Kitt Peak Vacuum Telescope -- Raw to Synoptic Map J. Harvey.

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Kitt Peak Vacuum Telescope -- Raw to Synoptic Map J. Harvey

Transcript of Kitt Peak Vacuum Telescope -- Raw to Synoptic Map J. Harvey.

Page 1: Kitt Peak Vacuum Telescope -- Raw to Synoptic Map J. Harvey.

Kitt Peak Vacuum Telescope --Raw to Synoptic Map

J. Harvey

Page 2: Kitt Peak Vacuum Telescope -- Raw to Synoptic Map J. Harvey.

Pre-History

• KP 40-channel collected daily FD maps in March 1970 to compare with corona at eclipse

• Randy Levine worked with Marty Altschuler at HAO to make synoptic map and extrapolations; did it again in 1972

• Skylab prompted start of daily observations in 1973 & construction of KPVT

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First KP Synoptic Map – CR 1558

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More History

• Synoptic map algorithm was basically derived from Randy’s HAO work

• 1974: 40-chan replaced with 512-chan

• 1974: Started doing helium 10830 maps

• 1993: 512-chan replaced by SPMG

• 2003: KPVT replaced by SOLIS VSM

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512-ch Calibration

• It was an array of Babcock magnetographs

• Calibrated with circular polarizer + known displacement

• 8688 Å linear response to ~9000 G

• Not much center – limb variation

• Calibration done very rarely

• Observations sensitive to I & vel crosstalk

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SPMG Calibration

• Used TV images of polarized spectra

• Still used 8688 Å (small disk variation)

• Uses whole line profile so Zeeman displacement measured directly

• Vulnerable to modulator efficiency being less than 100%

• Did a cross-comparison between 512 for ~9 months

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Synoptic Map Basic Recipe

1. Clean up full-disk image• Filter noisy pixels • Geometric fit (P-angle, disk center and radius)• Adjust zero point (if needed)• Multiply by sec ρ

2. Map to Carrington coordinates (sin B, CMD)• 3 resolutions: 180 x 180, 360 x 360, 900 x 900• 2 maps: sum and weight• Flux conserved

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Recipe – con’t.

3. Weighted merge of images– Cos4 CMD for low resolution– 1-D gaussians in CMD for higher resolution– Build sum and weight merged images– Divide merged sum by weight

4. Pole correction

5. Publish– Done for B and |B|

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Pole Correction

• Remap pole region to polar coordinates

• Iterative fit of 2-D 5th-order cubic spline to measured data (rejects wild points)

• Replace missing and noisy pixels with fit

• Map back to Carrington grid

• Latitude-dependent blend with original map

• Tested by absence of annual signal

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Variants

1. Snapshot maps started in 1998 until Y2K2. Polar projections3. Daily difference maps4. CR difference maps5. Neutral line and AR summaries6. Movies7. Butterfly diagrams8. Coronal holes

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Problems

• Assumes each image is instantaneous• Except for the snapshot maps, does not

represent the full solar surface at any specific time

• Dubious polar correction• Dark umbras poorly handled• Leaves a small monopole• Radial correction is bad in AR• Bad in quiet photosphere, too

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Status

• Old KPVT mags have been cleaned up

• New set of synoptic maps from CR 1625-2007 about to be prepared