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Spectrometer HELLRIDE as a Testing Ground for Fulldisk Velocity Mapping Joachim Staiger, KIS Freiburg. - HELLRIDE Overview First Observations at VTT 2013 Problems Ongoing Development Fulldisk „Lab“ Fulldisk Tests 2014. HELLRIDE Overview.
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SpectrometerHELLRIDEas a TestingGround forFulldiskVelocity Mapping Joachim Staiger, KIS Freiburg • - HELLRIDEOverview • First Observationsat VTT 2013 • Problems • Ongoing Development • Fulldisk „Lab“ • Fulldisk Tests 2014
HELLRIDEOverview Instrument Type: 2D Fabry-Perot Spectrometer Operation Focus: Multiline Operation 16 Bands available 100“-by-100“ FOV standard 300“-by-300“ synthetic Fulldisk ?
HELLRIDEOverview HELLRIDEstandsfor HELioseismologicalLarge RegionsInterferometricDevice
HELLRIDEOverview Scientific Target: - AnalysingWaves in theAtmosphere - AnalysingFlares Requirements: - Long Recording Times Oportunity: - Future VTT Usage
HELLRIDEOverview Development Goals - Simple Design - Easy Handling - Step-by-Step Approach - Costeffective Approach (Stock / Scrap)
HELLRIDEOverview Optical Layout - Dual Etalon Tandem Configuration - Collimated Beam Design
HELLRIDEOverview Etalons - IC Optical EC50 and EC70 - 530 nm – 860 nm
HELLRIDEOverview Narrowband Filter Mount - 4 x 4 Matrix - 0.5 μRepositioning
HELLRIDEOverview Narrowband Filter Mount - 4 x 4 Matrix - 0.5 μRepositioning
HELLRIDEOverview NarrowbandDetector - Dalsa 1M30 CCD - 14 μ Pixel Square - 4-Axis Mount
HELLRIDEOverview „Onboard“ Software - System Simulation - Data Quicklook - Ringdiagramm Pipeline (64 x 64)
HELLRIDEOverview Status: Installedat VTT since 2013
First Observations 2013 Campaign 1: A. Wisniewska (April, 6 Days) Campaign 2: A. Wisniewska (September, 6 Days) Sunspot / Quiet Sun 2 SpectralLines (5434 / 5890) Cadence 15 secs 10 Hour Records
First Light Results 2013, A.Wisniewska Linear Powerspectrum, 2 Hours, 5434 Angstr. Pixel Average
First Light Results 2013, A.Wisniewska Ringdiagram 64x64, 8 Hours 5434 Angstr., 3.0 mHz
First (andonly) Multiline Test 2009 Multiline Ringdiagramms 4 Hours, 60 secsCadence, 16 Lines Using GFPI Etalons 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
First (andonly) Multiline Test 2009 Multiline Ringdiagramms 4 Hours, 60 secsCadence, 16 Lines Using GFPI Etalons
Problems andShortcomings Crash after appr. 2 hours:Resolved - Axis 2 Malfunction:Not yetresolvedSpring 2014 Graphics Overload: Not yetresolvedSpring 2014 Camera Upgrade: Not yetresolvedAutumn 2014 Outdated VTT Handling UnderdevelopmentSpring 2014 Environmental Exposure:Not yetresolved2014 / 2015 Image Motion: Not yetresolvedSpring 2015 Lateral FOV DriftsUnderdevelopment2015 / 2016 Data Processing Software: Underdevelopment2015
Problems andShortcomings • Pending Tasks: • Update: Aging Components • Camera System • Computing • Reduce: Thermal Exposure • Straylight • Seeingbased Image Motion • PointingInstabilities
Developments Encasement - Shield off Dust - Shield off Straylight - ReduceTemperatureFluctuations
Developments High Speed Drives - Norotating Parts - Moving EM Field - 10 G Acceleration -
Developments TabletUsage - Versatility - Hardware Reduction - Remote Handling
Developments RealtimeVelocity Mapping - EnableRealtime Ringdiagram-Pipeline - Reduce Data Storage Bottleneck - Enable Remote Operations - Offline Tests Successful - Calibrationwith SDO Pending - Will beimplementedas an Observers Option
