Search Publications

Comparison of HMI Dopplergrams with GONG and MDI data
DOI: 10.1088/1742-6596/271/1/012060 Bibcode: 2011JPhCS.271a2060H

Howe, R.; Komm, R.; Hill, F. +3 more

We compare sample Dopplergrams from the Helioseismic and Magnetic Imager, the Michelson Doppler Imager and the Global Oscillation Network Group. Each instrument has a distinct static velocity patterm across the disk; once this has been subtracted and the images interpolated to a common grid, the agreement is satisfactory.

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 3
Progress in sunspot helioseismology
DOI: 10.1088/1742-6596/271/1/012001 Bibcode: 2011JPhCS.271a2001B

Birch, A. C.

Local helioseismology is a set of methods that are used to study wave propagation and infer physical conditions in the solar interior. Sunspots are a particularly challenging target for local helioseismology. In this review, I will show that some new methods (magnetoconvection simulations and numerical wave propagation simulations) lead to shallow…

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 3
Temporal Variations of High-Degree Solar p-Modes from GONG and MDI
DOI: 10.1088/1742-6596/271/1/012012 Bibcode: 2011JPhCS.271a2012B

Howe, Rachel; Hill, Frank; Jain, Kiran +4 more

We study temporal variations in the amplitudes and widths of high-degree acoustic modes in the quiet and active Sun by applying ring-diagram technique to the GONG+ and MDI Dopplergrams during the declining phase of cycle 23. The increase in amplitudes and decrease in line-widths in the declining phase of the solar activity is in agreement with pre…

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 3
Angular-degree dependence of p-mode frequencies during solar cycle 23
DOI: 10.1088/1742-6596/271/1/012055 Bibcode: 2011JPhCS.271a2055T

Hill, F.; Salabert, D.; Garcia, R. A. +3 more

We analyze simultaneous helioseismic observations collected by the ground- and space-based instruments during solar cycle 23 by computing oscillation frequencies for low- and intermediate-degree p-modes on a time scale of 36 days. We find that the frequency shifts corresponding to different angular degree, ell, indicate different epochs for the on…

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 3
Localized averaging kernels for probing the deep meridional flow with data from GONG, MDI and HMI
DOI: 10.1088/1742-6596/271/1/012057 Bibcode: 2011JPhCS.271a2057D

Roth, M.; Doerr, H. -P.

The Fourier-Legendre decomposition (FLD) method to study wave absorption in sunspots is a helioseismic technique which is also suited for the measurement of the meridional flow. Because the FLD method is sensible to low-degree oscillation modes, it bears the potential to be used to probe the average meridional flow in much deeper layers as it is c…

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 3
The Need for Physics-based Inversions of Sunspot Structure and Flows
DOI: 10.1088/1742-6596/271/1/012010 Bibcode: 2011JPhCS.271a2010B

Birch, A. C.; Braun, D. C.; Crouch, A. D. +1 more

Current controversy exists in the interpretation and modeling of helioseismic signals in and around magnetic regions like sunspots. Unresolved issues include the dependence of the sign of both the inferred flows and wave speed on the type of filtering used, and the discrepancy between the relatively deep two-layer wave-speed models derived from st…

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 3
Characteristics of Solar Meridional Flows
DOI: 10.1088/1742-6596/271/1/012071 Bibcode: 2011JPhCS.271a2071B

Basu, Sarbani; Antia, H. M.

We have done a ring-diagram analysis of MDI full-disc data to determine the properties of solar meridional flow in the outer 2% of the Sun over the solar cycle 23. The meridional flows show a migrating pattern with higher-velocity flows migrating toward the equator as activity increases. Additionally, we find that the migrating pattern of the meri…

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 2
Variation of high-degree mode frequencies during the declining phase of solar cycle 23
DOI: 10.1088/1742-6596/271/1/012024 Bibcode: 2011JPhCS.271a2024T

Hill, F.; Jain, K.; Tripathy, S. C.

We investigate the spatial and temporal variation of the high-degree mode frequencies during the declining phase of the solar cycle 23 and the extended minimum between the cycle 23 and 24. We find that the frequency shifts of high-degree modes obtained through the ring-diagram analysis in different phases of the solar cycle are not equally correla…

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 2
Investigating the correlation between high-frequency global oscillations and solar flares
DOI: 10.1088/1742-6596/271/1/012048 Bibcode: 2011JPhCS.271a2048C

Rabello-Soares, M. C.; Bogart, R. S.; Chakraborty, S. +1 more

Global oscillations have been observed in the high-frequency spectrum in velocity and intensity measurements above the acoustic cutoff frequency of the solar atmosphere. In a recent work, strong correlation at high frequencies, determined between helioseismic spectra and soft x-ray flux has been cited as evidence that solar flares may be one of th…

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 2
A search for coherent structures in subsurface flows
DOI: 10.1088/1742-6596/271/1/012065 Bibcode: 2011JPhCS.271a2065K

Howe, R.; Komm, R.; Hill, F.

We search for coherent patterns in horizontal subsurface flows obtained from Global Oscillation Network Group (GONG) Dopplergram data using ring-diagram analysis. The existence of north-south aligned downflow patterns near the equator has been predicted by numerical models of the solar convection zone. We analyze time series of daily flow measurem…

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 2