1 GONG Magnetogram Data Products. 2 Sky-coordinate images Single-site or merged? –Single-site requires users to select. –Merge has lower noise, may require.

Slides:



Advertisements
Similar presentations
1 GONG Magnetogram pipeline. 2 The GONG Data Processing Pipeline
Advertisements

HMI Data Analysis Software Plan for Phase-D. JSOC - HMI Pipeline HMI Data Analysis Pipeline Doppler Velocity Heliographic Doppler velocity maps Tracked.
Back Reaction on the Photospheric Magnetic field in Solar Eruptions Dandan Ye.
CS 551 / CS 645 Antialiasing. What is a pixel? A pixel is not… –A box –A disk –A teeny tiny little light A pixel is a point –It has no dimension –It occupies.
3/2/2005MUG Meeting, Tucson1 Status of GONG+ Magnetograms How GONG makes magnetograms Performance Problems Solutions Schedule Data availability Pilot Projects.
AGU – Fall 2006 The Solar Polar Field – Cycles 21 – 23 The Solar Polar Field During Solar Cycles J. Todd Hoeksema, Yang Liu, XuePu Zhao & Elena Benevolenskaya.
A particularly obvious example of daily changing background noise level Constructing the BEST High-Resolution Synoptic Maps from MDI J.T. Hoeksema, Y.
September 2006 CISM All Hand Meeting Progress in the Past Year and Plan for Next Year Yang Liu and the Solar Group in Stanford University
1Yang LiuCISM All-hand meeting CISM All-hand Meeting Yang Liu – Stanford University
Recent ILCT Results & LCT Pipeline The UCB-MURI, UCB-CISM, SOHO/MDI, SOLIS, & GONG Teams!
Source detection at Saclay Look for a fast method to find sources over the whole sky Provide list of positions, allowing to run maximum likelihood locally.
HMI MDI Comparison Y. Liu. CR 2104 CR 2109 MDI = 1.2 * HMI 720s / 45s.
Helioseismic Holography & some experiments on “field effects” in CR1988 NorthWest Research Associates Colorado Research Associates Division D. Braun.
A particularly obvious example of daily changing background noise level Constructing the BEST High-Resolution Synoptic Maps from MDI J.T. Hoeksema, Y.
3D full object reconstruction from kinect Yoni Choukroun Elie Semmel Advisor: Yonathan Afflalo.
SPD – June 2006 Solar Polar Flux – MDI The Sun’s Polar Magnetic Flux Observed with SOHO/MDI J. Todd Hoeksema E.E. Benevolenskaya,
Instrumental & Technical Requirements. Science objectives for helioseismology Understanding the interaction of the p-mode oscillations and the solar magnetic.
Seething Horizontal Magnetic Fields in the Quiet Solar Photosphere J. Harvey, D. Branston, C. Henney, C. Keller, SOLIS and GONG Teams.
1 Status of Ring-diagram Analysis of MOTH Data Kiran Jain Collaborators: F. Hill, C. Toner.
F. I. Suárez-Sol á 1, E. González-Suárez 1, I. González-Hernández 1, A.R. Davey 2,J. Hourcl é 3, VSO Team 1 National Solar Observatory, Tucson AZ – 2 Harvard-Smithsonian.
7/12/20011 Observing Sequences in View of the SECCHI Science Goals From the EUVI Perspective J-P. Wülser.
Magnetogram Users Group Role of the MUG –Charge –Functioning –Agenda Scientific Objectives & Functional Requirements –One person's noise is another’s signal.
Sky Coordinate Image Specs Fully processed: –Merged –10-min cadence –“sky to sky” interpolation –Gaussian temporal filter –Renormalized such that time.
P MODE TRAVEL TIME IN ACTIVE REGIONS USING TIME-DISTANCE METHOD CRAAG, Observatory of Algiers, BP 63 Bouzareah 16340, Algiers, Algeria. (1)
GONG data and pipelines: Present & future. Present data products 800x800 full-disk images, one per minute, continuous (0.87 average duty cycle) Observables:
Regional climate prediction comparisons via statistical upscaling and downscaling Peter Guttorp University of Washington Norwegian Computing Center
Lecture 4: Image Resampling and Reconstruction CS4670: Computer Vision Kavita Bala.
GONG Magnetograms - Raw to Synoptic Map J. Harvey.
Comparing and Ordering Decimals. Using Models If you are comparing tenths to hundredths, you can use a tenths grid and a hundredths grid. Here, you can.
1 Zero Point Correction. 2 Basic Steps - I For a given site on a given day: 1.Create a magnetic flat field from the east & west calibration images. 2.Using.
Aquarius Level-3 Binning and Mapping Fred Patt. Definitions Projection - any process which transforms a spatially organized data set from one coordinate.
