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Rachel Howe. Why do we need to continue observing? Why ground-based? Requirements for a new...

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HELIOSEISMOLOGY WITH SYNOPTIC NETWORK OBSERVATIONS Rachel Howe
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Page 1: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

HELIOSEISMOLOGY WITHSYNOPTIC NETWORK OBSERVATIONS

Rachel Howe

Page 2: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

SYNOPSIS

Why do we need to continue observing?

Why ground-based? Requirements for a new network

Page 3: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

WHY CONTINUE OBSERVING?

Page 4: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

LONG-TERM VARIATIONS

Dynamics changes – rotation-rate variationsPart of the puzzle for the dynamoUseful for “preview” of activity cycle timing

Page 5: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

LONG-TERM VARIATIONS -- DYNAMICSRotation-rate variations near the tachocline

Page 6: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

TORSIONAL OSCILLATION (LOCAL HELIOSEISMOLOGY)

Torsional oscillation from ring-diagram analysis: MDI-GONG combo that I showed at the AGU meeting. MDI before mid-2001, GONG after. The flows are averaged in depth over 4-10 Mm. Bands of faster (or slower) rotation move toward the equator. The fast band of cycle 24 appears before there is any surface activity present. The new fast band is stronger in the northern hemisphere indicating that the activity will be stronger in this hemisphere.

Courtesy of R. Komm

Page 7: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

Figure 2 from Meridional Circulation During the Extended Solar Minimum: Another Component of the Torsional Oscillation?I. González Hernández et al. 2010 ApJ 713 L16 doi:10.1088/2041-8205/713/1/L16

MERIDIONAL CIRCULATION VARIATION

Temporal variation of the fitted polynomial to the meridional circulation observations at a depth of 5.8 Mm. (Bottom panel symmetrized; poleward velocities positive.)

Page 8: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

FREQUENCY SHIFTS WITH SOLAR CYCLE

ACRIM (Woodard & Noyes 1985, 1988, Gelly, Fossat & Grec 1988)

BiSON, Mark I (Palle et al. 1989, Elsworth et al. 1990)

Chaplin et al. 2007

Page 9: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

ASPHERICITY VARIATIONS

Normalized even-a coefficients vary as Legendre decomposition of magnetic field distribution

Page 10: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

ASPHERICITY VARIATIONS

Normalized even-a coefficients vary as Legendre decomposition of magnetic field distribution – but fit isn’t perfect; residuals correlated between GONG, MDI

Page 11: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

LONG-TERM VARIATIONS (STRUCTURE)

Localized GONG frequency shifts

Page 12: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

WHY GROUND-BASED?

Page 13: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

WHY GROUND-BASED?Redundancy/ease of repair -- lose one site for a few months, still get usable data

Page 14: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

WHY GROUND-BASED?

Longevity

BiSON – courtesy W. Chaplin

Page 15: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

WHY GROUND-BASED?

Redundancy

Page 16: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

REQUIREMENTS FOR A FUTURE NETWORK

Page 17: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

BASIC REQUIREMENTS

Minimum for global: continuation of GONG classic cadence/resolution/duty cycle

For local: > 75% duty cycle, <0.1 deg angular drift Overlap between sites for cross-

calibration Minimum 1-year overlap with

predecessor Improved peak fitting

Page 18: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

MULTI-WAVELENGTH

Work for example with AIA UV intensity has shown how mode behavior varies through the atmosphere

Page 19: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

COHERENCE WITH HMI V

Page 20: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

PHASE RELATIVE TO HMI V

Page 21: Rachel Howe.  Why do we need to continue observing?  Why ground-based?  Requirements for a new network.

POWER MAPS

HMI V

HMI Ic

HMI Lc

AIA 1700

3mHz 5mHz 7mHz


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