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The VTT Helioseismology Concept with HELLRIDE and CARMA J.Staiger , KIS Freiburg. The VTT Helioseismology Concept. KIS Helioseismology Group: Markus Roth Gisela Baumann Hanspeter Doerr Kolja Glogowski Wiebke Herzberg Ariane Schad Aneta Wisniewska Wolfgang Zima
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The VTT HelioseismologyConcept withHELLRIDEandCARMA J.Staiger, KIS Freiburg
The VTT HelioseismologyConcept KIS Helioseismology Group: Markus Roth Gisela Baumann Hanspeter Doerr Kolja Glogowski Wiebke Herzberg Ariane Schad Aneta Wisniewska Wolfgang Zima Joachim Staiger
The VTT HelioseismologyConcept KIS Helioseismology Research: - Global / LocalHelioseismology - Seismologyof Stars - Waves in the Solar Atmosphere (new)
The VTT HelioseismologyConcept Vacuum Tower Telescope
The VTT HelioseismologyConcept HELLRIDE
The VTT HelioseismologyConcept Vacuum Tower Telescope
The VTT HelioseismologyConcept Vacuum Tower Telescope Current Operation: Primary KIS ObservingFacility Future Option: Observing time available VTT advantage: Establishedtechnology
The VTT HelioseismologyConcept Primary VTT Scientific Target: Observation ofatmosphericwaves atfine-grainedverticalresolutionwith large FOV
The VTT HelioseismologyConcept Instrument Requirements: Multiline Operation
The VTT HelioseismologyConcept New Instrument: Etalon-based 2D-Spectrometer HELLRIDE HELioseimicLarge RegionsInterferometricDEvice
The VTT HelioseismologyConcept Development Focus: Low Numberof Optical Components Easy Handling
The VTT HelioseismologyConcept HELLRIDE Instr. Features: Dual Etalon Configuration Manufacturer: IC Optical Spectral Range: 530 nm – 860 nm Gaps: 1.4 , 0.25 mm
The VTT HelioseismologyConcept HELLRIDE Instr. Features: Dual Etalon Configuration Manufacturer: IC Optical Spectral Range: 530 nm – 860 nm Gaps: 1.4 , 0.25 mm
The VTT HelioseismologyConcept HELLRIDE Instr. Features: Collimated Beam Layout
The VTT HelioseismologyConcept HELLRIDE Instr. Features: Cartesian Filter-“Wheel“ Dual Stepper Drive Spatialresolution: 0.0004 mm 16 Filter Mounts
The VTT HelioseismologyConcept HELLRIDE Test 2009 16 Spectral Lines , 60 sec Cadence Spectral Lines: 517.2 nm Mg I 20 Scansteps 538.0 nm C I 15 Scansteps 538.1 nm Fe I 15 Scansteps 538.2 nm Ti I 15 Scansteps 543.4 nm Fe I 10 Scansteps 557.6 nm Fe I 20 Scansteps 589.6 nm Na I 30 Scansteps 590.0 nm Na I 30 Scansteps 630.1 nm Fe I 20 Scansteps 630.15 nm Telluric 15 Scansteps 630.2 nm Fe I 15 Scansteps 654.5 nm H-Alpha 25 Scansteps 632.0 nm He-Ne 15 Scansteps 709.1 nm Fe I 20 Scansteps 777.1 nm Fe I 20 Scansteps 777.2 nm Fe I 10 Scansteps
The VTT HelioseismologyConcept HELLRIDE Test Setup 2009 Multilevel P-Mode evidence
The VTT HelioseismologyConcept HELLRIDE Instr. Features: Camera Mount 4-Axis Mount CCD: Dalsa 1M30
The VTT HelioseismologyConcept HELLRIDE Instr. Features: SyntheticAperture Goal: Enlarge CCD FOV (100“ square) Procedure: Tiling Test: 300“ square 2 Bands 60 sec cadence
The VTT HelioseismologyConcept HELLRIDE Instr. Features: Velocity Drift Compensation Laser mountedto filter-matrix Laser-line scanne likeabsorptionline
The VTT HelioseismologyConcept HELLRIDE Instr. Features: Velocity Drift Compensation
The VTT HelioseismologyConcept HELLRIDE Instr. Features: Embedded Device Simulation -
The VTT HelioseismologyConcept HELLRIDE Instr. Features (future): Fast Filter Displacement -
The VTT HelioseismologyConcept HELLRIDE Instr. Features (future): RealtimeVelocityMaps Goal: Storage Reduction Speed Improvement Quality Monitoring Remote Operation
The VTT HelioseismologyConcept HELLRIDE Instr. Features (future): Remote Control Motivation: Easy Adjustments Remote Maintenance Device-VTT Coupling Remote Operation Properties: TCP/IP Berkley Unix Sockets HTTP-type ASCII Protocol
The VTT HelioseismologyConcept HELLRIDE Instr. Features (future): Online Support Docu -
The VTT HelioseismologyConcept HELLRIDE Instr. Features (future): TabletUsage -
The VTT HelioseismologyConcept HELLRIDE Instr. Features (future): TabletUsage -
The VTT HelioseismologyConcept HELLRIDE Instr. Features: New Finesse Procedure
The VTT HelioseismologyConcept HELLRIDE Instr. Features: New Finesse Procedure Adjust Plate Parallelity No Scanning Few Components
The VTT HelioseismologyConcept HELLRIDE Instr. Features (future): ‘Abs. HeliographicPointing‘ - Problem: Slow lateral FOV driftswith time Origin: Unbalanced thermal loads Approach: Project CARMA
The VTT HelioseismologyConcept HELLRIDE in servicenowat VTT
The VTT HelioseismologyConcept First campaigndedicatedtodoctoralthesis
The VTT HelioseismologyConcept Enhanced TelescopePointing: Project CARMA CorrelativeArea MAtching
The VTT HelioseismologyConcept CARMA Motivation: Image Drift Problem: Slow Migration of FOV with time, Not compensatedbyTelescopeGuiding
The VTT HelioseismologyConcept CARMA Motivation: Not a problemforpronouncedfeatures But a problemforquietsunobservations And a problemforsynchronizedobservations.
The VTT HelioseismologyConcept VTT Drift NumericalExample:
The VTT HelioseismologyConcept Problem Source: Guiding Beam not identicalto Main Beam
The VTT HelioseismologyConcept CARMA Hypothesis: Continuumbrightnessfluctuationsareuniquepositionidentificator
The VTT HelioseismologyConcept CARMA Test Results 2012 with SDO:
BEOBACHTUNGEN MIT DEM VTT - Erneuerung der Steuerung - Neue instrumentelle Nutzungsmöglichkeiten Helioseismologie (HELLRIDE) Präzisions-Pointing (CARMA)
VTT Nachführung Aufgabenstellung der Nachführung Anfahren einer heliographischen Position Fixieren der Position
VTT Nachführung Probleme Initialisierung Betriebs-Stabilität Langzeit-Genauigkeit
VTT Nachführung Komponenten: Optomechanik: Primärspiegel mit radialer Bahnführung
VTT Nachführung Komponenten: Optomechanik: Primärspiegel mit radialer Bahnführung
VTT Nachführung Komponenten: Optomechanik: Sekundärspiegel mit kardanischer Halterung
VTT Nachführung Komponenten: Optomechanik: Auskoppelspiegel mit Halterung (Spinne)
VTT Nachführung Komponenten: Optomechanik: Kreuztisch mit Segment- und Umlenkspiegeln