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Items: 7

1.

Shape of a slowly rotating star measured by asteroseismology.

Gizon L, Sekii T, Takata M, Kurtz DW, Shibahashi H, Bazot M, Benomar O, Birch AC, Sreenivasan KR.

Sci Adv. 2016 Nov 16;2(11):e1601777. doi: 10.1126/sciadv.1601777. eCollection 2016 Nov.

2.

Helioseismic Holography of Simulated Sunspots: dependence of the travel time on magnetic field strength and Wilson depression.

Felipe T, Braun DC, Birch AC.

Astron Astrophys. 2017;604. pii: A126. doi: 10.1051/0004-6361/201730798. Epub 2017 Aug 25.

3.

HELIOSEISMIC HOLOGRAPHY OF SIMULATED SUNSPOTS: MAGNETIC AND THERMAL CONTRIBUTIONS TO TRAVEL TIMES.

Felipe T, Braun DC, Crouch AD, Birch AC.

Astrophys J. 2016 Oct 1;829(No 2). pii: 67. doi: 10.3847/0004-637X/829/2/67. Epub 2016 Sep 23.

4.

A low upper limit on the subsurface rise speed of solar active regions.

Birch AC, Schunker H, Braun DC, Cameron R, Gizon L, Löptien B, Rempel M.

Sci Adv. 2016 Jul 13;2(7):e1600557. doi: 10.1126/sciadv.1600557. eCollection 2016 Jul.

5.

EVALUATION OF THE CAPABILITY OF LOCAL HELIOSEISMOLOGY TO DISCERN BETWEEN MONOLITHIC AND SPAGHETTI SUNSPOT MODELS.

Felipe T, Crouch AD, Birch AC.

Astrophys J. 2014;788(No 2). pii: 136. doi: 10.1088/0004-637X/788/2/136. Epub 2014 Jun 2.

6.

Helioseismology challenges models of solar convection.

Gizon L, Birch AC.

Proc Natl Acad Sci U S A. 2012 Jul 24;109(30):11896-7. doi: 10.1073/pnas.1208875109. Epub 2012 Jul 18. No abstract available.

7.

Heartburn and waterbrash.

BIRCH AC.

Practitioner. 1955 Jan;174(1039):105-7. No abstract available.

PMID:
13224591

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