Developments Doppler Signal Locking - Laser attachedto Matrix Mount - Continuous Laser Line Scanning
Developments Doppler Signal Locking - Laser attachedto Matrix Mount - Continuous Laser Line Scanning
Developments Doppler Signal Locking - UsingFrequencystabilized Laser (< 3 MHz) - Drift < 2 m/sec, 8 hours - Realtime Peak Location Processing - Feedback to Etalons
Developments New Finesse Calibration - Adust Etalon Plate Parallelity - StabilizeWavelengthPurity
Developments New Finesse Calibration - Adust Etalon Plate Parallelity - StabilizeWavelengthPurity
Developments New Spectroscopic Tracking Problem: - Image Motion - No AO Usageover 10 hours. Solution: - SpectroscopicCorrelation - Individual Wavelength Tracking - OverlayWavelengths
Developments Remote Control Motivation: Off-Lab Monitoring Remote Maintenance Staff Limited Operation Automated Operation Realization: TCP/IP Sockets Client / Server Architecture ASCII Commands
Developments Full Disk Velocity Mapping Tests Goals: - EvaluateExposure Times - Evaluate Scan StepRequirements - EvaluateReadout Options - Evaluate Multiline Options - EvaluateFulldisk / Subfield-Tiling - Test Flat Procedures - Compareto SDO /GONG - Extrapolatefrom 5 cm to 50 cm Aperture
Developments New Absolute Pointing Existing Problem: - ThermallyrelatedDrifts
Developments New Absolute Pointing Thermal Drifts: - May Influence Co-Alignment - May influence Data Analysis - Is InherentPointingShortcoming
Developments New Absolute Pointing Thermal Drifts: - May Influence Co-Alignment - May influence Data Analysis - Is InherentPointingShortcoming
Developments New Absolute Pointing Thermal Drifts: - May Influence Co-Alignment - May influence Data Analysis - Is InherentPointingShortcoming
Developments New Absolute Pointing Thermal Drifts: - May Influence Co-Alignment - May influence Data Analysis - Is InherentPointingShortcoming
Developments New Absolute Pointing Goal: - Develop New Pointing Model
Developments New Absolute Pointing Approach: - GuidingTelescopeis Imaging Telescope - Pointingisof Barcode Type Reading
Developments New Absolute Pointing Tests: - VTT / SDO 2012 - VTT / GONG 2012 - VTT / SUMER / IRIS 2013
Developments New Absolute Pointing Benefits: - Delivering absolute Coordinatescontinuously - First Primary Beam Closed-Loop Operation - SignificantStabilityImprovement - No rigid Link betweenGuidingand Main Telescope - Multiple Telescopes maysharesingleGuidingTelescope - Single Telescopemayuse Multiple Guiding Telescopes - Minimum Engineering required - Off-the-Shelf Components maybeused.
Fulldisk „Laboratory“ Usage: - New Pointing - HELLRIDE Fulldisk Tests - IAC Coelo Test (Solar Orbiter) ?
Fulldisk „Laboratory“ Locations: Fulldisk „Lab“ HELLRIDE
Fulldisk „Laboratory“ Test Setup 2012: - Setup HELLRIDE Data Aquis. System - DivertGuiding Beam toDalsa - Fit Sun toDetector - RecordFulldiskat Short Cadence
Fulldisk „Laboratory“ Test Setup 2012:
Fulldisk „Laboratory“ Test Setup 2012: Problems: - Mounting / Dismountingrequired - Vertical Optical Axis - „Transit“-Area
Fulldisk „Laboratory“ New Setup 2013 / 2014:
Fulldisk „Laboratory“ New Setup 2013 / 2014:
Fulldisk „Laboratory“ New Setup 2013 / 2014:
Fulldisk „Laboratory“ New Setup 2013 / 2014:
Fulldisk „Laboratory“ New Setup 2013 / 2014: - SecludedLocation off „Transit“-Area - BeamsplitterinsteadofMirror - Continuous Operation - Horizontal Optical Bench - Elevator Access („HELLRIDE Drive-In“) - Standard HELLRIDESoftware maybeused - Retrofit time appr. 1 – 2 hours