Contents of the Site On the MY NASA DATA homepage you can find: Data Access Lesson Plans Computer Tools Science Focus E-Notes.
VARIABILITY OF TOTAL ELECTRON CONTENT AT EUROPEAN LATITUDES A. Krankowski(1), L. W. Baran(1), W. Kosek (2), I. I. Shagimuratov(3), M. Kalarus (2) (1) Institute.
1 Synoptic Maps of Magnetic Field from MDI Magnetograms: polar field interpolation. Y. Liu, J. T. Hoeksema, X. P. Zhao, R. M. Larson – Stanford University.
Opportunities for Joint SOT – Ground Based Observations Using NSO/Tucson Facilities J. Harvey, NSO.
Slide 1 NATO UNCLASSIFIEDMeeting title – Location - Date Satellite Inter-calibration of MODIS and VIIRS sensors Preliminary results A. Alvarez, G. Pennucci,
Holography far-side images with HMI Irene Gonzalez Hernandez Charlie Lindsey Richard Bogart Phil Scherrer Sebastian Couvidat, and the calibration team.
Kitt Peak Vacuum Telescope -- Raw to Synoptic Map J. Harvey.
Krivljenje slike - warping. Princip 2D krivljenja Demo.
(c) 2002 University of Wisconsin, CS 559
Three-Dimensional Power Spectra of GONG++ High- Cadence Magnetograms F. Hill, J. Bolding, R. Clark, K. Donaldson-Hanna, J. Harvey, G. Petrie, C. Toner.
Synoptic Chart of Magnetic Field from MDI Magnetograms J. T. Hoeksema, Y. Liu, X.P. Zhao, A. Amezcua – Stanford University
Solar X-ray Imager (SXI) Current and Future Requirements 22 May 2001 Steve Hill Solar Causes and Effects... Operational Requirements Improvements for GOES-R+
GONG Time distance pipeline status Shukur Kholikov.
SHINE August, 2006 C.J. Henney (NSO/SOLIS) SOLIS/VSM Coronal Hole Estimation Maps Carl J. Henney (NSO/SOLIS)
MHD model in HMI pipeline HMI/AIA science team meeting Sep , 2009 Stanford, CA HMI/AIA science team meeting Sep , 2009 Stanford, CA.
SOLIS-VSM Magnetic Synoptic Maps
Spatial Image Enhancement
Mapping the Solar Magnetic Surface (a la Worden & Harvey)
Studies on Twisted Magnetic Flux Bundles
“Old” data – new science or why do we need long-term synoptic programs
GONG Measurements – Pre-eruptive signatures
Observables codes: written by Richard, Jesper, and Sebastien
Image Pre-Processing in the Spatial and Frequent Domain
M15672: View synthesis software and assessment of its performance
PSP, SO, and Ground-based Synoptic Observations from NSO
New Iterative Method of the Azimuth Ambiguity Resolution
Carrington Rotation 2106 – Close-up of AR Mr 2106 Bt 2106
Scale: Kilometers.
HMI Data Analysis Pipeline
The Moat Flow Observed in Two Different TRACE-Filters
HMI Data Analysis Pipeline
Non-local Means Filtering
Questions/avenues to be addressed by all of the instrument-related sessions throughout this day: How well can we define, observe, and measure those phenomena.
Filtering Images Work in the spatial domain
Scale: Kilometers.
Data search & distribution
Apex scanning strategy & map-making
Automated Detection and Analysis of Ca2+ Sparks in x-y Image Stacks Using a Thresholding Algorithm Implemented within the Open-Source Image Analysis Platform.
Olga Burtseva and Shukur Kholikov (NSO/GONG)
Presentation transcript:

1 GONG Magnetogram Data Products

2 Sky-coordinate images Single-site or merged? –Single-site requires users to select. –Merge has lower noise, may require site- specific correction to reduce jumps as stations change. At what cadence? –1 min – highest cadence, most noise. –3 min or 5 min – compromises. –10 min – lowest cadence, least noise, rotational smearing starts to be a concern. Rotational smearing correction? How? –Rotation crosses 1 pixel at disk center in about 15 min. –Remap and average in heliographic coordinates, transform back to sky. What temporal filter/averaging algorithm? –Simple box car. –Hathaway filter (Gaussian). –Will need to specify width in any case.

3 Remapped images Same questions as for sky images: –Single-site/merged –Cadence –Rotational smearing easy to deal with –Temporal filter What spatial resolution for remapped images? –Currently 0.2° What projection for remapped images? –Currently longitude - sine latitude

4 Synoptic Maps Single-site or merged? At what cadence –Trade-off between effort and science: What’s rapid enough for space weather? –1, 2, 4, 8 hours? How to interact with SOLIS cadence? –Identical times for comparison? –Different times to fill in temporal gaps ? How to treat poles, projection of LOS, missing data?