . . . . . . . . 29 Systematic exploration of the second solar spectrum . . . . . . . . . . . . . . . . . . . . . . . . . . . . 30 Transition region small-scale dynamics as seen by SUMER on SOHO . . . . . . . . . . . . . . . . . . 30 On the widths of the Mg X lines near 60 nm in the corona . . . . . . . . . . . . . . . . . . . . . . . . . 31 Observations of small-scale ejecta using SUMER, UVCS and LASCO . . . . . . . . . . . . . . . . . . 32 Characteristics of solar explosive events . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32 Postflare supra-arcade dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32 Relationship between variability of intensity and Doppler shift in EUV-spectra . . . . . . . . . . . . . . 33 Polarimetry of the solar corona . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 33 Are large velocity distribution anisotropy really present in the solar corona? . . . . . . . . . . . . . . . 33 Coronal shock waves associated with Coronal Mass Ejections (CMEs) . . . . . . . . . . . . . . . . . . 34 Spectroscopic observations of heating and cooling in coronal loops . . . . . . . . . . . . . . . . . . . . 34 Slow-mode standing waves in hot coronal loops observed by SUMER . . . . . . . . . . . . . . . . . . 35 Coronal holes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 35 Magnetic field modelling, stereoscopy and tomography for SECCHI on STEREO . . . . . . . . . . . . 36 Vector tomography for the coronal magnetic field . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36 Solar wind and heliosphere Solar corona and solar wind . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 37 Ion velocity distributions and cyclotron wave absorption or opacity . . . . . . . . . . . . . . . . . . . . 37 Interplanetary and solar surface properties of coronal holes . . . . . . . . . . . . . . . . . . . . . . . . 39 Dynamics of the solar corona . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 40 EUV post-eruptive arcades: Physical properties and association with coronal mass ejections . . . . . . . 40 3D magnetic field configuration in coronal mass ejections . . . . . . . . . . . . . . . . . . . . . . . . . 41 Properties of interplanetary coronal mass ejections . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41 Geoeffectice interplanetary structures: Their origins on the Sun and in the solar wind . . . . . . . . . . 42 Long term solar variations Reconstruction of past solar activity from terrestrial records of 10 Be . . . . . . . . . . . . . . . . . . . 43 Reconstruction of solar irradiance variations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44 Solar variability and global warming . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44 Surface magnetic fields cause UV radiance of the quiet Sun to vary over the solar cycle . . . . . . . . . 44 Total magnetic flux of the Sun . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 45 A relationship between solar cycle strength and length . . . . . . . . . . . . . . . . . . . . . . . . . . . 45 Was one sunspot cycle in the 18th century really lost? . . . . . . . . . . . . . . . . . . . . . . . . . . . 46 Ongoing future missions Solar Ultraviolet Measurements of Emitted Radiation – SUMER . . . . . . . . . . . . . . . . . . . . . 46
INHALT/CONTENTS III LASCO (Large Angle and Spectrometric COronagraph on SOHO) . . . . . . . . . . . . . . . . . . . . 46 MICA (Mirror Coronagraph for Argentina) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47 Sunrise: A balloon-borne telescope for high-resolution observations of the Sun . . . . . . . . . . . . . 47 Tenerife Infrared Polarimeter (TIP) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48 The NASA STEREO Mission . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48 Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) for STEREO – SCIP . . . . . 49 Solar Orbiter: A high-resolution mission to the Sun and inner heliosphere . . . . . . . . . . . . . . . . 51 Technological pre-studies for the Solar Orbiter VIM instrument . . . . . . . . . . . . . . . . . . . . . . 53 Stars and solar-stellar connections Understanding solar variability as groundwork for planet transit detection . . . . . . . . . . . . . . . . 53 Stellar wind regime at the orbit of close-in extrasolar planets . . . . . . . . . . . . . . . . . . . . . . . 54 Constraints set by the Sun and degenerate stars on new couplings between electromagnetism and gravity 54 Asteroseismology: Determination of cool star rotation properties . . . . . . . . . . . . . . . . . . . . . 55 Spot sizes on Sun-like stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 55 Magnetically trapped circumstellar matter around hot stars . . . . . . . . . . . . . . . . . . . . . . . . 56 Weak magnetic fields in white dwarfs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56 A stream of particles from the β Pictoris disc . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56 2 Planeten, ihre natürlichen Satelliten und Kometen/ Planets, their moons and comets Schwerpunktthema: SMART-1 – Europas Mission zum Mond . . . . . . . . . . . . . . . . . . . . . . . 58 Highlight: SMART-1 – Europe’s Mission to the Moon . . . . . . . . . . . . . . . . . . . . . . . . . . . 60 Terrestrial planets research – Venus Analyser of Space Plasmas and Energetic Atoms ASPERA-4 for Venus Express . . . . . . . . . . . . . 63 Terrestrial planets research – Earth Power requirement of planetary dynamos . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 63 Stochastic resonance in a bistable geodynamo model . . . . . . . . . . . . . . . . . . . . . . . . . . . 63 Comparison of mean-field theory with direct numerical dynamo calculations . . . . . . . . . . . . . . . 64 Tomography and geodynamic models of the Eifel Plume . . . . . . . . . . . . . . . . . . . . . . . . . 65 Terrestrial planets research – Mars Three-dimensional evolution models of convection in the Martian mantle . . . . . . . . . . . . . . . . . 65 Mars Climate Simulator: Investigation of the current and ancient Martian climate, its stability and mechanisms of changes by means of a modular planet simulator model . . . . . . . . . . 65 Mesoscale modelling of Martian fog formation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 66 Development of the LTE version of the general circulation and climate model of the Martian atmosphere MART-ACC . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 67 Implementation of non-LTE radiation transport into the general circulation and climate model of the Martian atmosphere MART-ACC . . . . . . . . . . . . . . . . . . . . . . . . . . . . 67 LTE radiative heating rates based on MGS/TES nadir temperature measurements . . . . . . . . . . . . 68
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140 1. August 1999 - 31. Juli 2002.
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142 A. Zhukov, November 2002. EU-IN
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158 to CNES, nicht genehmigt, 2002.
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