'Hmi data' diaporamas de présentation

Sarbani Basu Yale Unoversity

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Helioseismic and Magnetic Imager hmi.stanford

Helioseismic and Magnetic Imager http://hmi.stanford.edu. LWS-SDO Workshop 23-26 March 2004. Philip Scherrer pscherrer@solar.stanford.edu. HMI Investigation Overview. Investigation Overview Science Objectives Data Products and Objectives Data Product Examples

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UK E-Science Initiative and its Application to SDO

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HMI Data Products: Plan and Status

HMI Data Products: Plan and Status. Primary goal: origin of solar variability.

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HMI Investigation Overview

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Using HMI to Understand Flux Cancellation

Cancellation of magnetic flux in magnetograms has been defined in observational terms as "the mutual apparent loss of magnetic flux in closely spaced features of opposite polarity."

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Resolving the 180 Degree Ambiguity in Vector Magnetic Fields

Resolving the 180 Degree Ambiguity in Vector Magnetic Fields. T. Metcalf. The Transverse field is Ambiguous by 180 Deg. This ambiguity must be resolved before analysis. Ambiguity Resolution is Required to Compute Correct Neutral Lines. From K.D. Leka. N22 E20. 2000 Jun 05.

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Algorithm Preparation and Data Availability

for the SDO Investigations in the Context of the UK Virtual Observatory J.L. Culhane 1 , E.C. Auden 1 , Y.P. Elsworth 2 , R.A. Harrison 3 , M.J. Thompson 4. SDO Data on the Grid

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HMI Major Science Objectives

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HMI Major Science Objectives

The Helioseismic & Magnetic Imager on the Solar Dynamics Observatory. HMI Data Processing. Data Product. HMI Data. Internal rotation ?(r,?) (0<r<R). Spherical Harmonic Time series To l =1000. Heliographic Doppler velocity maps. Filtergrams.

102 views • 1 slides