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|---|---|---|
 Date: 2008-11-26 12:17:31National Science Foundation Science Sun National Optical Astronomy Observatory Global Oscillations Network Group Solar Observing Optical Network National Solar Observatory Air Force Weather Agency Magnetogram Astronomy Solar telescopes Space |
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Graph0_wave1 vs wave0;... | A Potential New Method for Measuring the Solar Diameter Changes with Time Distance Helioseismology A.V. Serebryanskiy1 and Sh.S. Kholikov1 and GONG team 1 National Solar Observatory, Tucson, AZ, USDocID: 114u3 - View Document |
| Searching for GONG p-Mode Frequency Variations Generated by Perturbations Near the Base of the Convection Zone Serebryanskiy A.V.1 , Chou Dean-Yi 2DocID: 10VVy - View Document |
| NSO | National Solar Observatory NSO News & Announcements ATST Awaits Final Decision The ATST TeamDocID: 1028p - View Document |
| GONG Global Oscillation Network Group GONG John LeibacherDocID: 100vf - View Document |
| GLOBALOSCILLATIONNETWORKGROUP EL TEIDE • UDAIPUR • LEARMONTH • MAUNA LOA • BIG BEAR • CERRO TOLOLO GONG John Leibacher & the GONG TeamDocID: ZY0D - View Document |